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ESPResSo can solve rotation motion too. By default, particles are non-rotating. Rotation must be specified at particle creation (section Rotational degrees of freedom and particle anisotropy). Thermostats have a flag |
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Thans a lot for this explanation. It is really help.
Best wishes,
Wenming Yang
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At 2025-09-12 09:37:12, "Jean-Noël Grad" ***@***.***> wrote:
ESPResSo can solve rotation motion too. By default, particles are non-rotating. Rotation must be specified at particle creation (section Rotational degrees of freedom and particle anisotropy). Thermostats have a flag gamma_rotation. Anisotropy can be achieved by setting the particle rotational inertial tensor. The particle director, quaternion, and magnetic dipole are internally all linked together: modifying one modifies the other. Hope this helps! Sorry for the late answer.
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I have noticed that in tutorials and introductions related to Langevin dynamics, only the translational motion equations of particles are typically presented. Does ESPResSo have the capability to also solve for the rotational dynamics of particles?
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