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hepal's Introduction

HEPAL

This is a list of acronyms, abbreviations and similar stuff that I've had to look up or remember over the years, mostly due to reading hep-lat, hep-ph and hep-th arXiv postings. It is organized alphabetically rather than thematically. Fermilab and CTEQ have similar lists here and here.

This basic list has largely been superseded by the High Energy Physics Acronym Dictionary constructed by Casper van Veen and Ilya Fokin, but will continue to be updated on occasion.

#

  • 2DEG: Two-dimensional electron gas
  • 2dFGRS: Two-degree-Field Galaxy Redshift Survey
  • 2MASS: Two Micron All-Sky Survey
  • 2MRS: 2MASS redshift survey
  • 2p2h: Neutrino interactions with two nucleons producing two holes
  • 2SC: Two-flavor color superconducting phase
  • 3FD: Three-fluid dynamics
  • 3VIL: Three-loop Vacuum Integral Library
  • 6dF: 6 degree Field Galaxy Survey

A

  • AAdS: Asymptotically anti-de Sitter
  • AAMQS: Albacete, Armesto, Milhano, Quiroga-Arias and Salgado
  • AARM: Assay and Aquisition of Radiopure Materials
  • AB: Aharonov and Bohm
  • ABC: Abashian, Booth and Crowe
  • ABDK: Anastasiou, Bern, Dixon and Kosower
  • ABJ: Adler, Bell and Jackiw
  • ABJM: Aharony, Bergman, Jafferis and Maldacena
  • ABKM: Alekhin, Blümlein, Klein and Moch
  • ABMP: Alekhin, Blümlein, Moch and Placakyte parton distribution functions
  • ABM: Alekhin, Blümlein and Moch parton distributions
  • ABRACADABRA: A Broadband/Resonant Approach to Cosmic Axion Detection with an Amplifying B-field Ring Apparatus
  • ACAT: Advanced Computing and Analysis Techniques in Physics Research
  • ACBAR: Arcminute Cosmology Bolometer Array Receiver
  • ACD: Appelquist, Cheng and Dobrescu
  • ACES: Alliance for Computing at Extreme Scale partnership between Los Alamos and Sandia
  • ACM: Anomalous chromomagnetic moment
  • ACM: Association for Computing Machinery
  • ACME: Advanced Cold Molecule Electron electric dipole moment experiment
  • ACOT: Aivazis, Collins, Olness and Tung renormalization scheme
  • ACT: Atacama Cosmology Telescope
  • ACTpol: Atacama Cosmology Telescope Polarimeter
  • AD: Affleck and Dine
  • ADD: Arkani-Hamed, Dimopoulos and Dvali
  • ADE: Dynkin diagrams with only single lines; see page 252 of Georgi
  • ADHM: Atiyah, Drinfeld, Hitchin and Manin construction of instantons
  • ADI: Alternating direct implicit methods
  • ADM: Arnowitt, Deser and Misner formalism of general relativity
  • ADMX: Axion Dark Matter eXperiment
  • AEGIS: Antimatter Experiment: Gravity, Interferometry, Spectroscopy at CERN
  • AFM: Atomic force microscopy
  • AFTER: A Fixed Target ExpeRiment at the LHC
  • AFZ: Arutyunov, Frolov and Zamaklar
  • AGASA: Akeno Giant Air Shower Array
  • AGE: Antimatter Gravity Experiment
  • AGILe: A Generator Interface Library (and executable) for Monte Carlo event generators
  • AGIS: Advanced Gamma-ray Imaging System
  • AGK: Abramovsky, Gribov and Kancheli
  • AGN: Active galactic nuclei
  • AGS: Alternating Gradient Synchrotron
  • AGSS: Asplund, Grevesse, Sauval and Scott
  • AGT: Alday, Gaiotto and Tachikawa duality
  • AICS: RIKEN Advanced Institute for Computational Science
  • AION: Atom Interferometer Observatory and Network for ultra-light dark matter and gravitational waves
  • AIRES: AIR-shower Extended Simulations system
  • AIT: Advanced Instrumentation Testbed at Boulby Underground Laboratory, North Yorkshire
  • aITALC: an Integrated Tool for Automating Loop Calculations
  • AKNS: Ablowitz, Kaup, Newell and Segur
  • AKSZ-BV: Alexandrov, Kontsevich, Schwarz, Zaboronsky, Batalin and Vylkovisky
  • AL3X: A Laboratory for Long-Lived eXotics proposed LHC detector near ALICE
  • ALFA: Arecibo L-band Feed Array
  • ALICE: A Large Ion Collider Experiment
  • ALICE: Accelerators and Lasers In Combined Experiments at Daresbury, formerly ERL
  • ALICE: Imaging spectrograph aboard the New Horizons mission, not an acronym but sometimes treated as such
  • ALMA: Atacama Large Millimeter Array run by the NRAO
  • ALE: Arbitrary Lagrangian--Eulerian techniques
  • ALE: Asymptotically locally Euclidean
  • ALEPH: Apparatus for LEP PHysics
  • ALF: Asymptotically locally flat
  • ALLM: Abramowicz, Levin, Levy and Maor parameterization of the structure function F2
  • ALP: Axion-like particle
  • ALPGEN: A generator for hard multiparton processes in hadronic collisions, apparently not an acronym
  • ALPHA: Antihydrogen experiment at CERN
  • ALPS: Algorithms and Libraries for Physics Simulations
  • ALPS: Axion-Like Particle Search (or Any Light Particle Search) at DESY
  • ALR: Alternative left-right scenario
  • AMANDA: Antarctic Muon And Neutrino Detector Array
  • AMBER: Apparatus for Meson and Baryon Experimental Research proposed at CERN
  • AMBRE: Automatic Mellin-Barnes Representation (Mathematica package)
  • aMC@NLO: Automated MC@NLO code, apparently independent of MC@NLO itself
  • aMCfast: Interface between MadGraph5_aMC@NLO and APPLgrid
  • AMIAS: Athens Model-Independent Analysis Scheme for excited states in two-point functions
  • AMIDAS: A Model-Independent Data Analysis System for direct dark matter detection experiments
  • AMPT: A Multi-Phase Transport model for hadrons
  • AMS: Alpha Magnetic Spectrometer on the International Space Station
  • AMY: Arnold, Moore and Yaffe
  • ANAIS: Annual modulation with NaI Scintillators dark matter search project
  • ANDES: Agua Negra Deep Experiment Site
  • ANITA: Antarctic Impulsive Transient Antenna
  • ANKE: Apparatus for Studies of Nucleon and Kaon Ejectiles at the Jülich Cooler Synchrotron
  • ANL: Argonne National Laboratory
  • ANN: Artificial Neural Network
  • ANP: Adler, Nussinov and Paschos pion leptoproduction model
  • ANTARES: Astronomy with a Neutrino Telescope and Abyss environmental RESearch
  • APCTP: Asia Pacific Center for Theoretical Physics
  • APE: Array Processor Experiment
  • APEX: A-Prime EXperiment at Jlab
  • APFEL: A Parton distribution Function Evolution Library
  • APPEC: Astroparticle Physics European Consortium
  • APPLgrid: Code to quickly reproduce NLO results, apparently not an acronym
  • APT: Analytic Perturbation Theory
  • ARC: Applied Research Center at JLab
  • ARCA: Astronomy Research with Cosmics in the Abyss under construction as part of KM3NeT
  • ARCADE: Absolute Radiometer for Cosmology, Astrophysics and Diffuse Emission
  • ARES: Automated Resummer for Event Shapes semi-numerical approach
  • ARGO-YBJ: Astrophysical Radiation with Ground-based Observatory at YangBaJing
  • ArgoNeuT: Argon Neutrino Test project at Fermilab
  • ARGUS: A Russian--German--United States--Swedish Collaboration at DORIS
  • ARNPS: Annual Review of Nuclear and Particle Science
  • ARPA-E: Advanced Research Projects Agency-Energy
  • ARPES: Angle-resolved photoemission spectroscopy
  • ART: A Relativistic Transport model for hadrons
  • ASACUSA: Atomic Spectroscopy And Collisions Using Slow Antiprotons experiment at CERN
  • ASC: Advanced Simulation and Computing at Livermore
  • ASCR: Advanced Scientific Computing Research program of the DOE
  • ASD: Anti-self-dual
  • ASEP: Asymmetric simple exclusion process
  • ASIC: Application-specific integrated circuit
  • ASTROD: Astrodynamical Space Test of Relativity using Optical Devices
  • AT: Astronomical Transient (e.g., AT2017gfo)
  • ATCA: Australia Telescope Compact Array
  • ATF: Accelerator Test Facility at KEK
  • ATHENA: Antihydrogen experiment at CERN
  • ATHOS: Analysis Tools for next generation Hadron Spectroscopy
  • ATIC: Advanced Thin Ionization Calorimeter
  • ATK: Atomistix ToolKit Python programming environment
  • ATLAS: A Toroidal LHC ApparatuS at CERN
  • ATMNC: ATmostpheric Muon Neutrino Calculation
  • ATNF: Australia Telescope National Facility
  • AUC: Area Under the [receiver operating characteristic] Curve machine learning performance measure
  • AUT: Single-spin target Asymmetry with Unpolarized beam and Transversely polarized target
  • AVX: Advanced vector extensions
  • AWAKE: Advanced proton driven plasma Wakefield acceleration experiment based at CERN
  • AXP: Anomalous X-ray pulsar

B

  • B/C: Boron-to-Carbon flux ratio in cosmic rays
  • BAMPS: Boltzmann Approach of Multi-Parton Scatterings
  • BAO: Baryon Acoustic Oscillation
  • BaSc: Baryon Scattering lattice collaboration
  • BAT: Burst Alert Telescope aboard the Swift satellite observatory
  • BATSE: Burst and Transient Source Experiment
  • BAU: Baryon asymmetry of the universe
  • BBGKY: Bogoliubov, Born, Green, Kirkwood and Yvon
  • BBGLN: Beneke, Buchalla, Greub, Lenz and Nierste
  • BBN: Big Bang nucleosynthesis
  • BBO: Big Bang Observer
  • BBTW: Bedaque, Buchoff, Tiburzi and Walker-Loud
  • BCA: bremsstrahlung, Compton scattering, and axio-recombination processes
  • BCC: Body-centered cubic crystal structure
  • BCDMS: Bologna, CERN, Dubna, Munich and Saclay DIS experiment using CERN's SPS muon beam
  • BCFW: Britto, Cachazo, Feng and Witten
  • BCG: Brightest cluster galaxies
  • b-CGC: Impact-parameter-dependent Color Glass Condensate
  • BCJ: Bern, Carrasco and Johansson duality proposing that quantum gravity is a double copy of SU(3) gauge theory
  • BCOV: Bershadsky, Cecotti, Ooguri and Vafa
  • BCS: Bardeen, Cooper, and Schrieffer
  • BCVEGPY: An event generator for Bc meson production interfaced with VEGAS and PYTHIA
  • BDF: Proposed Beam Dump Facility at CERN
  • BdG: Bogoliubov and de Gennes
  • BDI: Chiral orthogonal topological insulator symmetry class, not an acronym
  • BDic: Bunch-Davies initial conditions
  • BDM: Bound dark matter model
  • BDMPS-Z: Baier, Dokshitzer, Mueller, Peigne and Schiff; Zakharov
  • BDS: Bern, Dixon and Smirnov
  • BDT: Boosted decision tree
  • BDX: Beam-Dump eXperiment at Jefferson Lab
  • BEACH: Hyperons, Charm and Beauty Hadrons (in French?)
  • BEGe: Broad Energy Germanium detector
  • BELLA: Berkeley Lab Laser Accelerator
  • BEMC: Barrel Electromagnetic Calorimeter
  • BEPC: Beijing Electron-Positron Collider
  • BeppoSAX: Giuseppe Occhialini Satellite per Astronomia X
  • BES: Beam energy scan at RHIC
  • BES: Beijing Spectrometer
  • BES: Beisert, Eden and Staudacher
  • BESS: Balloon-borne Experiment with a Superconducting Spectrometer
  • BESS: Breaking electroweak symmetry strongly
  • BEST: Baksan Experiment on Sterile Neutrino
  • BET: Boundary effective theory
  • BETS: Balloon-borne Electron Telescope with Scintillating fibers
  • BF: "Background field" topological field theory involving two-form B and curvature form F
  • BF: Breitenlohner and Freedman
  • BFACF: Berg, Forster, Aragao, Caracciolo and Frohlich algorithm
  • BFKL: Balitsky, Fadin, Kuraev and Lipatov
  • BFLK: Bukhvostov, Frolov, Lipatov and Kuraev
  • BFM: Background field method
  • BFP: Berkeley, Fermilab and Princeton
  • BFRT: Brookhaven, Fermilab, Rochester and Trieste
  • BFSS: Banks, Fischler, Shenker and Susskind
  • BFV: Batalin, Fradkin and Vilkovisky
  • BGK: Bhatnagar, Gross and Krook
  • BGL: Boy, Grinstein and Lebed form factor parameterization
  • BGL: Branco, Grimus and Lavoura two-Higgs-doublet model
  • BGO: Bismuth orthogermanate
  • BHHRS: Brown, Harada, Holt, Rho and Sasaki
  • BHL: Beisert, Hernandez and Lopez
  • BHL: Brodsky, Huang and Lepage
  • BHT: Bergshoeff, Hohm and Townsend
  • BICEP: Background Imaging of Cosmic Extragalactic Polarization
  • BiCGStab: Bi-conjugate gradient stabilized
  • BiCGGR: Bi-conjugate gradient gap-reducing
  • BIM: Bouchiat, Iliopoulos and Meyer
  • BINP: Budker Institute of Nuclear Physics, Russia
  • BjPSR: Bjorken polarized sum rule
  • BJU: Buras, Jager and Urban
  • BK: Balitsky and Kovchegov
  • BK: Becirevic and Kaidalov
  • BKP: Bartels, Kwiecinski and Praszalowicz
  • BKT: Berezinskii, Kosterlitz and Thouless
  • BKY: Bando, Kugo and Yamawaki
  • BL Lac: BL Lacertae objects, a subclass of active galactic nuclei; BL doesn't seem to be an acronym
  • BLAST: Balloon-borne Large-Aperture Sub-millimeter Telescope
  • BLAST: Bates Large Acceptance Spectrometer Toroid
  • BLG: Bagger, Lambert and Gustavsson
  • BLKT: Boundary-localized kinetic term in (non-minimal) extra-dimensional models
  • BLM: Brodsky, Lepage and Mackenzie perturbation theory scale setting procedure
  • BLMSSM: A simple extension of the Minimal Supersymmetric Standard Model where the baryon and lepton numbers are (or just B-L is) local gauge symmetries
  • BLSSM: B-L Supersymmetric Standard Model
  • BLNP: Bosch, Lange, Neubert and Paz
  • BLTP: Bogoliubov Laboratory of Theoretical Physics at JINR
  • BMN: Berenstein, Maldacena and Nastase
  • BMPV: Breckenridge, Myers, Peet and Vafa
  • BMS: Bakulev, Mikhailov and Stefanis
  • BMS: Bass, Mueller and Srivastava parton cascade model code based on VNI
  • BMS: Bondi, Metzner and Sachs asymptotic symmetry group of general relativity
  • BMSSM: Beyond the Minimal Supersymmetric Standard Model
  • BMV: Bessis, Moussa and Villani
  • BOOMERANG: Balloon Observations Of Millimetric Extragalactic Radiation and Geophysics
  • BooNE: Booster Neutrino Experiment
  • BOSS: Baryon Oscillation Spectroscopic Survey
  • BPHZ: Bogoliubov, Parasuik, Hepp and Zimmerman
  • BPS: Bogomolnyi, Prasad and Sommerfield
  • BPSH: Blas, Pujolas, Sibiriakov and Horava
  • BPST: Belavin, Polyakov, Schwarz and Tyupkin classical SU(2) instanton
  • BR: Brown and Rho
  • BR: Burnier and Rothkopf bayesian reconstruction method
  • BRAHMS: Broad RAnge Hadron Magnetic Spectrometers experiment at RHIC
  • BREAD: Broadband Reflector Experiment for Axion Detection proposed at Fermilab
  • BRNS: Indian DAE Board of Research in Nuclear Sciences
  • BRpV: Bilinear R parity Violation
  • BRST: Becchi, Rouet, Stora, and (independently) Tyutin
  • BSI: British Standards Institution
  • BSS: Blankenbecler, Scalapino and Sugar quantum Monte Carlo algorithm
  • BSSN: Baumgarte, Shapiro, Shibata and Nakamura
  • BSV: Bajc, Senjanovic and Vissani
  • BSW: Bauer, Stech and Wirbel
  • BT: Buchmuller and Tye
  • BTZ: Banados, Teitelboim and Zanelli
  • BUU: Boltzmann, Uehling and Uhlenbeck
  • BV: Batalin and Vilkovisky
  • BW: Balkan Workshop
  • BZ: Ball and Zwicky

