Comments (5)
Thanks for the advice, I'll add it to the to-do list.
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It is probably worth noting that the degrees of freedom are only 3*N, where N is number of particles, for the Andersen thermostat. DF are different for stochastic or deterministic thermostats, and this rippled to kinetic energy. The difference is small, but nonetheless, worth accounting for.
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Thanks, let me know as you see anything else, it's useful.
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I think @BradenDKelly suggestion would enhance the performance and simplicity of the api. The suggested table can also have a r_cutoff field for each pair of particle types. Then something like negative values can be set to it to exclude that pair of particle types from force calculation (or neighbor searching). That's the method that HOOMD-Blue uses.
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I think it's a good idea but will wait to see how the GPU kernel work (#60) progresses as this may require a refactor of other parts of the API too.
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Related Issues (20)
- Links in Docs are broken HOT 2
- Boltzmann Constant in LAMMPS 'real' units does not work HOT 5
- AtomsBase not properly implemented HOT 4
- GPU error with custom pairwise interactions HOT 5
- Inconsistent Units Crash Simulation HOT 5
- apply_coupling! method is not found for custom coupling function HOT 2
- Example for new MC membrane barostat HOT 12
- How to cite? HOT 6
- [feature request] velocity-dependent forces HOT 2
- Should we pass more properties (e.g. velocities, step number) to `force`/`potential_energy`? HOT 4
- Should we have functions to add and remove atoms to/from a `System`? HOT 3
- open an sdf file HOT 10
- Molly.jl: AD with Enyzme returns 0 gradient HOT 1
- Units in Nose Hoover temperature HOT 1
- GPU error with the example HOT 4
- return type for force for pairwise potential in CUDA HOT 1
- sys.coords does not work as Vector{Vector} HOT 2
- EAM implementation and dimension error HOT 5
- Boundary Conditions HOT 1
- UndefVarError: `σ6` not defined ERROR when simulating the NPT ensemble HOT 1
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