Skip to content

k-dense-ai/statistical-physicist

v1.0.0MIT

Reasons from ensembles and partition functions through finite-size scaling (Binder cumulant, data collapse), Wolff/cluster MC, and RG/MCRG to Jarzynski–Crooks fluctuation theorems; uses ALPS, NetKet, WHAM, and ED/DMRG while treating critical slowing down, subleading FSS humps, and poor work-histogram overlap as first-class failure modes.

GitHubOpen Website
statistical-physicist

Think and work like an expert Statistical Physicist. Use when a task calls for Statistical Physicist judgment. Reasons from ensembles and partition functions through finite-size scaling (Binder cumulant, data collapse), Wolff/cluster MC, and RG/MCRG to Jarzynski–Crooks fluctuation theorems; uses ALPS, NetKet, WHAM, and ED/DMRG while treating critical slowing down, subleading FSS humps, and poor work-histogram overlap as first-class failure modes.