C

  • CAAR: Center for Accelerated Application Readiness at Oak Ridge
  • CAFPE: Centro Andaluz de Física de Partículas Elementales
  • CALET: CALorimetric Electron Telescope on the International Space Station
  • CAMB: Code for Anisotropies in the Microwave Background
  • CANGAROO: Collaboration of Australia and Nippon for a GAmma Ray Observatory in the Outback
  • CAPRICE: Cosmic AntiParticle Ring Imaging Cherenkov Experiment
  • CARLOMAT: Automatic tool for electron--positron annihilation into hadrons at low energies, apparently not an acronym
  • CASCADE: Monte Carlo event generator, apparently not an acronym
  • CASPAR: Compact Accelerator System for Performing Astrophysical Research at SURF
  • CAST: CERN Axion Solar Telescope
  • CaSToRC: Computation-based Science and Technology Research Center in Cyprus
  • CAT: Computed Axial Tomography
  • CBELSA: Crystal Barrel Detektor at the Elektronen Stretcher Anlage in Bonn
  • CBEA: Cell Broadband Engine Architecture
  • CBI: Cosmic Background Imager
  • CBM: Compressed Baryonic Matter experiment at FAIR/GSI
  • CBPF: Centro Brasileiro de Pesquisas Físicas (Brazilian Center for Research in Physics)
  • CCB: Charge and color breaking
  • CCD: Charge-coupled device
  • CCDM: Creation of cold dark matter (a cosmological model)
  • CCF: Combinatorial collapse filter
  • CCFM: Ciafaloni, Catani, Fiorani and Marchesini evolution equation
  • CCFM-K: Catani, Ciafaloni, Fiorani, Marchesini and Kwiecinski evolution equation
  • CCFR: Chicago, Columbia, Fermilab and Rochester
  • CCQE: Charged current quasielastic scattering
  • CCPR: Computer Center Problem Reporting at JLab
  • CCR: Canonical commutation relations
  • CCWZ: Callan, Coleman, Wess and Zumino
  • cD: central Dominant galaxy
  • CDD: Castillejo, Dalitz, and Dyson
  • CDER: Cluster-decomposition error reduction technique
  • CDEX: China Dark Matter Experiment
  • CDF: Collider Detector at Fermilab
  • CDF: Combinatorial drop filter
  • CDHS: CERN, Dortmund, Heidelberg and Saclay neutrino experiment
  • CDHSW: CERN, Dortmund, Heidelberg, Saclay and Warsaw neutrino experiment
  • CDL: Coleman and De Luccia
  • CDMS: Cryogenic Dark Matter Search
  • CDMS: Constrained dark matter singlet
  • CDP: CERN, Dubna and Protvino
  • CDR: Conceptual Design Report
  • CDR: Conventional dimensional regularization
  • CDT: Causal dynamical triangulation
  • CDW: Charge-density wave
  • CEA: Commissariat a l'energie atomique
  • CEBAF: Continuous Electron Beam Accelerator Facility
  • CEDAR: Combined e-Science Data Analysis Resource for high-energy physics
  • CEDM: Chromo-electric dipole moment
  • CEE: Mathematics Centre for Enhancement in Education
  • CEEX: Coherent exclusive exponentiation
  • CELLO: Not an acronym, particle detector at DESY's PETRA
  • CELSIUS: Cooling with ELectrons and Storing of Ions from the Uppsala Synchrocyclotron
  • CENTRA: Centro Multidisciplinar de Astrofísica at the Instituto Superior Técnico Lisboa
  • CEP: Critical end point
  • CEPC: Circular Electron Positron Collider proposed in China
  • CESR: Cornell Electron Storage Ring
  • CETUP: Center for Theoretical Underground Physics
  • CE$\nu$NS: Coherent Elastic Neutrino--Nucleus Scattering
  • CFF: Compton form factor
  • CFHT: Canada-France-Hawaii telescope
  • CFHTLenS: Canada-France-Hawaii Telescope Lensing Survey
  • CfA: Harvard--Smithsonian Center for Astrophysics redshift survey
  • CFL: Color-flavor-locked
  • CFNS: Center for Frontiers in Nuclear Science at Stony Brook
  • CGC: Clebsch--Gordan coefficient
  • CGC: Color glass condensate
  • CGLN: Chew, Goldberger, Low and Nambu
  • CGNE: Conjugate gradient on the normal equations
  • CGNR: Conjugate gradient normal residual
  • CGRO: Compton Gamma Ray Observatory
  • CHAMP: CHArged Massive Particle
  • ChaNGa: Charm N-body Gravity solver
  • CHAOS: Canadian High Acceptance Orbit Spectrometer at TRIUMF
  • CHAOS: Clustered High Availability Operating System
  • CHARM: CERN, HAmburg, Rome and Moscow Neutrino Experiment at the CERN SPS
  • CHASE: Chameleon Afterglow Search
  • CheckMATE: Check Models At Terascale Energies program
  • chGOE: Chiral gaussian orthogonal ensemble
  • chGSE: Chiral gaussian symplectic ensemble
  • chGUE: Chiral gaussian unitary ensemble
  • Chi Nu: Neutron detector at LANSCE, acronym unknown
  • CHIME: Canadian Hydrogen Intensity Mapping Experiment
  • CHIMERA: Comprehensive Hydrodynamical Integrated Modelling Evaluation and Reporting Algorithm
  • CHIPS: CHerenkov detectors In mine PitS experiment using Fermilab neutrinos
  • CHIRON: Package for two-loop numerical chiral perturbation theory, apparently not an acronym
  • CHL: Central Helium Liquefier at Jlab
  • CHL: Chaudhuri, Hockney and Lykken
  • CHORUS: CERN Hybrid Oscillation Research apparatUS
  • CHORUS: Clearinghouse for the Open Research of the United States
  • ChPT: Chiral perturbation theory
  • CHY: Cachazo, He and Yuan
  • CI: Chirally improved
  • CIBJET: Event-by-event generalization of CUJET, acronym unknown
  • CICY: Complete Intersection Calabi--Yau manifolds
  • CiDM: Composite inelastic dark matter
  • CII: Astronomical zone in which hydrogen is fully molecular but carbon is ionized
  • CIMBA: Cubic Interpolation for Minimum Bias Approximation Monte Carlo event generator
  • CINVESTAV: Mexican Centro de INVestigación y de ESTudios AVanzados del Instituto Politécnico Nacional
  • CIPANP: Conference on the Intersections of Particle and Nuclear Physics
  • CIPT: Contour-improved perturbation theory
  • CITA: Canadian Institute for Theoretical Astrophysics
  • CJPL: China Jin-Ping underground Laboratory
  • CJT: Cornwall, Jackiw and Tomboulis
  • CKKU: Cohen, Kaplan, Katz and Unsal
  • CKKW: Catani, Krauss, Kuhn and Webber
  • CKM: Cabibbo, Kobayashi and Maskawa
  • CKN: Cohen, Kaplan and Nelson
  • CKS: Carcamo, Kovalenko and Schmidt mechanism for SM flavor hierarchy
  • CLAF: Latin American Center for Physics in Rio de Janeiro
  • CLAFEX: Cosmology and High Energy Physics Laboratory
  • CLARA: Compact Linear Accelerator for Research and Applications at Daresbury
  • CLAS: CEBAF Large Acceptance Spectrometer
  • CLASS: Cosmic Lens All-Sky Survey
  • CLASS: Cosmic Linear Anisotropy Solving System code
  • CLEAN: Cryogenic Low-Energy Astrophysics with Noble gases
  • CLEO: Not an acronym, detector at CESR
  • CLEO: Conference on Lasers and Electro-Optics
  • CLF: Central Laser Facility at Harwell
  • cLFV: Charged lepton flavor violating observables
  • CLIC: Compact Linear Collider
  • CLICdp: Compact Linear Collider Detector and Physics Collaboration
  • CLICHE: CLIC Higgs Experiment
  • CLN: Caprini, Lellouch and Neubert form factor parameterization
  • CLQCD: Chinese Lattice QCD Collaboration
  • CLS: Coordinated Lattice Simulations
  • CLUES: Constrained Local UniversE Simulations
  • CMASS: "Constant mass" galaxies in the Sloan Digital Sky Survey
  • CMD: Cryogenic Magnetic Detector at VEPP
  • CMFV: Constrained minimal flavor violation
  • CMIT: Liverpool's Centre for Mathematical Imaging Techniques
  • CMOS: Complementary metal-oxide-semiconductor
  • CMS: Compact Muon Solenoid experiment at CERN
  • CMSSM: Minimal supersymmetric standard model constrained so that the scalar and gaugino masses are universal at the GUT scale
  • CMTF: Cryomodule Test Facility at Fermilab
  • CNGS: CERN Neutrinos to Gran Sasso
  • CNI: Computing and Networking Infrastructure
  • CNM: Cold nuclear matter
  • CNMSSM: Constrained next-to-minimal supersymmetric standard model
  • CNRS: Centre National de la Recherche Scientifique
  • CnuB: Cosmic Neutrino Background
  • COBE: Cosmic Background Explorer satellite
  • CoDECS: Coupled Dark Energy Cosmological Simulations database
  • CODEX: COsmic Dynamics and EXo-earth experiment spectrograph for the E-ELT
  • CODEX-b: COmpact Detector for EXotics at LHCb proposed for Run3
  • CoGeNT: Coherent Germanium Neutrino Technology
  • COHERENT: Elastic neutrino--nucleus scattering experiment at SNS, apparently not an acronym
  • COLLAPS: COLlinear LAser SPectroscopy [sic] experiment at ISOLDE
  • COLLIER: Complex One-Loop Library In Extended Regularisations
  • CoLoRFulNNLO: Completely Local subtRactions for Fully differential predictions at NNLO
  • COMET: COherent Muon Electron Transition experiment at J-PARC
  • COMPASS: COmmon Muon Proton Apparatus for Structure and Spectroscopy
  • COMPETE: COmputerized Models, Parameter Evaluation for Theory and Experiment
  • COMPTEL: Imaging Compton Telescope
  • CORE: Cosmic ORigins Explorer proposed satellite
  • CoRoT: Convection Rotation and planetary Transits
  • CORSIKA: COsmic Ray SImulations for KAscade program
  • COSINE: Dark matter experiment run by DM-Ice in collaboration with the Korea Invisible Mass Search, apparently not an acronym
  • COSINUS: Cryogenic Observatory for SIgnatures seen in Next-generation Underground Searches proposal
  • CosmoMC: Cosmological Monte Carlo
  • CoSMoN: Connecting the Standard Model to Nuclei lattice collaboration
  • CosPA: Cosmology and Particle Astrophysics
  • COSY: Cooler Synchrotron at Jülich
  • COUPP: Chicagoland Observatory for Underground Particle Physics
  • COW: Colella, Overhauser and Werner
  • CP^{N-1}: Complex projective model in SU(N)/U(N-1)
  • CPL: Chevallier, Polarski and Linder parameterization of dark energy
  • CP-PACS: Computational Physics by Parallel Array Computer System
  • CPX: Supersymmetric CP-violating benchmark scenario
  • cQPA: Coherent quasiparticle approximation
  • COBRA: Cadmium zinc telluride 0-neutrino double-Beta Research Apparatus at Gran Sasso
  • CORAL: Collaboration of Oak Ridge, Argonne and Lawrence Livermore national labs
  • COST: European Cooperation in Science and Technology framework
  • CQSM: Chiral quark soliton model
  • CPAD: Coordinating Panel for Advanced Detectors
  • CPW: Coplanar Waveguide
  • CR: Cauchy and Riemann
  • CR&D: Collaborative research and development
  • CREAM: Cosmic Ray Energetics And Mass
  • CRES: Cyclotron Radiation Emission Spectroscopy
  • CRESST: Cryogenic Rare Event Search with Superconducting Thermometers
  • CREST: Cosmic Ray Electron Synchrotron Telescope
  • CRID: Cherenkov Ring Imaging Detector, part of SLD
  • CRIRES: CRyogenic high-resolution InfraRed Echelle Spectrograph for ESO's VLT
  • CSA: Coordination and Support Action of the European Commission
  • CSBP: Continuous-state branching process
  • CSC: ATLAS Computing System Commissioning
  • CSD2: Constrained Sequential neutrino Dominance of type 2
  • CSE: Computational Science and Engineering
  • CSIC: Spanish Consejo Superior de Investigaciones Científicas
  • CSL: Continuous spontaneous localization
  • CSO: Cryogenic sapphire oscillator
  • CSP: Computer Security Program at Livermore
  • CSP: Concentrated solar power
  • cSMCS: Constrained Standard Model extended by a Complex Singlet scalar
  • CSS: Collins, Soper and Sterman
  • CSSHOWER: Color-coherent showering description in SHERPA, based on Catani--Seymour dipole factorization
  • CSSM: Centre for the Subatomic Structure of Matter (Australia)
  • CSTB: Coupled Scalar--Tachyon Bounce cosmological model
  • CSW: Cachazo, Svrcek, and Witten
  • CT: CTEQ-TEA parton distribution functions
  • CT: Computed tomography
  • CTA: Cherenkov Telescope Array
  • CTEQ: Coordinated Theoretical--Experimental Project on QCD
  • CTF: Counting Test Facility at Gran Sasso
  • CTP: Closed time path formalism of Schwinger and Keldysh
  • CTR: Controlled thermonuclear reactor
  • CTS: Commodity Technology System at Livermore
  • CUORE: Cryogenic Underground Observatory for Rare Events at Gran Sasso
  • CUDA: No longer an acronym, formerly Compute Unified Device Architecture
  • CUJET: Columbia University jet quenching Monte Carlo
  • CUSP: Magnetic field configuration used by ASACUSA, apparently not an acronym though sometimes treated as such
  • CUSTIPEN: China--US Theory Institute for Physics with Exotic Nuclei
  • CVC: Conserved vector current
  • CVD: Chemical vapor deposition
  • CVMN: Chamseddine and Volkov, later Maldacena and Nunez
  • CW: Closure-finite weak topology
  • CW: Coleman and Weinberg
  • CWoLa: Classification Without Labels machine learning method
  • CXC: Chandra X-ray Center
  • CXO: Chandra X-ray Observatory
  • CYGNO: CYGNUS TPC with Optical readout
  • CYGNUS: Directional dark matter search proposal, apparently not an acronym
  • CZ: Convective zone (for instance of the sun)

