{"title":"First part of Clausius heat theorem in terms of Noether's theorem","authors":"Aaron Beyen, Christian Maes","doi":"arxiv-2408.15773","DOIUrl":null,"url":null,"abstract":"After Helmholtz, the mechanical foundation of thermodynamics included the\nFirst Law $d E = \\delta Q + \\delta W$, and the first part of the Clausius heat\ntheorem $\\delta Q^\\text{rev}/T = dS$. The resulting invariance of the entropy\n$S$ for quasistatic changes in thermally isolated systems invites a connection\nwith Noether's theorem (only established later). In this quest, we continue an\nidea, first brought up by Wald in black hole thermodynamics and by Sasa\n$\\textit{et al.}$ in various contexts. We follow both Lagrangian and\nHamiltonian frameworks, and emphasize the role of Killing equations for\nderiving a First Law for thermodynamically consistent trajectories, to end up\nwith an expression of ``heat over temperature'' as an exact differential of a\nNoether charge.","PeriodicalId":501482,"journal":{"name":"arXiv - PHYS - Classical Physics","volume":"58 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Classical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.15773","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
After Helmholtz, the mechanical foundation of thermodynamics included the
First Law $d E = \delta Q + \delta W$, and the first part of the Clausius heat
theorem $\delta Q^\text{rev}/T = dS$. The resulting invariance of the entropy
$S$ for quasistatic changes in thermally isolated systems invites a connection
with Noether's theorem (only established later). In this quest, we continue an
idea, first brought up by Wald in black hole thermodynamics and by Sasa
$\textit{et al.}$ in various contexts. We follow both Lagrangian and
Hamiltonian frameworks, and emphasize the role of Killing equations for
deriving a First Law for thermodynamically consistent trajectories, to end up
with an expression of ``heat over temperature'' as an exact differential of a
Noether charge.