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.
What this package declares
The file a client reads when it loads this plugin, exactly as this revision carries it.
plugin.json
{
"$schema": "https://agent-plugins.org/schemas/1.0.0/plugin.schema.json",
"name": "statistical-physicist",
"version": "1.0.0",
"description": "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.",
"author": {
"name": "K-Dense",
"url": "https://www.k-dense.ai"
},
"homepage": "https://github.com/K-Dense-AI/scientific-agents",
"repository": "https://github.com/K-Dense-AI/scientific-agents",
"license": "MIT",
"keywords": [
"science",
"agents-md",
"expert-profile",
"statistical-physicist"
]
}