D

  • DA: Distribution amplitude (wave function integrated over transverse momentum with fixed longitudinal momentum fraction)
  • DAC: Development Assistance Committee of the OECD
  • DAE: Indian Department of Atomic Energy
  • DAEdALUS: Decay-At-rest Experiment for delta_CP studies At the Laboratory for Underground Science
  • DAF: Deterministic annealing filter
  • DANCE: Detector for Advanced Neutron Capture Experiments at LANL
  • DARWIN: DARk matter WImp search with Noble liquids
  • DAT: Dedicated application time
  • DAV: Type of variable white dwarf star, with spectral type DA (only hydrogen absorption)
  • DAFNE: Double Annular Factory for Nice Experiments at Frascati
  • DAMA/LIBRA: DArk MAtter Large sodium Iodide Bulk for RAre processes experiment
  • DAMIC: Dark Matter In CCDs experiment
  • DAMPE: DArk Matter Particle Explorer satellite launched in 2015
  • DARMA: De Angelis, Roncadelli and Mansutti
  • DART: NASA's Double Asteroid Redirection Test
  • DAS: Double asymptotic scaling approximation
  • DASI: Degree Angular Scale Interferometer
  • DBD: Detailed Baseline Design for the ILC
  • DBESS: Degenerate breaking electroweak symmetry strongly
  • DBI: Dirac, Born and Infeld
  • DBR: Differential branching ratio
  • DBV: Type of variable white dwarf star, with spectral type DB (only helium absorption)
  • DBW2: Doubly blocked from Wilson action in two coupling space
  • DCC: Disoriented Chiral Condensate
  • DCC: Dynamical coupled channels
  • DCE: Dynamical Casimir effect
  • DCP: Deconfined critical point
  • DCT: Discrete cosine transform
  • DCV: Desktop Cloud Visualization
  • dDGLAP: double DGLAP framework for double PDFs
  • DDH: Desplanques, Donoghue and Holstein
  • DDM3Y: Density-Dependent Michigan 3-range Yukawa effective interaction
  • DDVCS: Double deeply virtual Compton scattering
  • DEAP: Dark matter Experiment with Argon and Pulse shape discrimination
  • DEC: Discrete exterior calculus
  • DECam: Dark Energy Camera on the Blanco Telescope
  • DECaLS: DECam Legacy Survey
  • DECIGO: DECI-hertz interferometer Gravitational wave Observatory
  • DeeMe: Muon experiment at J-PARC, acronym unknown
  • DELPHES: Detector simulation code, apparently not an acronym
  • DELPHI: Detector with Lepton, Photon and Hadron Identification
  • DES: Dark energy survey
  • DESI: Dark Energy Spectroscopic Instrument
  • DESY: Deutsches Elektronen Synchrotron
  • DETF: Dark Energy Task Force
  • DFELL: Duke Free-Electron Laser Laboratory
  • DFG: Deutsche Forschungsgemeinschaft (German Research Foundation)
  • DFR: Doplicher, Fredenhagen and Roberts
  • DFSZ: Dine, Fischler, Srednicki and Zhitnitsky
  • DFT: Discrete Fourier transform
  • DGLAP: Dokshitzer, Gribov, Lipatov, Altarelli and Parisi
  • DGLAP-CS: Dokshitzer, Gribov, Lipatov, Altarelli, Parisi, Callan and Symanzik
  • DGLV: Djordjevic, Gyulassy, Levai and Vitev
  • DGP: Dvali, Gabadadze and Porrati braneworld model
  • DGR: Deryagin, Grigoriev and Rubakov
  • DHF: Dark Matter, Hadron Physics and Fusion Physics conference
  • DHM: Dorey, Hofman and Maldacena
  • DHM: Double Higgs Model
  • DHOST: Degenerate Higher-Order Scalar--Tensor modified gravity
  • DIANA: Xenon bubble chamber at IHEP, acronym unknown
  • DIANA: Dakota Ion Accelerators for Nuclear Astrophysics proposed for DUSEL
  • DIANA/HEP: Data Intensive ANAlysis for High Energy Physics project
  • DIAS: Dubna International Advanced School
  • DIANE: DIstributed ANalysis Environment
  • DiRAC: Distributed Research utilising Advanced Computing in the UK
  • DIRAC: DImeson Relativistic Atom Complex at CERN
  • dIrr: Dwarf Irregular galaxy
  • DKP: Duffin, Kemmer and Petiau
  • DKS: Dymarsky, Kuperstein and Sonnenschein
  • DLCQ: Discrete Light-Cone Quantization
  • DLS: Diamond Light Source at Harwell
  • DLS: DiLepton Spectrometer experiment
  • DM-Ice: Sodium iodide (thallium) dark matter direct detection experiment in the South Pole ice
  • DMA: Direct memory access
  • DMFA: Slovenian Society of Mathematicians, Physicists and Astronomers (Drustvo matematikov, fizikov in astronomov)
  • DMRG: Density matrix renormalization group tensor network method
  • DMS: Data Movement and Storage department at Fermilab
  • DMTPC: Dark Matter Time Projection Chamber experiment
  • DNDO: Domestic Nuclear Detection Office in the Department of Homeland Security
  • DONUT: Direct Observation of the NU Tau experiment at Fermilab
  • DORIS: DOppel-RIng Speicher (double-ring storage) at DESY
  • DP: Data parallelism
  • DPD: Double parton distribution
  • DPDF: Diffractive parton distribution function
  • dPDF: Double parton distribution function
  • DPMJET: Monte Carlo code based on the Dual Parton Model
  • DPR: Dilepton production rate in quark--gluon plasma
  • DPT: Dispersively improved perturbation theory
  • DR: Data release
  • DR3: Simultaneous modelling of D-term (DT) scalar mass splitting, right-handed neutrino (RHN) Yukawa coupling effects, and mass splitting between the third generation and first two generations of matter scalars (3GS)
  • DRA: Method of multiloop integral evaluation based on D-dimensional Recurrence relations and Analytical properties as a function of D
  • DRbar: Modified Dimensional Reduction
  • DRED: Dimensional reduction
  • DREG: Dimensional regularization
  • DREENA-B: Dynamical Radiative and Elastic ENergy loss Approach for medium modeled by Bjorken expansion code
  • DREENA-C: Dynamical Radiative and Elastic ENergy loss Approach for Constant-temperature QCD medium code
  • dRGT: de Rham, Gabadadze and Tolley massive gravity theory
  • DSE: Dyson--Schwinger equation
  • DSIT: Department for Science, Innovation and Technology in the UK
  • dSph: Dwarf Spheroidal galaxy
  • DSR: Doubly or deformed Special Relativity
  • DSSM: Delta-deformed Supersymmetric Standard Model
  • DSSV: De Florian, Sassot, Stratmann and Vogelsang helicity parton densities global fit
  • DSTL: Defence Science and Technology Laboratory in the UK
  • DTRA: Defense Threat Reduction Agency
  • DTT: Divergence-type theory
  • DUNE: Deep Underground Neutrino Experiment
  • DURA: Deep Underground Research Association
  • DUSEL: Deep Underground Science and Engineering Laboratory
  • DV: Duality violation (terms potentially complementing the OPE)
  • DVCS: Deeply Virtual Compton Scattering
  • DVMP: Deeply Virtual exclusive Meson leptoProduction
  • DVZ (or vDVZ): van Dam, Veltman and (independently) Zakharov
  • DWARF: Debugging With Arbitrary Record Formats standard
  • DWIA: Directed wave impulse approximation

E

  • EADL: Evaluated Atomic Data Library
  • EAIM: An exact analytical iteration method
  • EAS: Extensive air shower
  • EAS-MSU: Telescope array run by Moscow State University to detect and analyze extensive air showers
  • EBAC: Excited Baryon Analysis Center at Jlab
  • EBEX: E and B Experiment balloon-borne CMB telescope
  • EBL: Extragalactic background light
  • eBOSS: Extended Baryon Oscillation Spectroscopic Survey
  • EBSD: Electron Backscatter Diffraction
  • EC: Electron capture
  • ecCNO: Electron capture reactions taking nitrogen to Carbon, oxygen to Nitrogen, and fluorine to Oxygen
  • ECFA: European Committee for Future Accelerators
  • ECHO: Eulerian Conservative High-Order code for astrophysics and QGP
  • ECO: Exotic compact object
  • ECOSMOG: Efficient COde for Simulating MOdified Gravity
  • ECS: ESnet Collaboration Service
  • ECT: European Center for Theoretical Studies in Nuclear Physics and Related Areas
  • ECuME: Electroplated Cuprum Manufacturing Experiment
  • EDD: Exclusive double diffractive
  • EDELWEISS: Expérience pour DEtecter Les Wimps En Site Souterrain
  • EDGES: Experiment to Detect the Global Epoch of reionization Signature
  • EDI: Equity, diversity and inclusion
  • EDMFT: Extended Dynamical Mean Field Theory
  • EDS: Elastic and diffractive scattering
  • E-ELT: European Extremely Large Telescope of ESO
  • EEX: Exclusive exponentiation
  • EF: Eddington and Finkelstein
  • EGEE: Enabling Grids for E-sciencE
  • EGI: European Grid Infrastructure foundation
  • EGM: Extended gauge model
  • EGO: European Gravitational Observatory
  • EGRB: Extragalactic gamma ray background
  • EGRET: Energetic Gamma Ray Experiment Telescope
  • EHT: Event Horizon Telescope
  • EIC: Electron-Ion Collider
  • EicC: Proposed Electron-Ion Collider in China, based on HHIAF in Huizhou
  • EIC: European Innovation Council
  • EKHARA: e+e- event generator, acronym unknown
  • EKRT: Eskola, Kajantie, Ruuskanen and Tuominen heavy-ion collision model
  • EKS: Ellis, Kunszt and Soper (code for jet distribution calculations)
  • EKS: Eskola, Kolhinen and Salgado
  • ELBNF: Experimental program at the Long-Baseline Neutrino Facility collaboration
  • ELDER: ELastically DEcoupling Relic dark matter
  • ELKO: Eigenspinoren des Ladungskonjugationsoperators (dual-helicity eigenspinors of the charge conjugation operator)
  • ELI: Extreme Light Infrastructure
  • eLISA: evolved Laser Interferometer Space Antenna, also known as NGO
  • ELISe: ELectron Ion scattering in a Storage ring (eA-collider) experiment at FAIR
  • ELPH: Research Center for ELectron PHoton Science at Tohoku University
  • ELSA: Elektronen Stretcher Anlage in Bonn
  • eLSM: Extended Linear Sigma Model
  • EMC: European Muon Collaboration
  • EMCCD: Electron multiplication charge-coupled device
  • EMMA: Electron Machine with Many Applications accelerator at Daresbury
  • EMMI: ExtreMe Matter Institute
  • EMPIC: Electromagnetic particle-in-cell
  • EMSSM: MSSM with Environmentally selected dark matter
  • ENC: Electron-Nucleon Collider
  • ENDF: Evaluated Nuclear Data File
  • ENDL: Evaluated Nuclear Data Library
  • ENUBET: Enhanced NeUtrino BEams from kaon Tagging proposed facility
  • EOGM: Extra-ordinary gauge mediation
  • EoR: Epoch of Reionization
  • EP: Event plane
  • EPAC: Extreme Photonics Applications Centre at the CLF at Harwell
  • EPAPS: Electronic Physics Auxiliary Publication Service
  • EPCC: Edinburgh Parallel Computing Centre
  • EPECUR: pi-p elastic scattering experiment at ITEP, acronym unknown, Russian for Epicurus
  • EPIC: Einstein Polarization Interferometer for Cosmology
  • EPICS: Experimental Physics and Industrial Control System
  • EPIQS: Emergent Phenomena In Quantum Systems
  • EPM: Ephemerides of Planets and the Moon
  • EPN: European Photon and Neutron campus in Grenoble
  • EPNJL: Entangled Polyakov, Nambu and Jona-Lasinio model
  • EPOS: Hadronic interaction model with Energy conserving quantum mechanical multiple scattering approach, based on Parton ladders, Off-shell remnants and Splitting of parton ladders
  • EPoSS: European Technology Platform on Smart Systems Integration policy initiative
  • EPPCN: European Particle Physics Communication Network
  • EPPS: Eskola, Paakkinen, Paukkunen and Salgado
  • EPS: Eskola, Paukkunen and Salgado
  • EPTA: European Pulsar Timing Array
  • ePUMP: Error PDF Updating Method Package code
  • eQPA: Extended quasiparticle approximation
  • ERA: European Research Area (e.g., QuantERA)
  • ERBL: Efremov, Radyushkin, Brodsky and Lepage
  • ERE: Effective range expansion
  • ERE: Encuentros Relativistas Españoles
  • ERL: Energy Recovery Linac at Daresbury, renamed ALICE
  • EROS: Expérience pour la Recherche d'Objets Sombres microlensing survey
  • eROSITA: X-ray instrument for Russian--German Spektr-RG space observatory, superseding ROSAT
  • ESA: European Space Agency
  • ESAAB: DOE Energy Systems Acquisition Advisory Board
  • ESD: Education for Sustainable Development
  • ESFRI: European Strategy Forum on Research Infrastructures
  • ESG: Environmental, Social and Governance strategy
  • ESI: Erwin Schrodinger International Institute for Mathematical Physics
  • ESNet: Energy Sciences Network
  • ESO: European Southern Observatory
  • ESPRESSO: Echelle SPectrograph for Rocky Exoplanet- and Stable Spectroscopic Observations
  • ESRF: European Synchrotron Radiation Facility
  • ESRL: Earth System Research Laboratory of NOAA
  • ESS: European Spallation Source in Sweden
  • ESSFSM: Extended Singlet Scalar Fermionic Standard Model
  • ESSnuSB: European Spallation Source Neutrino Super Beam
  • ESSENCE: Equation of State: SupErNovae trace Cosmic Expansion
  • ETH: Swiss Federal Institute of Technology (Eidgenössische Technische Hochschule) in Zurich, and a pion--nucleon scattering model developed there
  • ETI: NNSA Consortium for Enabling Technologies and Innovation
  • ETM: European Twisted Mass Collaboration
  • ETHOS: Effective THeory Of Structure Formation cosmological N-body simulations
  • ETP: European Technology Platform
  • ETQS: Efremov, Teryaev, Qiu and Sterman
  • EuCAPT: European Consortium for Astroparticle Theory
  • EUREKA: European Research Coordination Agency
  • EVN: European Very Long Baseline Interferometry Network
  • EWBG: Electroweak baryogenesis
  • EWIP: Extremely Weakly Interacting Particle
  • EWPT: Electroweak phase transition
  • EWPT: Electroweak precision tests
  • EWSB: Electroweak symmetry breaking
  • EXO: Enriched Xenon Observatory
  • EYM: Einstein, Yang and Mills

F

  • FACET: Facility for Advanced Accelerator Experimental Tests at SLAC
  • FAIR: Facility for Antiproton and Ion Research at GSI
  • FAIR: Findable, Accessible, Interoperable and Reusable data
  • FAIRNESS: FAIR NExt generation ScientistS
  • FAKT: Fachausschusses für Kern- und Teilchenphysik of the Austrian Physical Society
  • FAPT: Fractional Analytic Perturbation Theory
  • FAQSC: Liverpool Faculty Academic Quality and Standards Committee
  • FASER: ForwArd Search ExpeRiment at the LHC
  • FAST: Fermilab Accelerator Science and Technology facility
  • FAST: Five-hundred-meter Aperture Spherical radio Telescope in China
  • FASTSUM: Frascati, Argonne, Seoul, Trinity, Swansea, Utah and Maynooth
  • FBA: Forward--backward asymmetry
  • FBS: Few-body system
  • FCAL: Collaboration to develop Forward CALorimeters for future electron--positron colliders
  • FCC: Face-centered cubic crystal structure
  • FCC: Future Circular Collider
  • FCHAMP: Fractionally charged massive particle
  • FCT: Fundação para a Ciência e a Tecnologia in Portugal
  • FDH: Four-dimensional helicity regularization scheme
  • FDR: Four Dimensional Regularization scheme
  • FDTD: Finite-difference time-domain
  • FEL: Free electron laser
  • FEM: Finite element method
  • FEN: Front-end node
  • FEROS: Fiber-fed Extended Range Optical Spectrograph for the MPG/ESO 2.2-meter telescope
  • FEWZ: Fully Exclusive W and Z production code
  • feynMF: LaTeX/Metafont package for drawing Feynman diagrams
  • feynMP: LaTeX/MetaPost package for drawing Feynman diagrams
  • FFLO: Fulde, Ferrel, Larkin and Ovchinnikov
  • FFNS: Fixed flavor number scheme
  • FG: Fefferman and Graham
  • F-GUT: F-theory Grand Unified Theory
  • FGCR: Flexible Generalized Conjugate Residual
  • FGL: Fermi Gamma-ray Large-area telescope
  • FGMRES: Flexible generalized minimal residual algorithm
  • FGMRES-DR: Flexible generalized minimal residual algorithm deflated restarted
  • FGY: Frampton, Glashow and Yanagida
  • FHL: Fermi Large Area Telescope Catalog of High-Energy Sources
  • FHSV: Ferrara, Harvey, Strominger and Vafa
  • FI: Fayet and Iliopoulos
  • FIESTA: Feynman Integral Evaluation by a Sector decomposiTion Approach
  • FIMP: Feebly Interacting Massive Particle
  • FImP: Feebly Interacting light Particle
  • FiO/LS: Frontiers in Optics / Laser Science conference
  • FIRAS: Far Infrared Absolute Spectrophotometer
  • FIRE: Feynman Integral REduction Mathematica package
  • FIS: File Interchange Service at Livermore
  • FJPPL: France Japan international-associated Particle Physics Laboratories
  • FK: Fortuin and Kasteleyn random cluster model
  • fKLN: Factorized Kharzeev, Levin and Nardi model for pre-equilibrium phase
  • FKPPL: France Korea international-associated Particle Physics Laboratories
  • FKS: Feldman, Kroll and Stech
  • FKS: Forshaw, Kerley and Shaw
  • FKS: Frixione, Kunszt and Signer subtraction
  • FKTUY: Fujiwara, Kugo, Terao, Uehara and Yamawaki
  • FL: Friedberg and Lee
  • FLAG: Flavour Lattice Averaging Group
  • FLASY: Workshop on FLAvour SYmmetries
  • FLHA: Flavor Les Houches Accord
  • FLIC: Fat Link Irrelevant Clover
  • FLRW: Friedmann, Lemaître, Robertson and Walker
  • FLUKA: FLUktuierende KAskade (fluctuating cascade) Monte Carlo package
  • FMO: Friedland, McKellar and Okuniewicz
  • FOA: Funding Opportunity Announcement
  • FONLL: Method originally based on combining Fixed (second) Order and Next-to-Leading Log calculations; now used more generally to combine fixed-order and resummed calculations
  • FOM: Figure of Merit
  • FOM: Full orthogonalization method
  • FOPI: Four-pi detector at GSI
  • FOPT: Fixed-order perturbation theory
  • FORM: Symbolic manipulation system, apparently not an acronym
  • FortEPiaNO: FORTran-Evolved PrimordIAl Neutrino Oscillations code
  • FPGA: Field-programmable gate array
  • FPY: Fission product yield
  • FR: Fanaroff and Riley classes of radio galaxies
  • FREYA: Fission Reaction Event Yield Algorithm
  • FRIB: Facility for Rare Isotope Beam at Michigan State
  • FRITIOF/FTF: Monte Carlo program(s) implementing Lund string dynamics, apparently not an acronym
  • FRG: Functional renormalization group
  • FRGE: Functional renormalization group equation
  • FROG: Fast and Realistic OpenGL event display
  • FRS: Freyhult, Rej and Staudacher
  • FRW: Friedmann, Robertson and Walker
  • FSC: Forward Shower Counter
  • FSI: Final state interactions
  • FSR: Final state radiation
  • FSRQ: Flat-spectrum radio quasar
  • FZ: Ferrara and Zumino

G

  • G2HDM: Gauged Two-Higgs-Doublet Model
  • GAM: Geodesic acoustic mode
  • GAMBIT: Global And Modular Beyond-the-standard-model Inference Tool
  • GammeV: Fermilab experiment searching for gamma to milli-eV particle transition
  • GAMS: Hodoscopic Automatic Multiphoton Spectrometer (in Russian)
  • GAN: Generative Adversarial (neural) Networks
  • GANIL: Grand Accélérateur National dIons Lourds
  • GAP: Groups, Algorithms, Programming code for computational discrete algebra
  • GAPP: Global Analysis of Particle Properties
  • GAPS: General Antiparticle Spectrometer
  • GARD: General Accelerator Research and Development
  • GARM: Generalized atmospheric Rosenbluth method
  • GB: Gunion and Bertsch
  • GBM: Gamma-ray Burst Monitor, part of Fermi/GLAST
  • GBW: Golec-Biernat and Wüsthoff
  • GCG: Generalized Chaplygin gas
  • GCM: Generator coordinate method
  • GCR: Generalized conjugate residual algorithm
  • GCRF: Global Challenges Research Fund of UKRI
  • GDA: Generalized distribution amplitude
  • GDE: Global Design Effort of the ILC
  • GDH: Gerasimov, Drell and Hearn
  • GDR: GPUDirect RDMA
  • GEANT: GEometry ANd Tracking toolkit for simulating of the passage of particles through matter using Monte Carlo methods
  • GEMMA: Germanium Experiment for measurement of Magnetic Moment of Antineutrino at the Kalinin Nuclear Power Plant
  • GEMS: Gravity and Extreme Magnetism (proposed NASA mission)
  • GENEVA: A Monte Carlo combining higher-order resummations with higher fixed-order calculations, apparently not an acronym
  • GENIE: Generates Events for Neutrino Interaction Experiments
  • GENXICC: A Generator for Hadronic Production of Double Heavy Baryons Xi_{cc}
  • GERDA: GERmanium Detector Array at Gran Sasso
  • GERT: General Employee Radiological Training
  • GeVin: GeV inert fermion
  • GEVP: Generalized eigenvalue problem
  • Gfitter: A Generic Fitter Project for HEP Model Testing
  • GGA: Generalized gradient approximation
  • GGM: Generalized Gauge Mediation
  • GGRESRC: e+e- event generator, acronym unknown
  • GGT: Gluon-gluino tree
  • GHZ: Greenberger--Horne--Zeilinger state in quantum information theory
  • GiBUU: Giessen Boltzmann--Uehling--Uhlenbeck transport model project
  • GIM: Glashow, Iliopoulos and Maiani
  • GIMP: Gravitationally Interacting Massive Particle
  • GINGER: Gyroscopes IN GEneral Relativity
  • GiNaC: GiNaC is Not a CAS (Computer Algebra System)
  • GKP: Gubser, Klebanov and Polyakov rotating string
  • GKPY: Garcia-Martin, Kaminski, Palaez and Yndurain
  • GL: General Linear group
  • GL: Global and local electromagnetic simulation
  • GLACIER: Giant Liquid Argon Charge Imaging ExpeRiment
  • GLAST: Fermi Gamma-ray Large Area Space Telescope
  • GLE: Generalized Langevin equation
  • GLMM: Gotsman, Levin, Maor and Miller
  • GLoBES: General Long Baseline Experiment Simulator
  • GLR-MQ: Gribov, Levin, Ryskin, Mueller and Qiu
  • GLV: Gyulassy, Levai and Vitev
  • GLW: de Groot, van Leeuwen and van Weert energy--momentum and spin tensors
  • GM-VFN: General-mass variable-flavor-number
  • GMO: Goldberger, Miyazawa and Oehme
  • GMOR: Gell-Mann, Oakes and Renner
  • GMRES: Generalized minimal residual algorithm
  • GMRES-DR: Generalized minimal residual algorithm deflated restarted
  • GMRESR: Generalized minimal residual recursive algorithm
  • GmSUGRA: Generalized Minimal Supergravity model
  • GMSB: Gauge-mediated supersymmetry breaking
  • GNMSSM: The most general form of the NMSSM
  • GNO: Goddard, Nuyts and Olive magnetic charge
  • GNSS: Global Navigation Satellite System
  • GOE: Gaussian orthogonal ensemble
  • GOLEM: General One Loop Evaluator for Matrix elements
  • GoSam: Package that bundles GOLEM and SAMURAI among others
  • GPD: Generalized parton distribution
  • GPFS: IBM General Parallel File System
  • GPhyS: Gravitation and Fundamental Physics in Space
  • GPI: Global Address Space Programming Interface
  • GPPZ: Girardello, Petrini, Porrati and Zaffaroni
  • GRAAL: GRenoble Anneau Accelerateur Laser
  • GRACE: Gravity Recovery and Climate Experiment
  • GRACE: Event generator, apparently not an acronym
  • GRAIL: Gravity Recovery and Interior Laboratory NASA mission
  • GRAMS: Gamma-Ray and AntiMatter Survey proposal
  • GRAND: Giant Radio Array for Neutrino Detection
  • GRANIT: Gravitational Neutron Induced Transitions spectrometer
  • GRAPES: Gamma Ray Astronomy PeV EnergieS muon telescope in Tamil Nadu
  • GRAVITY: Interferometric instrument for ESO's VLTI, acronym unknown
  • GR@PPA: Grace at Proton-Proton/Antiproton event generator based on GRACE
  • GRB: Gamma-ray burst
  • GRS: Gamma Ray Spectrometer aboard the Solar Maximum Mission
  • GRS: Gregory, Rubakov and Sibiryakov
  • GS: Gaunt and Stirling
  • GS: Green and Schwarz superstring
  • GSE: Gaussian symplectic ensemble
  • GSI: Gesellschaft für Schwerionenforschung (Center for Heavy Ion Research)
  • GSM: Generic small quark mass regime of chiPT
  • GSO: Gliozzi, Scherk and Olive
  • GSR: Generalized slow-roll formalism
  • GTC: NVIDIA GPU Technology Conference
  • GUE: Gaussian unitary ensemble
  • GVD: Gigaton Volume Detector in Lake Baikal
  • GW: Gravitational wave
  • GWAS: Genome-wide association study
  • GZ: Gribov and Zwanziger
  • GZK: Greisen, Zatsepin and Kuzmin

H

  • HA-PACS: Highly Accelerated Parallel Advanced system for Computational Sciences in Tsukuba
  • HADES: High Acceptance Di-Electron Spectrometer experiment at FAIR
  • HAL QCD: Hadrons to Atomic nuclei from Lattice QCD Collaboration
  • HALO: Helium And Lead Observatory at SNO
  • HAPPEX: Hall A Precision Parity EXperiment at JLab
  • HARDPING: HARD Probe INteraction Generator Monte Carlo event generator
  • HARP: Hadron Production experiment at CERN
  • HARPS: High Accuracy Radial Velocity Planet Searcher spectrograph at La Silla
  • HATCH: Holography: Applications to Technicolor, Condensed matter and Hadrons
  • HATHOR: HAdronic Top and Heavy quarks crOss section calculatoR
  • HAWC: High-Altitude Water Cherenkov observatory in Mexico
  • HAWK: A Monte Carlo generator for the production of Higgs bosons Attached to WeaK bosons at hadron colliders
  • HAYSTAC: Haloscope At Yale Sensitive To Axion CDM
  • HB: Horizontal Branch (classification of stars near Main Line)
  • HBL: High-frequency-peaked BL Lacertae objects
  • HBT: R. Hanbury Brown and R. Twiss
  • HDF: Hierarchical Data Format
  • HDL: Hard density loop
  • HEAO: High Energy Astronomy Observatory
  • HEAT: High Energy Antimatter Telescope
  • HECOLS: High Energies, Compact Objects, and Large Surveys Polish--French lab
  • HEdSA: Higher Education Service Area of the IMA
  • HEFTY: DOE Topical Collaboration on HEavy-Flavor TheorY for QCD Matter
  • HEGET: HELAS Evaluation with GPU Enhanced Technology
  • HEIDI: extension of the standard model with a "higher dimensional" scalar singlet field
  • HEIF: Higher Education Innovation Funding in the UK
  • HELAC: A package to compute electroweak helicity amplitudes
  • HELAS: Helicity Amplitude Subroutines
  • HEPAP: High Energy Physics Advisory Panel
  • HEPGEN: Hard Exclusive Production GENerator for leptoproduction at COMPASS
  • HERA: Hadron Elektron Ring Anlage at DESY
  • HERA: Hydrogen Epoch of Reionization Array interferometer
  • HERD: High Energy cosmic-Radiation Detection facility proposed for a future Chinese space station
  • HERMES: High-Energy Radiation Megavolt Electron Source at Sandia National Lab
  • HERMES: DESY fixed-target experiment to explore spin, apparently not an acronym
  • HERWIG: Hadron Emission Reactions With Interfering Gluons parton shower generator
  • HERWIRI: High Energy Radiation with Infrared Improvements parton shower generator
  • HESE: High-energy starting events in neutrino telescopes like IceCube
  • HESR: High Energy Storage Ring collider at FAIR
  • HESS: High Energy Stereoscopic System
  • HFAG: Heavy Flavor Averaging Group
  • HFET: Heterojunction field effect transistor
  • HFI: High frequency instrument
  • HFIR: High Flux Isotope Reactor at ORNL
  • HFS: Hyperfine splitting or hyperfine structure
  • HH: Herbig and Haro object in jets from star formation
  • HHchiPT: Heavy hadron chiral perturbation theory
  • HHIAF: High-intensity Heavy-Ion Accelerator Facility (formerly Heavy-Ion Advanced research Facility, HIAF?) under construction in Huizhou
  • HI: Astronomical zone in which hydrogen is mostly atomic
  • HIC: Helmholtz International Center for FAIR
  • HIE-ISOLDE: High Intensity and Energy upgrade of ISOLDE
  • HIGS: High-Intensity Gamma-ray Source at DFELL
  • HIJING: Heavy Ion Jet INteraction Generator
  • HILAS: High Intensity Large Acceptance Spectometer proposed for Jlab
  • HIP: Heterogeneous-compute Interface for Portability for GPU programming
  • HiPER: High Power laser Energy Research
  • HIRAX: Hydrogen Intensity and Real-time Analysis eXperiment telescope array in South Africa
  • HIRES: High Resolution Echelle Spectrometer at the Keck observatory in Hawaii
  • HiRes-MIA: Hybrid detector consisting of the High Resolution Fly's Eye prototype and the MIchigan muon Array in Utah
  • HiSCORE: Hundred Square-km Cosmic ORigin Explorer
  • HISKP: Helmholtz-Institut für Strahlen- und Kernphysik (Helmholtz Institute for Radiation and Nuclear Physics)
  • HISZ: Hagiwara, Ishihara, Szalapski and Zeppenfeld EW EFT basis
  • HKN: Hirai, Kumano and Nagai nuclear parton distribution functions
  • HL: Heavy-light, factorization used in neutrino oscillation studies
  • HLRF: High-level radio frequency
  • HLS: Hidden local symmetry
  • HM: High-mass
  • HMChPT: Heavy Meson Chiral Perturbation Theory
  • HMM: Hidden Markov Model
  • HOBET: Harmonic-Oscillator-Based Effective Theory
  • HOMFLY-PT: Hoste, Ocneanu, Millett, Freyd, Lickorish, Yetter, Przytycki and Traczyk
  • HORACE: Higher Order RAdiative CorrEctions event generator
  • HPCC: High Performance Computing and Communications
  • HPL: Harmonic polylogarithms
  • HPQCD: High-precision QCD collaboration
  • HPS: Heavy Photon Search experiment at JLab
  • HQE: Heavy quark expansion
  • HQET: Heavy quark effective theory
  • HQL: Heavy Quarks and Leptons conference
  • HQSS: Heavy quark spin symmetry
  • HPGe: High-purity germanium
  • HRG: Hadron resonance gas
  • HRS: High Resolution Separator at ISOLDE
  • HSA: Heterogeneous Systems Architecture
  • HSC: Hadron Spectrum Collaboration
  • HSC: Subaru Hyper Suprime-Cam
  • HSS: Harmonic superspace
  • HST: Hubble Space Telescope
  • HT: Higher twist
  • HTL: Hard thermal loop
  • HTLpt: Hard thermal loop perturbation theory
  • HUNTER: Heavy Unseen Neutrinos from Total Energy-momentum Reconstruction experiment at UCLA
  • HVeV: High-voltage CDMS detector, possibly pushing for eV-scale energy resolution
  • HVP: Hadronic Vacuum Polarisation
  • HXMT: Hard X-ray Modulation Telescope, also known as Insight
  • HYDJET: HYDrodynamics plus JETs heavy ion event generator

I

  • IAA: Impact Acceleration Account
  • IACT: Imaging Atmospheric Cherenkov Telescope
  • IAM: Inverse Amplitude Method for unitarization
  • IARD: International Association for Relativistic Dynamics
  • IARPA: Intelligence Advanced Research Projects Activity
  • IASD: Imaginary anti-self-dual
  • IAU: International Astronomical Union
  • IAXO: International Axion Observatory proposed at CERN
  • iBF: Impact-parameter beam function
  • IB: Isospin breaking
  • IBSHEPP: Iternational Baldin Seminar on High-Energy Physics Problems
  • IBIS: Imager on Board the INTEGRAL Satellite
  • IBL: Intergalactic background light
  • IBP: Integration by parts
  • IC: Inverse-Compton
  • ICAL: Magnetized Iron CALorimeter detector under construction for INO
  • ICAM: Institute for Complex Adaptive Matter
  • ICAP: International Conference on Atomic Physics
  • ICARUS: Imaging Cosmic And Rare Underground Signals, originally at Gran Sasso then moved to Fermilab
  • ICATPP: International Conference on Advanced Technology and Particle Physics
  • ICCA: International Conference on Clifford Algebras
  • ICCING: Initial Conserved Charges in Nuclear Geometry model
  • ICCS: International Conference on Computational Science
  • IceCube: Neutrino observatory in Antarctica, not an acronym but sometimes treated as such
  • ICERM: Institute for Computational and Experimental Research in Mathematics at Brown
  • ICF: Inertial confinement fusion
  • ICFA: International Committee for Future Accelerators
  • ICFO: Instituto de Ciencias Fotónicas (Institute of Photonic Sciences) in Barcelona
  • ICG: Institute of Cosmology and Gravitation
  • ICGAC: International Conference on Gravitation, Astrophysics and Cosmology
  • ICGC: International Conference on Gravitation and Cosmology
  • ICHEC: Irish Centre for High-End Computing
  • ICISE: International Centre for Interdisciplinary Science Education in Quy Nhon
  • ICM: International Conference on Magnetism
  • ICNAAM: International Conference of Numerical Analysis and Applied Mathematics
  • ICRC: International Cosmic Ray Conference
  • ICT: Information and communications technology
  • ICURe: Innovation to Commercialisation of University Research program of Innovate UK
  • iDM: Inelastic dark matter
  • IDM: Inert doublet model
  • IDM: Interacting dark matter
  • iDMRG: Infinite density matrix renormalization group tensor network method
  • IDPASC: International Doctorate Network in Particle Physics, Astrophysics and Cosmology in Portugal and Spain
  • IDS-NF: International Design Study of the Neutrino Factory
  • iEBE-VISHNU: Integrated(?) Event-By-Event Viscous Israel Stewart Hydrodynamics aNd UrQMD
  • IEEE: Institute of Electrical and Electronics Engineers
  • IERC: Integrated Engineering Research Center at Fermilab
  • IETF: UK Industrial Energy Transformation Fund
  • IFAE: Incontri di Fisica di Alta Energia
  • IFIC: Instituto de Física Corpuscular
  • IGCAC: International Conference on Gravitation, Astrophysics and Cosmology
  • IGRB: Isotropic diffuse gamma-ray background
  • IHEP: Institute for High Energy Physics at Protvino, Russia
  • iHixs: Inclusive Higgs boson cross section program
  • IIASA: International Institute for Applied Systems Analysis
  • IIRC: Ito International Research Center in Tokyo
  • IKAROS: Interplanetary Kite-craft Accelerated by Radiation Of the Sun spacecraft
  • IKKT: Ishibashi, Kawai, Kitazawa and Tsuchiya
  • ILC: International Linear Collider
  • ILD: International Large Detector proposed for the ILC
  • ILGTI: Indian Lattice Gauge Theory Initiative
  • ILL: Institut Laue-Langevin
  • IMA: Institute of Mathematics and its Applications
  • IMB: Irvine, Michigan and Brookhaven neutrino detector
  • IMP: Institute of Modern Physics in China
  • IN2P3: Institut national de physique nucléaire et de physique des particules
  • INDIGO: Indian Initiative in Gravitational-wave Observations
  • INFIERI: INtelligent Signal Processing for FrontIEr Research and Industry
  • INFN: Istituto Nazionale di Fisica Nucleare
  • INLN: Institut Non Linéaire de Nice
  • INO: India-based Neutrino Observatory
  • INPOP: Intégration Numérique Planétaire de lObservatoire de Paris
  • INS: Institute for Nuclear Studies at The George Washington University
  • INTEGRAL: International Gamma-Ray Astrophysics Laboratory
  • IOC: Input Output Controller for EPICS
  • IOSH: Institution of Occupational Safety and Health
  • IOTA: Integrable Optics Test Accelerator at Fermilab
  • IP: Impact parameter, used in heavy-ion collision contexts
  • IP-Glasma: Impact-Parameter-dependent Glasma model
  • IP-Sat: Impact-Parameter-dependent Saturation
  • IPA: Interplay of Particle and Astroparticle Physics workshop
  • IPAC: International Particle Accelerator Conference
  • IPDPS: International Parallel and Distributed Processing Symposium
  • iPEPS: Infinite projected entangled pair states tensor network method
  • IPN: InterPlanetary Network of satellites
  • IPPOG: International Particle Physics Outreach Group
  • IPTA: International Pulsar Timing Array
  • IRAS: Irfra-Red Astronomical Satellite
  • IRC: Infrared and collinear
  • IRIS: Infrastructure for Research and Innovation for STFC
  • IRMA: Institut de Recherche Mathématique Avancée associated with CNRS
  • IS: Interstellar cosmic ray fluxes
  • ISAC: Isotope Separator and ACcelerator facility at TRIUMF
  • ISAPP: International School on AstroParticle Physics
  • ISARIC: International Severe Acute Respiratory and Emerging Infection Consortium
  • ISARIC4C: ISARIC Coronavirus Clinical Characterisation Consortium
  • ISC: International Supercomputing Conference
  • ISCO: Innermost stable circular orbit
  • ISD: Imaginary self dual
  • iSF: Inverse soft function
  • ISGW: Isgur, Scora, Grinstein and Wise
  • ISM: Interstellar Medium
  • ISNET: Information and Statistics in Nuclear Experiment and Theory
  • ISW: Integrated Sachs--Wolfe effect from cosmic string
  • IsoDAR: Isotope Decay-At-Rest electron anti-neutrino source for BSM searches
  • ISOLDE: Isotope mass Separator On-Line facility at CERN
  • ISPE: Initial single pion emission
  • ISPF: International Science Partnerships Fund in the UK
  • ISR: Initial-state radiation
  • ISR: Intersecting Storage Rings
  • ISS: Intriligator, Seiberg and Shih
  • ISS: Inverse Seesaw model
  • ISSO: Information System Security Officer
  • ISSYP: International Summer School for Young Physicists at Perimeter
  • ISVHECRI: International Symposium on Very High Energy Cosmic Ray Interactions
  • iTEBD: Infinite time-evolving block decimation tensor network method
  • ITEP: Institute for Theoretical and Experimental Physics in Moscow
  • ITIY: Intriligator, Thomas, Izawa and Yanagida models of dynamical supersymmetry breaking
  • ITMD: Improved Transverse Momentum Dependent factorization
  • ITNA: Individual Training Needs Assessment at Fermilab
  • IWNT: International Workshop on Nuclear Theory
  • IXO: International X-ray Observatory
  • IZEST: International Center for Zetta- Exawatt Science and Technology in Paris
  • IZMIRAN: Institute of Earth magnetism, ionosphere and radiowaves propagation named after Nikolay Pushkov of the Russian Academy of Sciences (Institut zemnogo magnetizma, ionosfery i rasprostraneniya radiovoln im. N. V. Pushkova Rossiyskoy Akademii nauk)

J

  • J-PARC: Japan Proton Accelerator Research Complex
  • JADE: Japan, Deutschland, and England detector at DESY's PETRA, also refers to type of jet algorithm developed by this collaboration
  • JADE: Joint Academic Data-science Endeavour in the UK
  • JAGS: Just Another Gibbs Sampler bayesian analysis code
  • JAM: Jet A--A Microscopic transport model
  • JAXA: Japan Aerospace Exploration Agency
  • JDEM: Joint Dark Energy Mission
  • JEDI: Jülich Electric Dipole moment Investigations collaboration
  • JEM-EUSO: Japan Experiment Modules Extreme Universe Space Observatory
  • JEWEL: Jet Evolution With Energy Loss event generator
  • JET: Topical collaboration on Jet and Electromagnetic Tomography of extreme phases of matter in heavy-ion collisions
  • JETSCAPE: Jet Energy-loss Tomography with a Statistically and Computationally Advanced Program Envelope
  • JGRG: General Relativity and Gravitation in Japan
  • JHF: Japan Hadron Facility
  • JIMWLK: Jalilian-Marian, Iancu, McLerran, Weigert, Leonidov and Kovner
  • JINR: Joint Institute for Nuclear Research in Dubna, Russia
  • JISC: Joint Information Systems Committee
  • JLA: Joint Light-curve Analysis of SDSS and SNLS supernova data
  • JNIPER: Joint Network for Informal Physics Education and Research
  • JPAC: Joint Physics Analysis Center set up by Indiana and JLab
  • JS: Jacobsen and Saleur
  • JSNS2: J-PARC Sterile Neutrino Search at the J-PARC Spallation Neutron Source
  • JSPS: Japan Society for the Promotion of Science
  • JTFI: Joint Task Force Initiative at Fermilab
  • JUNIPR: Jets from UNsupervised Interpretable PRobabilistic models framework
  • JUNO: Jiangmen Underground Neutrino Observatory, formerly Daya Bay
  • JVAS: Jodrell/Very Large Array Astrometric Survey
  • JWST: James Webb Space Telescope
  • JYFL: Jyväskylä Department of Physics (Fysiikan Laitos)

K

  • K2K: KEK to Super-Kamiokande long-baseline neutrino oscillation experiment
  • KAGRA: Kamioka Gravitational Wave Detector
  • KamLAND: Kamioka Liquid Scintillator Anti-Neutrino Detector
  • KamLAND-ZeN: KamLAND Zero Neutrino double beta decay experiment
  • KARMEN: Karlsruhe Rutherford interMediate Energy Neutrino experiment
  • KASCADE: KArlsruhe Shower Core and Array DEtector
  • KATRIN: KArlsruhe TRItium Neutrino experiment
  • KCWI: Keck Cosmic Web Imager
  • KdV: Korteweg and de Vries
  • KEDR: Detector at VEPP, acronym unknown
  • KEK: High Energy Accelerator Research Organization (Ko Enerugi Kasokuki Kenkyu Kiko)
  • KEK-PS: Proton-synchrotron at KEK
  • keVin: keV inert fermion
  • KGBJS: Kutak, Golec-Biernat, Jadach and Skrzypek evolution equation
  • KIC: Kepler Input Catalog of stars
  • KiDS: Kilo-Degree Survey using the VST at ESO
  • KIMS: Korea Invisible Mass Search dark matter experiment
  • KK: Kaluza and Klein
  • KK: Event generator apparently superseding both KORALB and KORALZ, which are apparently not acronyms
  • KKLT: Kachru, Kallosh, Linde, and Trivedi
  • KKMC: Monte Carlo event generator written in Krakow and Knoxville during year 2K-1
  • KL: Kallen and Lehmann
  • KL: K-Long facility proposed at JLab
  • KLASH: KLoe magnet for Axion SearcH proposed experiment at Frascati
  • KLN: Kharzeev, Levin and Nardi model for pre-equilibrium phase
  • KLN: Kinoshita, Lee and Nauenberg cancellations of IR-divergent Feynman diagrams
  • KLOE: K-Long Experiment
  • KLT: Kawai, Lewellen, and Tye relation between open- and closed-string amplitudes
  • KLWMIJ: Kovner, Leonidov, Weigert, McLerran, Iancu and Jalilian-Marian, apparently a different limit of JIMWLK
  • KM3NeT: Cubic Kilometre Neutrino Telescope under construction in the Mediterranean
  • KMMW: Kruczenski, Mateos, Myers and Winters
  • KMR: Khoze, Martin and Ryskin
  • KMR: Kimber, Martin and Ryskin parton distribution formalism
  • KMS: Kubo, Martin and Schwinger
  • KNC: Knights Corner co-processor
  • KNO: Koba, Nielsen and Olesen
  • KNP: Kim, Nilles and Peloso axion inflation model
  • KO: Kugo and Ojima
  • KoMPoST/K0MP0ST/KMPST: Linear kinetic theory code by Kurkela, Mazeliauskas, Paquet, Schlichting and Teaney
  • KoRIA: Korea Rare Iostope Accelerator
  • KOTO: K0 at TOkai experiment
  • KP: Kadomtsev and Petviashvili
  • KPI: Key performance indicator.
  • KPP: Kolmogorov, Petrovsky and Piskunov partial differential equation
  • KPZ: Kardar, Parisi and Zhang equation
  • KREEP: Potassium, rare-earth element and phosphorus component of some lunar rocks
  • KRKMC: NLO Monte Carlo program, acronym unknown, may have something to do with re-inserting LO kernels.
  • KS: Klebanov and Strassler
  • KSRF: Kawarabayashi, Suzuki, Riazuddin and Fayyazudin
  • KSS: Kovtun, Son and Starinets
  • KSVZ: Kim, Shifman, Vainshtein and Zakharov
  • KSW: Kaplan, Savage and Wise
  • KT: Kennedy and Thorndike
  • KTeV: Kaons at the Tevatron
  • KTY: Kimura, Takamura and Yokomakura
  • KvBLL: Kraan, van Baal, Lee and Lu calorons

L

  • L3: Detector at LEP, apparently not an acronym
  • LAB: Linear alkylbenzene
  • LAC: Large Application Compile node
  • LAFEX: High Energy Physics Laboratory of the Universidade do Estado do Rio de Janeiro
  • LAGEOS: Laser Geodynamics Satellites
  • LAGO: Latin American Giant Observatory
  • LAGUNA: Large Apparatus studying Grand Unification and Neutrino Astrophysics
  • LaMET: Large-Momentum Effective field Theory
  • LANL: Los Alamos National Lab
  • LANSCE: Los Alamos Neutron Science Center
  • LapH: Laplacian Heaviside smearing
  • LAPW: Linearized augmented plane wave
  • LARP: LHC Accelerator Research Program
  • LArIAT: Liquid Argon In A Testbeam neutrino experiment at Fermilab
  • LArTPC: Liquid Argon Time Projection Chambers
  • LASAGNA: Lepton Asymmetric Sterile--Active momentum-Grid Neutrino Analyser adaptive ODE solver
  • LASS: Large Acceptance Solenoid Spectrometer at SLAC
  • LAT: Large Area Telescope
  • LBNE: Long Baseline Neutrino Experiment
  • LBNF: Long-Baseline Neutrino Facility
  • LBNO: Long Baseline Neutrino Observatory
  • LBT: Linear Boltzmann Transport model and corresponding event generator
  • LCC: Linear Collider Collaboration
  • LCD: Linear Collider Detector project at CERN
  • LCE: Large cut-off effects regime of chiPT
  • LCG: Light cone gauge
  • LCLS: Linac Coherent Light Source at SLAC
  • LCQ: Light cone quantization
  • LCWF: Light-cone wave function
  • LDA: Local density approximation
  • LDAP: Lightweight Directory Access Protocol
  • LDM: Light dark matter
  • LDME: Long-distance matrix element
  • LDMX: Light Dark Matter eXperiment proposed at SLAC
  • LDRD: Laboratory Directed Research and Development at Livermore
  • LEAR: Low Energy Antiproton Ring at CERN
  • LEBC: LExan Bubble Chamber at CERN
  • LeCosPA: Leung Center for Cosmology and Particle Astrophysics
  • LEDA: Library of Efficient Data types and Algorithms
  • LEGEND: Large Enriched Germanium Experiment for Neutrinoless ββ Decay and Gran Sasso
  • LENA: Low Energy Neutrino Astronomy liquid scintillator
  • LEPS: Laser Electron Photon Experiment at SPring-8
  • LESA: Lepton-number Emission Self-sustained Asymmetry [dipole neutrino minus antineutrino]
  • LETI: Laboratoire d'électronique des technologies de l'information of CEA
  • LFD: Light-front dynamics
  • LFI: Low frequency instrument
  • LFQM: Light front quark model
  • LFV: Lepton flavor violation
  • LHAASO: Large High Altitude Air Shower Observatory planned for Yangbajing, Tibet
  • LHAPDF: Les Houches Accord Parton Density Functions
  • LHCC: Large Hadron Collider Committee
  • LHCO: Standardized detector simulator output format
  • LHCHXSWG: Large Hadron Collider Higgs Cross Section Working Group
  • LHeC: Large Hadron-electron Collider
  • LHEF: Les Houches Event File format
  • LHPC: Lattice Hadron Physics Collaboration
  • LHT: Littlest Higgs model with T-parity
  • Li_n: Polylogarithm
  • LIFE: Laser Inertial Fusion Energy
  • LIGO: Laser Interferometer Gravitational Wave Observatory
  • LILITH: LIght LIkelihood fiT for the Higgs Python tool for constraining new physics from signal strength measurements
  • LIME: Lattice QCD Interchange Message Encapsulation format
  • LIPSS: Light Pseudoscalar and Scalar Search
  • LISA: Laser Interferometer Space Antenna
  • LISHEP: LAFEX International School on High Energy Physics
  • LiteBIRD: Lite (Light) satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection
  • LiteRed: A tool for the Loop InTEgrals REDuction
  • LKF: Landau, Khalatnikov and Fradkin transformations relating n-point functions in different gauges
  • LKP: Lightest Kaluza-Klein particle
  • LLAMA: Large Latin American Millimeter Array radio telescope in Argentina
  • LLESA: Livermore Laboratory Employee Services Association
  • LLNS: Lawrence Livermore National Security, LLC
  • LLR: Langfeld, Lucini and Rago
  • LLRF: Low-level radio frequency
  • LLVM: Compiler infrastructure project formerly named Low Level Virtual Machine
  • LMA: Large mixing angle solution of the solar neutrino problem
  • LMC: Large Magellanic Cloud
  • LME: Large mass expansion
  • LMP: Lu, Mei and Pope
  • LMXB: Low-mass X-ray binary
  • LNF: Laboratori Nazionali di Frascati, INFN
  • LNGS: Laboratori Nazionali del Gran Sasso
  • LNV: Lepton number violation
  • LOFAR: Low-Frequency Array interferometer
  • LOOL: Leading-order one-loop
  • LOFF: Larkin, Ovchinnikov, Fulde and Ferrel
  • LORRI: LOng-Range Reconnaissance Imager on the New Horizons mission to Pluto
  • LOSP: Lightest Ordinary Supersymmetric Particle
  • LPM: Landau, Pomeranchuk and Migdal
  • LPSC: Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
  • LQC: Loop Quantum Cosmology
  • LOFT: Large Observatory For X-ray Timing proposed ESA mission
  • LQG: Loop Quantum Gravity
  • LRG: Luminous red galaxies
  • LRTH: Left--right twin Higgs model
  • LRZ: Leibniz-Rechenzentrum near Munich
  • LSB: Low Surface Brightness
  • LSCO: Lanthanum copper oxide
  • LSDS: Lead Slowing Down Spectrometer at LANL
  • LSF: Light-quark spin--flavor symmetry
  • LSND: Liquid Scintillator Neutrino Detector at the Los Alamos Meson Physics Facility
  • LSP: Lightest supersymmetric particle
  • LSS: Large-scale structure
  • LSST: Large Synoptic Survey Telescope
  • LSZ: Lehmann, Symanzik and Zimmermann
  • LTB: Lemaître, Tolman and Bondi
  • LTD: Loop--tree duality
  • LTI: Learning Tools Interoperability in Canvas
  • LUCIAE: Hadron and string cascade model, acronym meaning unknown
  • LUPM: Laboratoire Univers et Particules de Montpellier
  • LUX: Large Underground Xenon dark matter experiment
  • LVD: Large Volume Detector neutrino experiment at Gran Sasso
  • LVS: Large volume scenario
  • LXCDM: Cold dark matter model with variable cosmological term Lambda and dynamical cosmon X
  • LZ: LUX-ZEPLIN

M

  • MACRO: Monopole, Astrophysics and Cosmic Ray Observatory
  • MADMAX: MAgnetized Disc and Mirror Axion eXperiment dielectric haloscope
  • MAGIC: Major Atmospheric Gamma Ray Imaging Cherenkov telescope
  • MAGIC: Mathematics Access Grid Instruction and Collaboration project
  • MagICAL: Magnetized Iron CALorimeter detector under construction for INO
  • MAGIS: Mid-band Atomic Gravitational-wave Interferometric Sensor
  • MAID: Mainz Analysis Interactive Dial-in
  • MALBEK: Majorana Low-background BEGe detector at Kimballton
  • MAMI: Mainz Microtron
  • mAMSB: Minimal anomaly-mediated supersymmetry breaking model
  • MAOS: M_T2-Assisted On-Shell momentum
  • MAP: Muon Accelerator Program
  • MAPT: Massless Analytic Perturbation Theory
  • MARTINI: Modular Algorithm for Relativistic Treatment of heavy IoN Interactions
  • MATHUSLA: MAssive Timing Hodoscope for Ultra Stable neutraL pArticles proposed surface detector at CERN
  • MATTER: Modular All-Twist Transverse and Elastic scattering induced Radiation event generator
  • MaVaN: Mass-varying neutrino
  • MAXI: Monitor of All-sky X-ray Image experiment on the International Space Station
  • MAXIMA: Millimeter Anisotropy eXperiment IMaging Array balloon-borne CMB telescope
  • MBR: Minimum Bias Rockefeller model of cross sections
  • MCC: Machine Control Center at JLab
  • MCFL: Magnetic-color-flavor-locked phase
  • MCFM: Monte Carlo for FeMtobarn processes
  • MCPMFV: Maximally CP- and Minimally Flavour-Violating
  • MCT: Contransverse mass kinematic variable
  • MCT2: Constransverse mass kinematic variable
  • MCPM: Maximally CP-symmetric two-Higgs-doublet Model
  • MDI: Momentum-dependent interaction
  • MDM: Matrix decomposition method
  • MDM: Michigan, Dartmouth and MIT observatory on Kitt Peak
  • MDS: Metadata Server in Lustre system
  • ME: Matrix element
  • MEC: Meson-exchange current
  • MEG: Mu to E Gamma experiment at PSI
  • MEGA: Mu to E GAmma experiment at Los Alamos
  • MEGa-ray: Mono-energetic gamma-ray at Livermore
  • MEIC: Medium-energy Electron--Ion Collider under consideration for Jlab or Brookhaven
  • MEKS: Modified Ellis, Kunszt and Soper code?
  • MELA: Matrix Element Likelihood Analysis
  • MEM: Matrix element method
  • MEM: Maximum entropy method
  • MEMO: Metastable exotic multi-hypernuclear object
  • MENLOPS: Matrix Element plus Next-to-Leading Order Parton Shower
  • MEPHI: Moscow Engineering Physics Institute
  • MEPS: Matrix Element plus Parton Shower
  • MERA: Multi-scale Entanglement Renormalization Ansatz
  • MERLIN: Multi-Element Radio Linked Interferometer Network
  • MESA: Mainz Energy Recovery Superconducting Accelerator
  • MESA: Modules for Experiments in Stellar Astrophysics stellar evolution code
  • MESE: Medium Energy Starting Events at IceCube
  • MEtop: Single-top production generator, acronym unknown
  • MFV: Minimal flavor violation
  • MFT: Mean field theory
  • mGMSB: Minimal gauge-mediated supersymmetry breaking
  • MGS: Mars Global Surveyor
  • MHV: Maximal helicity violation
  • MIAN: Steklov Mathematical Institute of the Russian Academy of Sciences (Matematicheskiy Institut Akademiya Nauk)
  • MIAPP: Munich Institute for Astro- and Particle Physics
  • MIB: Minimal integrity basis for polynomials of order parameters
  • MIC: Multiprogrammatic and Institutional Computing at Livermore
  • MICE: Muon Ionization Cooling Experiment
  • MicrOMEGAs: Program for calculating dark matter properties (including the relic density Omega h^2), apparently not an acronym
  • MICROSCOPE: MICRO-Satellite à traînée Compensée pour l'Observation du Principe d'Equivalence
  • MiDM: Magnetic inelastic Dark Matter
  • MIKE: Magellan Inamori Kyocera Echelle spectrograph
  • Milagro: Gamma-ray observatory, Spanish for "miracle", not an acronym but sometimes treated as such
  • MIMAC: MIcro TPC MAtrix of time projection Chambers for dark matter directional detection
  • MIND: Magnetized Iron Neutrino Detector
  • MINERVA: Main Injector Experiment for nu--A at Fermilab
  • MiNLO: Multi-scale improved next-to-leading order method
  • MINOS: Main Injector Neutrino Oscillation Search
  • MINSIS: Main Injector Non-Standard Interaction Search
  • MIPP: Main Injector Particle Production experiment at Fermilab
  • MIRO: Microwave-Induced Resistance Oscillations
  • MISC: Maskawa Institute for Science and Culture at Kyoto Sangyo University
  • MiXDM: Multiple states for inelastic and exciting dark matter
  • MKL: Intel Math Kernel Library
  • MLC: Mandelbrot Locally Connected conjecture
  • MLF: Material and Life Science Experimental Facility at J-PARC
  • MLM: M. L. Mangano
  • MLS: Minimal Length Scenario
  • MMCP: Mathematical Modeling and Computational Physics
  • MMHT: Martin, Motylinski, Harland-Lang and Thorne parton distributions
  • MNS: Maki, Nakagawa and Sakata
  • MO: Muskhelishvili and Omnes
  • MoEDAL: Monopole and Exotics Detector At the LHC
  • MOLLER: Moller scattering experiment at Jlab, not an acronym
  • MOMENT: MuOn-decay MEdium baseline NeuTrino beam experiment
  • MOND: Modified Newtonian Dynamics
  • MonteCUBES: Monte Carlo Utility Based Experiment Simulator
  • MoS2: Molybdenum disulfide
  • MOS: Metal oxide semiconductor (or silicon) cameras on XMM-Newton
  • MPD: Multi-Purpose Detector at NICA at JINR
  • MPG: Max Planck Gesellschaft (society)
  • MPI: Message Passing Interface
  • MPI: Multiple parton interactions
  • MPQ: Max-Planck-Institut für Quantenoptik
  • MPS: Matrix product states
  • MPS: Multiparticle spectrometer at Fermilab in the 1980s
  • MPT: Modified perturbation theory
  • mQ: Millicharged particles (and a proposed search for them in hep-ex/9804008)
  • MRI: Major Research Instrumentation program of the NSF
  • MRPC: Multigap Resistive Plate Chamber
  • MRAM: Magnetoresistive random access memory, or magnetic random access memory
  • MRS: Materials Research Society
  • MRSSM: Minimal R-symmetric supersymmetric standard model
  • MRST: A. D. Martin, R. G. Roberts, W. J. Stirling, and R. S. Thorne
  • MRW: Martin, Ryskin and Watt parton distribution formalism
  • MS: Magueijo and Smolin
  • MSbar: Modified Minimal Subtraction
  • MSR: Renormalization scheme claimed to be the simplest extension of MSbar to renormalization scales R << m_Q
  • MSSM: Minimal supersymmetric standard model
  • MSSU(5): Minimal supersymmetric SU(5) model
  • MST: Madison Symmetric Torus
  • MSTW: A. D. Martin, W. J. Stirling, R. S. Thorne, and G. Watt
  • mSUGRA: Minimal supergravity
  • MSW: Mikheev, Smirnov, and Wolfenstein
  • MT: Mathematica package to compute convolutions based on Mellin transforms
  • MT2: Stransverse mass kinematic variable (similar to transverse mass)
  • MTV: NNSA Consortium for Monitoring, Technology, and Verification
  • mu distortion of the CMB represents deviations from ideal black body radiation due to imperfect thermalization of energy dissipated from density fluctuations, which can be treated as an effective chemical potential
  • MUC: Munich airport code, applied to nearby supercomputer
  • muDAR: muon Decay At Rest
  • MUED: Minimal Universal Extra Dimension model
  • Mueller--Navelet jets are characterized by high p_T and large rapidity separation
  • MuLan: Muon Lifetime Analysis experiment at PSI
  • MUNU: Experiment measuring the neutrino magnetic moment
  • munuSSM: "mu from nu" supersymmetric standard model, in which the mu problem is solved by introducing right-handed neutrinos
  • MuPs: Muonium-positronium (mu+ e- e- e+)
  • MURMUR: Low-noise neutron-passing-through-walls experiment, acronym unknown but potentially related to the University of Namur
  • MUSE: Multi Unit Spectroscopic Explorer for ESO's VLT
  • MUSIC: MUSCL for Ion Collisions program
  • MUSCL: Monotone Upstream-centered Schemes for Conservation Laws
  • MUST: Tool to detect MPI usage errors, apparently not an acronym
  • MVA: Multi-variate analysis

N

  • N2HDM: Next-to-Two-Higgs-Doublet Model with a real singlet in addition to the second doublet
  • NAdS: Nearly anti-de Sitter
  • NAHE: Nanopoulos, Antoniadis, Hagelin and Ellis
  • NaI(Tl): Sodium iodide doped with thallium
  • NAMD: Not (just) Another Molecular Dynamics program
  • NANOGrav: North American Nanohertz Observatory for Gravitational Waves pulsar timing array
  • NBS: Nambu, Bethe and Salpeter
  • NCCP: Non-compact complex projective model in SU(N)/U(N-1)
  • NCEL: Neutral-current elastic cross section
  • NCh: Non-uniform chiral phase
  • NCQ: Number of constituent quarks
  • NCRM: UK National Centre for Research Methods
  • NCSC: UK National Cyber Security Centre
  • NCSL: National Superconducting Cyclotron Laboratory
  • nCTEQ: nuclear Coordinated Theoretical--Experimental Project on QCD
  • NDR: Naive dimensional regularization, with implicit MSbar subtraction
  • NDS: nHYP Dislocation Suppressing action
  • NEC: Null energy condition
  • NEFT: Nuclear effective field theory
  • NEMO: Neutrino Ettore Majorana Observatory
  • NEOS: Neutrino Experiment for Oscillation at Short baseline in Korea
  • NERSC: National Energy Research Scientific Computing Center
  • NESSiE: Neutrino Experiment with SpectrometerS in Europe, proposed for CERN and/or Fermilab
  • NESTA: UK charity, formerly National Endowment for Science, Technology and the Arts
  • NESTOR: Neutrino Extended Submarine Telescope with Oceanographic Research
  • NeurIPS: Neural Information Processing Systems conference
  • NEUT: Neutrino interaction simulation library, apparently not an acronym
  • NEWSdm: Nuclear Emulsions for WIMP Search---directional measurement
  • NeXSPheRIO: Hydrodynamics code combining NeXuS and SPheRIO
  • NEXT: Neutrino Experiment with a Xenon Time projection chamber
  • NExT: New connections between Experiment and Theory Institute
  • NeXuS: Hadronic interaction model, apparently replaced by EPOS
  • NFS: Network File System
  • NFT: Network File Transport utility at Livermore
  • NFW: Navarro, Frenk and White
  • NGC: New General Catalogue of galaxies
  • NGO: New Gravitational wave Observatory, also known as eLISA
  • NHDM: N-Higgs-doublet model
  • NIC: Network Interface Card
  • NICA: Nuclotron-based Ion Collider fAcility at JINR
  • NICODEMOS: Numerical Integration with COntour DEformation and MOdular Subtractions
  • NIF: National Ignition Facility
  • NISQ: Noisy Intermediate-Scale Quantum technology
  • NLCWF: Nonstandard light-cone wave function
  • NLEFT: Nuclear Lattice Effective Field Theory
  • NLOPS: Next-to-Leading Order Parton Shower
  • NMC: New Muon Collaboration
  • NME: Nuclear matrix element
  • NMFV: Non-minimal flavor violation
  • NMHV: Next-to-maximal helicity violation
  • NML: (Former) New Muon Lab at Fermilab
  • NMR: Nuclear magnetic resonance
  • NMSGUT: New Minimal Supersymmetric Grand Unified Theory
  • nNJL: Non-local Nambu and Jona-Lasinio model
  • NNMSM: Next to new minimal standard model
  • NNPDF: Collaboration using Neural Networks to calculate Parton Distribution Functions
  • NNSA: National Nuclear Security Administration
  • NOAA: National Oceanic and Atmospheric Administration
  • NOMAD: Neutrino Oscillation MAgnetic Detector at CERN
  • NORDITA: Nordic Institute for Theoretical Physics, Nordisk Institut for Teoretisk (Atom)fysik in Danish
  • NOvA: NuMI Off-axis electron-neutrino Appearance experiment
  • NOW: Neutrino Oscillation Workshop
  • NPA: Nuclear Physics in Astrophysics
  • NPDF: Nuclear Parton Distribution Functions
  • NPDGamma: Neutron--Proton to Deutron--Photon experiment to measure parity-violating asymmetry and pion--nucleon weak coupling
  • nPI: n-particle irreducible
  • NPQMSSM: Next-to-minimal supersymmetric standard model forced to solve the strong CP problem
  • NRAO: National Radio Astronomy Observatory, an NSF facility
  • NRGR: Non-relativistic general relativity
  • NRHEP: Numerical Relativity and High Energy Physics
  • nrMSSU(5): Minimal supersymmetric SU(5) model completed with flavor-dependent nonrenormalizable operators
  • NS: Neveu and Schwarz
  • NS: Non-singlet
  • NSI: Non-standard (neutrino) interaction
  • NSPT: Numerical Stochastic Perturbation Theory
  • NSR: Neveu, Schwarz and Ramond
  • NSSC: NNSA Nuclear Science and Security Consortium
  • NSUSY: Natural supersymmetry
  • NSVZ: Novikov, Shifman, Vainshtein and Zakharov
  • NUGHM: Non-universal gaugino and Higgs mass susy models
  • NUHM: Non-universal Higgs mass susy models
  • NUMA: Non-Uniform Memory Access
  • NuMI: Neutrinos at the Main Injector
  • nuMSM: Neutrino Minimal Standard Model including three sterile right-handed neutrinos
  • nuNMSM: Neutrino Next-to-Minimal Standard Model that also adds a scalar singlet
  • NuPECC: Nuclear Physics European Collaboration Committee
  • nuPIL: Neutrinos from a PIon beam Line design proposed for DUNE
  • NuQS: Collaboration acronym unknown but probably related to nuclear quantum simulations
  • NURT: NUclear and Related Technologies
  • NuSea: Nucleonic Sea asymmetry measurement experiment
  • NuSOnG: Neutrino Scattering On Glass
  • NuSTAR: Nuclear Spectroscopic Telescope Array
  • NuSTEC: Neutrino Scattering Theory Experiment Collaboration
  • nuSTORM: Neutrinos from STORed Muons
  • NUT: Newman, Unti and Tamburino
  • NuTeV: Neutrinos at the Tevatron
  • NuWro: Wroclaw Neutrino Event Generator
  • NVSS: NRAO Very Large Array Sky Survey

O

  • OAM: Orbital angular momentum
  • OBEP: One-boson-exchange potential for nuclei
  • ODA: Official Development Assistance
  • ODLRO: Off-diagonal long-range order
  • OGE: One-gluon exchange
  • OGLE: Optical Gravitational Lensing Experiment
  • OHe: Dark matter model of a lepton-like doubly charged particle O bound with a primordial helium nucleus
  • OISSO: Organizational Information System Security Officer
  • OKA: Experiments with Kaons in Russian
  • OME: Operator matrix element
  • OMEG: Origin of Matter and Evolution of Galaxies symposia
  • O'Mega: Optimizing Matrix Element Generator compiler
  • OMEGA EP: OMEGA extended performance; OMEGA is a high-power ultraviolet laser, and doesn't seem to be an acronym
  • OPAL: Omni Purpose Apparatus for LEP
  • OPE: Operator product expansion
  • OPERA: Oscillation Project with Emulsion-tRacking Apparatus at LNGS
  • OPP: Ossola, Papadopoulos and Pittau
  • OPUCEM: Oblique Parameters Using C with Error-checking Machinery code
  • ORCA: Oscillation Research with Cosmics in the Abyss proposed neutrino detector
  • ORCID: Open Researcher and Contributor ID
  • ORKA: The Golden KAon Decay experiment proposed at Fermilab
  • ORNL: Oak Ridge National Lab
  • OSB: Observational Science Board of the Einstein Telescope
  • OSCAR: Open Standard Codes and Routines
  • OscSNS: Experiment to search for sterile neutrino oscillations using the Spallation Neutron Source at Oak Ridge
  • OSQAR: Optical Search of QED vacuum magnetic birefringence, Axion and photon Regeneration experiment at CERN
  • OSG: Open Science Grid
  • OSI: Open Systems Interconnection model
  • OSIRIS-REx: Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer NASA asteroid sample-return mission
  • OSS: Lustre Object Storage Server
  • OST: Lustre object storage targets
  • OSTI: DOE Office of Scientific and Technical Information
  • OTO: Out-of-time-ordered correlators
  • OTS: Open Terminal Server
  • OWL: One Way Link
  • OWL: OverWhelmingly Large telescope of ESO
  • OZI: Okubo, Zweig and Iizuka

P

  • P5: Particle Physics Project Prioritization Panel
  • PAC: Program Advisory Committee at JLab
  • PACIAE: partonic and hadronic cascade model, acronym meaning unknown
  • PACIFIC: Particle Astrophysics and Cosmology Including Fundamental InteraCtions
  • PACS-CS: Parallel Array Computer System for Computational Sciences
  • PADME: Positron Annihilation into Dark Matter Experiment at Frascati
  • PAMELA: Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics
  • PANDA: antiProton ANnihilations at DArmstadt experiment at FAIR
  • PandaX: Liquid xenon dark matter experiment in China (CJPL), apparently not an acronym
  • PANIC: Particles and Nuclei International Conference
  • PanSTARRS: Panoramic Survey Telescope and Rapid Response System
  • PArthENoPE: Public Algorithm Evaluating the Nucleosynthesis of Primordial Elements
  • PARTICLEFACE: COST Action "Unraveling new physics at the LHC through the precision frontier", apparently not an acronym
  • PASC: Swiss Platform for Advanced Scientific Computing
  • PASEP: Partially asymmetric simple exclusion process
  • PAX: Polarized Antiproton eXperiments
  • PBH: Primordial black hole
  • PCA: Principal component analysis
  • PCIe: Peripheral Component Interconnect Express
  • PDS: Power divergence subtraction scheme
  • PEARC: Practice and Experience in Advanced Research Computing conference
  • PEB: Polarized electron beam
  • PEMD: Power electronics, machines and drives
  • PEN: Pion to e+nu experiment at PSI
  • PEP: Positron Electron Project at SLAC
  • PEPS: Projected entangled pair states tensor network method
  • PERKEO: Superconducting cold neutron beta-decay spectrometers at ILL, acronym unknown
  • PETRA: Positron-Electron Tandem Ring Accelerator at DESY
  • PFH: PAMELA, Fermi and HESS
  • PFX: Procedures for Researchers document at Fermilab
  • PGS: Pretty Good Simulation of high energy collisions
  • PHEGAS: A phase space generator for automatic cross-section computation
  • PHENIX: Pioneering High Energy Nuclear Interaction eXperiment at RHIC
  • PhET: Physics Education Technology
  • PHHQP: Pseudo-Hermitian Hamiltonians in Quantum Physics
  • PHOBOS: RHIC experiment, not an acronym, but a reference to a moon of Mars
  • PHOKHARA: Event generator including NLO QED effects, apparently not an acronym
  • PHSD: Parton-Hadron-String Dynamics transport model
  • PHY: The physical layer of the OSI model
  • PhySyHCAl: A Physics System based on Hierarchical Computer Algebra
  • PIBETA: Pion Beta experiment at PSI
  • PIC: Physics in Collision
  • PICASSO: Project in Canada to Search for Supersymmetric Objects, or Projet d'Identification de CAndidats Supersymétriques SOmbres at SNO
  • PICO: PICASSO + COUPP
  • PIDM: Planckian Interacting Dark Matter
  • PiENu: Pion decay experiment at TRIUMF
  • PINGU: Precision IceCube Next Generation Upgrade
  • PIP: Proton Improvement Plan at Fermilab
  • PIXIE: Primordial Inflation Explorer polarimeter
  • PJFry: Tensor reduction code, acronym unknown
  • PKS: Parkes observatory in Australia, and the radio catalog it produced
  • PLaIn LQCD: Lambda Cold Dark Matter with Power-LAw INflation
  • PLANCK: CMB satellite experiment; not an acronym, though sometimes treated as such
  • PLC: Photon linear collider
  • PLQCD: PRACE Lattice QCD library
  • pMSSM: Phenomenological Minimal Supersymmetric Standard Model
  • PMNS: Pontecorvo, Maki, Nakagawa and Sakata
  • PNDME: Precision Neutron Decay Matrix Elements collaboration
  • PNJL: Polyakov, Nambu and Jona-Lasinio
  • pNRQCD: Potential nonrelativistic QCD
  • POEMMA: Probe of Extreme Multi-Messenger Astrophysics NASA mission
  • PolarBeaR: Polarization of Background Radiation
  • POLARIS: Petawatt Optical Laser Amplifier for Radiation Intensive Experiments
  • POT: Protons on target
  • POWHEG: POsitive Weight Hardest Emission Generator
  • POWHEG BOX: Automatic implementation of POWHEG for generic NLO processes, apparently not an acronym
  • PowHel: Framework combining the POWHEG-Box with the HELAC-NLO package
  • PPAC: Parallel-plate avalanche counter
  • PPAP: STFC Particle Physics Advisory Panel
  • PPB: Polar Patrol Balloon
  • PPC: International Conference on Interconnections between Particle Physics and Cosmology
  • PPF: Pisano, Pleitez and Frampton
  • PPM: Piecewise Parabolic Method
  • PQ: Peccei and Quinn
  • POLARBEAR: CMB polarization experiment in Chile, apparently not an acronym
  • PQWW: Peccei, Quinn, Weinberg and Wilczek
  • PRACE: Partnership for Advanced Computing in Europe
  • PrimEx: Primakoff Experiment at Jlab
  • PRISM: Polarized Radiation Imaging and Spectroscopy Mission proposed to ESA
  • PRISMA: PRecision physics, fundamental Interactions and Structure of MAtter Cluster of Excellence at Mainz
  • PROPOSAL: PRopagator with Optimal Precision and Optimized Speed for All Leptons code
  • PROSA: PROton Structure Analyses in hadronic collisions collaboration
  • PROSPECT: A PRecision Oscillation and SPECTrum Experiment at Oak Ridge
  • PS: Pure-singlet
  • PSA: Phase-shift analysis
  • PSCz: Point Source Catalogue of redshifts from IRAS
  • PSI: Paul Scherrer Institut
  • PSL: Projective special linear group
  • PSLQ: Integer relation algorithm based on a Partial Sum of square implemented with a LQ (lower trapezoidal-orthogonal) matrix factorization
  • PSR: Pulsating Source of Radio (i.e., a pulsar)
  • PSRB: Professional, Statutory and Regulatory Bodies
  • PSRE: Public-Sector Research Establishment
  • PSXE: Intel Parallel Studio version
  • PT: Pinch technique
  • PTOLEMY: Princeton Tritium Observatory for Light, Early-universe, Massive-neutrino Yield
  • PTX: Parallel Thread Execution assembly-like language
  • PV: Parity-violating
  • PV: Principal value, used in regularization schemes
  • PVA4: Parity Violating Asymmetry experiment in hall 4 at MAMI
  • PVLAS: Polarizzazione del Vuoto con LASer
  • PWA: Partial wave analysis
  • PWMM: Plane Wave Matrix Model
  • PWNe: Pulsar Wind Nebulae
  • PyR@TE: Python Renormalization group equations At Two-loop for Everyone
  • PYTHIA: An event generator named after the Oracle of Delphi

Q

  • QCD_AS: QCD with quarks in the two-index anti-symmetric representation
  • QCDF: QCD factorization
  • QCDM: Quintessence Cold Dark Matter cosmological model
  • QCDSF: German lattice collaboration, acronym meaning unknown (related to SFB?)
  • QFEXT: Quantum field theory under the influence of external conditions
  • QGP: Quark--gluon plasma
  • QGS or QGSM: Quark--gluon string model
  • QHD: Quantum haplodynamics
  • QISM: Quantum Inverse Scattering Method
  • QJT: Quantum Jet Theory
  • QKD: Quantum key distribution
  • QLM: Atos Quantum Learning Machine
  • QMC: Quark-meson coupling
  • QMRK: Quasi-multi-Regge kinematics
  • QNM: Quasinormal mode
  • QPA: Quasiparticle approximation
  • QPACE: QCD Parallel Computing on the Cell Broadband Engine
  • QPE: Quantum phase estimation
  • QPIC: Quantum Photonics Integrated Circuit
  • QRPA: Quasiparticle random phase approximation
  • QSO: Quasi-stellar objects (quasars)
  • QSSR: QCD spectral sum rules
  • QTEC: Quantum Technology Enterprise Centre at Bristol
  • QTIC: Quantum Technologies Innovation Centre at Bristol
  • QTS: Quantum Theory and Symmetries
  • QUaD: QUEST at DASI
  • QuantEmX: Quantum Emergence Exchange
  • QUASAR: Quantum Systems and advanced Accelerator Research group
  • QUASAR: Proposed Quasi-Axisymmetric Stellarator Research facility
  • QUAX: QUaerere AXion ("search axion") proposal
  • QUBIC: Q and U Bolometric Interferometer for Cosmology observatory in Argentina
  • QUEST: Q and U Extragalactic Sub-mm Telescope
  • QUEST: Quantum Enhanced Superfluid Technologies for dark matter and cosmology
  • QUEST: Quasar/ULIRG Evolution STudy experiment
  • QuIC: European Quantum Industry Consortium
  • QUIET: Q/U Imaging ExperimenT (Q and U are Stokes parameters)

R

  • RAD: Rapidity anomalous dimension
  • RADES: Relic Axion Detector Exploratory Setup
  • RADICAL: Research in Advanced Distributed Cyberinfrastructure and Applications
  • RAID: Redundant array of inexpensive disks
  • RAL: STFC Rutherford Appleton Laboratory near Oxford
  • RAMBO: RAndom Momenta BOoster multi-particle phase space generator
  • RAMSES: Adaptive Mesh Refinement code for self-gravitating magnetized fluid flows, apparently not an acronym
  • RAN: Radio Access Network
  • RAS: Russian Academy of Sciences
  • RAVE: RAdial Velocity Experiment star survey
  • RC: Renormalization constant
  • RCMM: Liverpool's Research Centre in Mathematics and Modelling
  • RCNP: Research Center for Nuclear Physics at Osaka University
  • rcBK: Running coupling Balitsky and Kovchegov
  • RChL: Resonance chiral lagrangian
  • RChT: Resonance chiral theory
  • RCS: Rapid cycling synchrotron at J-PARC
  • RDM: Relativistic diffusion model
  • RDMA: Remote direct memory access
  • RDMS: Russia and Dubna Member States
  • RECOLA: REcursive Computation of One-Loop Amplitudes
  • RENO: Reactor Experiment for Neutrino Oscillation at Yeonggwang, Korea
  • REST: Representational State Transfer
  • REWSB: Radiative electroweak symmetry breaking
  • RFT: Reggeon Field Theory
  • RGE: Renormalization group equation
  • RGI: Renormalization group improvement (NOT invariant)
  • RGI: Renormalization group invariant
  • RGW: Relic gravitational wave
  • RGZ: Refined Gribov and Zwanziger formalism
  • RHIC: Relativistic Heavy Ion Collider
  • RHN: Right-handed neutrino
  • RI/MOM: Regularization-independent momentum subtraction renormalization scheme
  • RI/SMOM: Regularization-independent symmetric-momentum subtraction renormalization scheme
  • RIB: Radioactive ion beam
  • RICAP: Roma International Conference on Astro-Particle physics
  • RIDE: Radiative Inflation and Dark Energy
  • RIKEN: Japanese Institute of Physical and Chemical Research (Rikagaku Kenkyusho)
  • RIPPER: Repeated. Incremental Pruning to Produce Error Reduction (data mining algorithm)
  • RIVET: Robust Independent Validation of Experiment and Theory toolkit
  • RL: Reinforcement (machine) learning
  • RMACC: Rocky Mountain Advanced Computing Consortium
  • RMF: Relativistic mean-field framework
  • RMS: Robertson, Mansouri and Sexl
  • RMS: Root-mean-square
  • RN: Reissner and Nordstrom
  • RNP: International Workshop Relativistic Nuclear Physics from Hundreds of MeV to TeV
  • RNS: Ramond, Neveu and Schwarz superstring
  • RnuMDM: Model relating radiative seesaw and minimal dark matter mass scales with only SM gauge group
  • ROC: Receiver operating characteristic of signal efficiency as function of background efficiency
  • ROC: Remote operations center
  • ROCm: Radeon Open Compute platform
  • ROI: Rest observer at infinity
  • ROSAT: Röntgen Satellite (1990s X-ray observatory)
  • RP: Reaction plane
  • RP: Real projective space
  • RPA: Random phase approximation
  • RPV: R-parity violating
  • RQED: Dimensionally reduced quantum electrodynamics
  • RQM: Relativistic quantum mechanics
  • RR: Ramond--Ramond
  • RRTF: Rapid Reaction Task Force
  • RSA: Rivest, Shamir and Adleman encryption algorithm
  • RSc: Randall-Sundrum model with custodial protection
  • RSD: Redshift Space Distortion measurement relevant to dark matter
  • RSOS: Restricted solid-on-solid
  • RSS: Royal Statistical Society
  • RTG: Radioisotope thermoelectric generators
  • RTN: Reconfigurable Transputer Network
  • RTN: Research Training Network
  • RTO: Research and Technology Organisation
  • RUEDI: Relativistic Ultrafast Electron Diffraction and Imaging Facility
  • RVB: Resonating valence bond
  • RWP: Radiation Work Permit
  • RWTH: Rheinisch-Westfaelische Technische Hochschule
  • RX-DMFIT: Radio and X-ray extension of the gamma-ray fitting tool DMFIT
  • RXTE: Rossi X-ray Timing Explorer

S

  • S&FE: Schools and Further Education committee of the IMA
  • SAB: Strategic Advisory Board
  • SACOT: Simplified ACOT renormalization scheme
  • SAdS: Schwartzchild anti-de Sitter
  • SAGE: Soviet-American Gallium Experiment
  • SAID: Scattering Analysis Interactive Dial-in
  • SAIP: South African Institute of Physics
  • SAMPLE: Parity-violating electron scattering experiment at MIT, acronym unknown
  • SAMURAI: Scattering AMplitudes from Unitarity-based Reduction Algorithm at the Integrand level
  • SANC: Support of Analytic and Numeric Calculations for Experiments at Colliders
  • SAP: Schwarz alternating procedure
  • SAPHIR: Spectrometer Arrangement for Photon induced Reactions experiment at ELSA
  • SAPPHiRE: Small Accelerator for Photon-Photon Higgs production using Recirculating Electrons
  • SARAH: Mathematica package for building and analyzing (not only) supersymmetric theories, apparently not an acronym
  • SAS: Small Astronomical Satellite
  • SAS: Statistical Analysis System developed by Statistical Analysis Software
  • SB&F: Science Books & Films project of AAAS
  • SBND: Short-Baseline Near Detector for neutrinos at Fermilab
  • SBRI: Small Business Research Initiative in the UK
  • SCaN: Space Communications and Navigation program at NASA
  • SCET: Soft collinear effective theory
  • SCET_G: Soft-collinear effective theory with Glauber gluons
  • SCF: Strong color fields
  • SciBooNE: SciBar Booster Neutrino Experiment
  • Scotogenic: Caused by darkness (dark matter or dark energy)
  • SPAM: State preparation and measurement errors in quantum computing
  • SPSC: SPS and PS experiments Committee
  • SD: Single diffraction
  • SDE: Schwinger--Dyson equation
  • SdS: Schwarzschild and de Sitter
  • SDSS: Sloan Digital Sky Survey
  • SDWI: Strongly dissipative warm inflation
  • SecDec: Sector decomposition
  • SED: Spectral energy distribution
  • SELEX: Segmented Large X baryon spectrometer at Fermilab
  • SELFAS: Simulation of ELectric Field emitted by Air Shower program
  • SENSEI: Sub-Electron-Noise Skipper-CCD Experimental Instrument
  • SESAME: Synchrotron-light for Experimental Science and Applications in the Middle East
  • SET: Symmetry-enriched topological order
  • SET: Strategic Energy Technology
  • SFB: Sonderforschungsbereich (Collaborative Research Center)
  • SFI: Catalog of field spiral galaxies derived from the I-band Tully--Fisher relation
  • SFitter: An analysis tool to determine supersymmetric model parameters from collider measurements
  • SFT: String field theory
  • SGE: Sun Grid Engine
  • SGR: Soft gamma repeater
  • SGS: Subgrid Scale
  • SHALON: Extensive Air Showers from Neutrino (in Russian)
  • SHARE: Statistical HAdronization with REsonances code
  • SHERPA: Simulation of High-Energy Reactions of PArticles event generator
  • SHINE: SPS Heavy Ion and Neutrino Experiment
  • SHiP: Search for Hidden Particles experiment proposed at CERN
  • SHIP: Separator for Heavy Ion reaction Products at GSI
  • SHIPS: Solar Hidden Photon Search in Hamburg
  • SHM: Statistical hadronization model
  • SHOES: Supernova H0 for the Equation of State experiment on the Hubble Space Telescope
  • SHUMR: Shifted unitary minimal residual algorithm
  • SIAM: Single-impurity Anderson model
  • SIAM: Society for Industrial and Applied Mathematics
  • SIBYLL: Cosmic ray interaction event generator, apparently not an acronym
  • SiD: Silicon Detector for the ILC
  • SIDIS: Semi-inclusive deep inelastic scattering
  • SiFCC: Silicon Future Circular Collider detector
  • SIGHPC: ACM's Special Interest Group on High Performance Computing
  • SILAFAE: Simposio Latinoamericano de Física de Altas Energías
  • SILH: Strongly interacting light Higgs
  • SIMD: Single instruction, multiple data computers
  • SIMP: Strongly interacting massive particle
  • SIMPLE: Superheated Instrument for Massive ParticLe Experiments
  • SINFONI: Spectrograph for INtegral Field Observations in the Near Infrared
  • SIS: Schwer-Ionen Synchrotron (Heavy Ion Synchrotron) at GSI
  • SISCone: Seedless infrared-safe cone jet algorithm
  • SJ: String Junction
  • SK: Super-Kamiokande
  • SK: Schwinger and Keldysh
  • SKA: Square-Kilometer Array
  • SLAC: Stanford Linear Accelerator Center
  • SLag: Special Lagrangian
  • SLAM: Supersymmetry Les Houches Accord with Mathematica
  • SLD: SLAC Large Detector
  • SLHA: Supersymmetry Les Houches Accord
  • SLHM; Simplest little Higgs model
  • SLIC: Storage Lustre Interface Cluster
  • SLIM: Dark matter Scalar as LIght as MeV
  • SLIM: Search for LIght magnetic Monopoles
  • SLiNC: Stout Link Non-perturbative Clover fermion action
  • SLOCC: Stochastic local operations and classical communication
  • SLURM: Simple Linux Utility for Resource Management
  • SMASH: Simulating Many Accelerated Strongly-interacting Hadrons transport approach
  • SMASH: Standard model Axion Seesaw Higgs portal inflation
  • SMC: Sequential Monte Carlo (also known as particle filter methods)
  • SMC: Small Magellanic Cloud
  • SMD: Stochastic molecular dynamics
  • SME: Standard Model Extension framework
  • SMFNS: Symposium on Strong electroMagnetic Fields and Neutron Stars
  • SMG: Standard model group
  • SModelS: Simplified Model Spectrum topologies and package for analyzing them
  • SMOG: System for Measuring Overlap with Gas in LHCb
  • SMS: Simplified Model Spectrum topologies
  • sMSSM: Secluded-U(1)-extended MSSM
  • SNAP: Supernova/Acceleration Probe
  • SND: Spherical Neutral Detector at VEPP
  • SND@LHC: Scattering and Neutrino Detector at the LHC
  • SNEWS: Supernova Early Warning System
  • SNF: Supernova feedback to produce cored galaxy
  • SNLS: Supernovae Legacy Survey
  • SNM: Special nuclear material
  • SNO: Sudbury Neutrino Observatory
  • SNOwGLoBES: SuperNova Observatories with GLoBES
  • SNOP: Standard neutrino oscillation phenomenology
  • SNP DFS RAS: Section of Nuclear Physics, Physical Sciences Division of the Russian Academy of Sciences
  • SNR: Supernova remnant
  • SNS: Spallation Neutron Source at Oak Ridge
  • SNS: Something at the Rutherford Appleton Lab, now called ISIS, which is not an acronym
  • SNS: Superconductor--normal--superconductor Josephson junction
  • SNSI: Secret National Security Information
  • SNU: Solar neutrino unit
  • SOKENDAI: Graduate University for Advanced Studies (Sogo kenkyu daigakuin daigaku)
  • SOKOL: SOlnechnye KOLebaniya (Solar Oscillations) photometer, 1985--1986
  • SoLID: Solenoidal Large Intensity Device proposed for Jlab
  • SOPHIA: Simulations Of Photo-Hadronic Interactions in Astrophysics
  • SOPHIE: Spectrographe pour l'Observation des Phenomenes des Interieurs stellaires et des Exoplanetes in France
  • SOS: Solid-on-Solid
  • SOTR: Subcontracting Officer's Technical Representative
  • SOX: Short distance neutrino Oscillations with BoreXino
  • SPARC: Spitzer Photometry and Accurate Rotation Curves database
  • SPD: Spin Physics Detector at NICA at JINR
  • SPE: Synergistic Processor Element of Cell processor
  • SPEAR: Stanford Positron Electron Accelerating Ring
  • SEPCTRUM: Shaping Public hEalth poliCies to Reduce ineqUalities and harM consortium
  • sPHENIX: Proposed upgrade of PHENIX, apparently featuring a superconducting solenoid magnet
  • SPheno: Supersymmetric Phenomenology program for calculating spectrum and decays
  • SPheRIO: Smoothed Particle hydrodynamic evolution of Relativistic heavy IOn collisions
  • SPI: SPectrometer on INTEGRAL
  • SPICE: Simulation Package for Including flavor in Collider Events
  • SPIDER: Spectral Interferometry for Direct Electric Field Reconstruction
  • SPIE: Society of Photographic Instrumentation Engineers (no longer used)
  • SPIRAL: Système de Production dIons Radioactifs avec Accélération en Ligne
  • SPIRE: Spectral and Photometric Imaging Receiver on the Herschel Space Observatory
  • SPL: Superconducting Proton Linac at CERN
  • SppC: Super proton--proton Collider proposed in China
  • SPQCDR: Southampton, Paris and Rome QCD Collaboration
  • SPOR: Statistics, Probability and Operations Research
  • SPring-8: Super Photon ring at 8 GeV
  • SPS: Snowmass Points and Slopes
  • SPS: Super Proton Synchrotron at CERN
  • SPSS: Statistical Package for the Social Sciences
  • SPT: South Pole Telescope
  • SPT: Symmetry-protected trivial or symmetry-protected topological orders
  • SPTpol: A polarization-sensitive camera on SPT
  • sQGP: Strongly interacting quark--gluon plasma
  • SQM: Strange quark matter
  • SQUID: Superconducting quantum interference device
  • SONIC: Super hybrid mOdel simulationN for relativistic heavy-Ion Collisions
  • SRD: Secret Restricted Data
  • SRF: Superconducting radiofrequency
  • SRS: Synchrotron Radiation Source formerly at Daresbury
  • SSA: Single-spin asymmetry
  • SSA: Storage Systems Administration
  • SSC: Solid-state Slit Camera on MAXI
  • SSC: Superconducting Supercollider
  • SSC: Synchrotron self-Compton scattering
  • SSDL: Same sign dilepton channel
  • SSE: Streaming SIMD extensions
  • SSM: Sequential standard model
  • SSOR: Symmetric successive over-relaxation
  • SSP: Subaru Strategic Program for telescope on Mauna Kea
  • STAR: Solenoidal Tracker At RHIC
  • STARS: Caribbean Symposium on Cosmology, Gravitation, Nuclear and Astroparticle Physics, apparently not an acronym
  • STEM: Scanning transmission electron microscopy
  • STFC: UK Science and Technology Facilities Council
  • STM: Scanning tunneling microscopy
  • STU: Model that exhibits both exact S- and T-dualities
  • STXS: Simplified Template Cross Sections
  • sUED: Singlet-extended universal extra dimension
  • SuGAR: Searching for the sources of GAlactic cosmic Rays workshop
  • SUMR: Shifted Unitary Minimal Residual algorithm
  • SUNLAB: Underground laboratory in the Polkowice--Sieroszowice mine in Poland
  • SuperIso: Program for calculating flavor observables, focusing on isospin asymmetries in susy models
  • SURA: Southeastern Universities Research Association
  • SURF: Sanford Underground Research Facility in South Dakota
  • SuSA: SuperScaling Approach for neutrino--nucleus scattering
  • SusHi: Supersymmetric Higgs, program to calculate production cross sections
  • SVD: Spectrometer with Vertex Detector at IHEP
  • SVG: Scalable Vector Graphics
  • SVZ: Shifman, Vainshtein and Zakharov
  • SW: Sheikholeslami and Wohlert
  • SWME: Staggered fermion Weak Matrix Element Collaboration
  • SYK: Sachdev, Ye and Kitaev model
  • SYZ: Strominger, Yau and Zaslow conjecture that mirror symmetry is T-duality
  • SZ: Sunyaev and Zeldovich galaxy cluster effect

T

  • T2HK: Tokai to Hyper-Kamiokande
  • T2HKK: Tokai to Hyper-Kamiokande and Korea
  • T2K: Tokai to Kamioka
  • T2KK: Tokai to Kamioka and Korea
  • TA: Telescope Array air shower experiment in Utah
  • TALE: Telescope Array Low Energy extension
  • TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry
  • TAPAS: The Antiproton Annihilation Spectrometer at Fermilab
  • TAPS: Two-Arm Photon Spectrometer, has been used in the SPEAR detector at SLAC, the Crystal Ball detector at the Mainz Microtron, and perhaps teh Crystal Barrel Detektor at the Elektronen Stretcher Anlage in Bonn as well
  • TASCA: TransActinide Separator and Chemistry Apparatus at GSI
  • TASEP: Totally asymmetric simple exclusion process
  • TASK: Teilchen-, AStro- und Kernphysik in the Swiss Physical Society
  • TASSO: Two Arm Spectrometer Solenoid at DESY's PETRA
  • TAU: Tuning and Analysis Utilities performance analysis system
  • TAUOLA: Monte Carlo generator for tau lepton decays, apparently not an acronym
  • TAUP: Topics in Astroparticle and Underground Physics
  • TBA: Thermodynamic Bethe Ansatz
  • TBM: Tri-bimaximal mixing
  • TCC: Transplanckian Censorship Conjecture
  • TCE: TTA-based Co-design Environment
  • TCS: Timelike Compton scattering
  • TDA: Transition distribution amplitude
  • TDAQ: Trigger and Data Acquisition
  • TDGL: Time-dependent Ginzburg and Landau model
  • TE: Temperature and E-mode cross-correlation
  • TEA: Tung et al.
  • TEAM: Transmission Electron Aberration-Corrected Microscope
  • TEBD: Time-evolving block decimation tensor network method
  • TECHQM: Theory-Experiment Collaboration for Hot QCD Matter
  • TED: Technology and Engineering Development building at JLab
  • TED: Technology, Entertainment, Design conferences
  • TEK: Twisted Eguchi--Kawai model
  • TEM: Transmission electron microscopy
  • TERB: Tensor-entanglement renormalization group tensor network method
  • TES: Transition-edge sensor
  • TESLA: Teraelectronvolt Energy Superconducting Linear Accelerator
  • TESS: Transiting Exoplanet Survey Satellite launched by NASA in 2018
  • TeVeS: Modified Newtonian Dynamics with Tensor, Vector and Scalar fields
  • TEXONO: Taiwan Experiment on Neutrino
  • TF: Tully and Fisher
  • TFF: Transition form factor
  • TFH: Toorop, Feruglio and Hagedorn neutrino mixing patterns
  • TGAS: Tycho--Gaia Astrometric Solution combining the two data catalogs
  • THEIA: Proposed ESA satellite mission to study motion of faint astronomical objects in the Milky Way, apparently not an acronym
  • THEIA: Telescopic High-definition Earth Imaging Apparatus
  • THINGS: The HI Nearby Galaxy Survey
  • THOR: Theory of HOt matter and Relativistic heavy-ion collisions COST Action
  • TIAA: Teachers Insurance and Annuity Association
  • TikZ: LaTeX graphics package, apparently not an acronym
  • TILW: Tadpole improved Luescher-Weisz action
  • TJNAF: Thomas Jefferson National Accelerator Facility
  • TKNN: Thouless, Kohmoto, Nightingale and den Nijs number describing integer Hall conductivity
  • TL: Toda lattice
  • TLB: Translation lookaside buffer
  • TLEP: Triple Large Electron--Positron Collider
  • TM: Tri-maximal mixing
  • TMD: Tech company founded as Thorn Microwave Devices
  • TMD: Transverse momentum dependent parton distribution function
  • TMT: Thirty Meter Telescope proposed in Hawaii
  • TNE: Transnational education
  • TNS: Tensor network states
  • TOPAS: TOol for PArticle Simulation
  • TOPAZ: Detector at TRISTAN, acronym unknown, may be related to top quark
  • TOPIXS: TOP-pair Inclusive CROSS Section program
  • TOSS: Tri-lab Operating System Stack
  • TOTEM: TOTal cross section, Elastic scattering and diffraction dissociation Measurement at the LHC
  • TOV: Tolman, Oppenheimer and Volkoff
  • TPC: Time projection chamber
  • TPE: Two-photon exchange
  • TQFT: Thermal Quantum Field Theory and its Applications workshop series
  • TQFT: Topological quantum field theory
  • TREPS: Two-photonic REsonance Production Simulator
  • TRINAT: TRIUMF's Neutral Atom Trap
  • TRISTAN: Transposable Ring Intersecting Storage Accelerator in Nippon
  • TRIUMF: Originally TRI-University Meson Facility, now name of Canadian lab
  • TRV: Time-reversal violation
  • TS-PHMC: Two-Step Polynomial Hybrid Monte Carlo
  • TSSCPP: Totally symmetric self-complementary plane partition
  • TTA: Transport-Triggered Architecture
  • TTM: Top triangle moose
  • TUM: Technical University Munich
  • TUNL: Triangle Universities Nuclear Laboratory
  • TVID: Three-loop Vacuum Integrals from Dispersion relations Mathematica package
  • TWIST: TRIUMF Weak Interaction Symmetry Test
  • TXS: Texas Survey of astronomical radio sources
  • TYL: Toshiko Yuasa (1909--1980) Laboratory

U

  • UCAS: UK Universities and Colleges Admissions Service
  • UCN: Ultra-cold neutron
  • UCNA: Experiment to measure the Ultra-cold neutron "A-correlation" between the neutron's spin and its decay electron's momentum
  • UDM: Unified dark matter
  • UE: Underlying event
  • UED: Universal extra dimension
  • UERJ: Universidade do Estado do Rio de Janeiro
  • UFB: Unbounded from below
  • UFO: Universal FeynRules output file format
  • uGNI: User-level Generic Network Interface
  • UHECR: Ultra-high-energy cosmic ray
  • ULIRG: Ultraluminous infrared galaxy
  • UMSSM: U(1)-extended Minimal Supersymmetric Standard Model
  • uPDF: Unintegrated parton density function
  • URA: Universities Research Association
  • UrQMD: Ultra-relativistic quantum molecular dynamics
  • U-spin: SU(2) subgroup of flavor-SU(3) in which (d, s) are a doublet and u a singlet
  • USTFM: Unified Statistical Thermal Freeze-out Model of heavy-ion collisions
  • UT: Unitarity triangle
  • UTA: Unitarity triangle analysis
  • UTM: Upstream transverse momentum
  • UVES: Ultraviolet and Visual Echelle Spectrograph on the VLT

V

  • VAMPIR: Visualisation and Analysis of MPI Resources
  • VARC: Virginia Associated Research Campus at JLab
  • VBC: Valence bond crystal
  • VBF: Vector boson fusion
  • VBSCan: Vector Boson Scattering Coordination and Action Network
  • VECC: Variable Energy Cyclotron Centre in Kolkata
  • VEGAS: Algorithm to reduce errors in Monte Carlo calculations
  • VELO: VErtex LOcator LHCb sub-detector near the collision site
  • VENUS: VErsatile National Lab and Universities Spectrometer
  • VEPP: Electron-positron storage ring at the BINP
  • VERITAS: Very Energetic Radiation Imaging Telescope Array System
  • VES: VErtex Spectrometer at IHEP
  • VFNS: Variable Flavor Number Scheme
  • VGG: Vanderhaeghen, Guichon and Guidal
  • VHDL: VHSIC hardware description language
  • vHLLE: viscous hydrodynamics model based on the relativistic approximate Reimann solver of Harten, Lax, van Leer and Einfeldt
  • VHM: Very high multiplicity
  • VHSIC: Very-high-speed integrated circuits
  • VIKING: VISTA Kilo-Degree Infrared Galaxy Survey
  • VINCIA: Virtual Numerical Collider with Interleaved Antennae
  • VIRGO: Gravitational wave detector at EGO, apparently not an acronym
  • VISTA: Visible and Infrared Survey Telescope for Astronomy of ESO
  • VLA: Very Large Array of radio antennas run by the NRAO
  • VLBA: Very Long Baseline Array of radio telescopes run by the NRAO
  • VLBI: Very Long Baseline Interferometry consortium in Europe
  • VLENF: Very Low Energy Neutrino Factory, now nuSTORM
  • VLT: Very Large Telescope of ESO
  • VLTI: Very Large Telescope Interferometer of ESO
  • VLVnT: Very Large Volume Neutrino Telescopes workshop
  • VMD: Vector meson dominance
  • VME: VERSAmodule Eurocard bus
  • VNI: Parton cascade model code, acronym unknown
  • vNRQCD: Non-relativistic QCD matched to MSbar using a subtraction velocity rather than a subtraction scale
  • VSBL: Very short baseline
  • VSI: Vanishing Scalar Invariant
  • VSR: Very special relativity
  • VST: VLT Survey Telescope at ESO
  • VTR: Vault-Type Room at Livermore
  • VUV: Vacuum ultraviolet

W

  • WARP: Wimp Argon Programme
  • WASA: Wide Angle Shower Apparatus, once at CELSIUS, now at COSY
  • WATCHMAN: WATer CHerenkov Monitor for Anti-Neutrinos non-proliferation experiment at AIT
  • WB: Weak basis
  • wCDM: Cold dark matter model with free (constant) EOS w for dark energy
  • WCI: Weapons and Complex Integration at Livermore
  • WDM: Warm dark matter
  • WDRS: Workforce Development and Resources Section at Fermilab
  • WDVV: Witten, Dijkgraaf, Verlinde and Verlinde
  • WDWI: Weakly dissipative warm inflation
  • We: Electrical Watt
  • WEP: Weak equivalence principle
  • WF: Wilson and Fisher
  • WFCTA: Wide-Field-of-view Cherenkov Telescope Array in the LHAASO project
  • WFIRST: Wide Field Infrared Survey Telescope aimed to launch in 2020s
  • WGC: Weak Gravity Conjecture
  • WGMP: Workshop on Geometric Methods in Physics
  • WHDG: Wicks, Horowitz, Djordjevic and Gyulassy
  • WHIZARD: Monte Carlo event generator, apparently not an acronym
  • WIMT: Weitzenböck induced matter theory
  • WINHAC: Monte Carlo event generator for single W-boson production at hadron colliders
  • WISP: Weakly interacting sub-eV particle
  • WKB: Wentzel, Kramers and Brillouin
  • WKBJ: Wentzel, Kramers, Brillouin and Jeffreys
  • WMAP: Wilkinson Microwave Anisotropy Probe
  • WONP: Workshop On Nuclear Physics
  • WPCF: Workshop on Particle Correlations and Femtoscopy
  • WRAP: Waste & Resources Action Programme
  • Wth: Thermal Watt
  • WWND: Winter Workshop on Nuclear Dynamics
  • WZ: Wess and Zumino
  • WZNW: Wess, Zumino, Novikov, and Witten

X

  • XEFT: Low-energy effective theory for the X(3872)
  • XFEL: X-ray free electron laser
  • XFIRST: Wide Field Infrared Survey Telescope
  • XG: Xu and Greiner
  • XIS: X-ray Imaging Spectrometer
  • XMASS: All of (1) Xenon MASSive detector for solar neutrino, (2) Xenon detector for weakly interacting MASSive particles, (3) Xenon neutrino MASS detector
  • XMM-Newton: X-ray Multi-Mirror Mission of the ESA
  • XQC: X-ray Quantum Calorimetry rocket experiment reused for dark matter searches
  • XRISM: X-ray Imaging and Spectroscopy Mission
  • XRT: X-ray telescope
  • XSEDE: Extreme Science and Engineering Discovery Environment

Y

  • YaJEM: Yet another Jet Energy-loss Model
  • YBCO: Yttrium barium copper oxide
  • YETI: Young Experimentalists and Theorists Institute
  • YFS: Yennie, Frautschi and Suura
  • YMH: Yang, Mills and Higgs
  • Yp: Primordial helium abundance (mass fraction)
  • YSO: Young stellar object
  • YSS: Young Statisticians' Section of the RSS
  • YTF: Young Theorists' Forum at Durham
  • YUMGUT: Yukawon Ultra Minimal Grand Unified Theory

Z

  • ZAMO: Zero angular momentum observer
  • ZDC: Zero degree calorimeter
  • ZEPLIN: Liquid Xenon and proportional scintillation dark matter experiment
  • ZiF: Zentrum für interdisziplinäre Forschung at Bielefeld
  • ZTF: Zwicky Transient Facility at Palomar

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