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Promoting Fluctuation Theorems into Covariant Forms

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arxiv 2312.17621 v4 pith:GZUF7ZKC submitted 2023-12-29 cond-mat.stat-mech

classification cond-mat.stat-mech
keywords fluctuationheattheoremscovariancecovariantmovingprinciplethermodynamic
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The principle of covariance, a cornerstone of modern physics, asserts the equivalence of all inertial frames of reference. Fluctuation theorems, as extensions of the second law of thermodynamics, establish universal connections between irreversibility and fluctuation in terms of stochastic thermodynamic quantities. However, these relations typically assume that both the thermodynamic system and the heat bath are at rest with respect to the observer, thereby failing to satisfy the principle of covariance. In this study, by introducing covariant work and heat that incorporate both energy-related and momentum-related components, we promote fluctuation theorems into covariant forms applicable to moving thermodynamic systems and moving heat baths. We illustrate this framework with two examples: the work statistics of a relativistic stochastic field and the heat statistics of a relativistic Brownian motion. Although our study is carried out in the context of special relativity, the results can be extended to the nonrelativistic limit. Our work combines the principle of covariance and fluctuation theorems into a coherent framework and may have applications in the study of thermodynamics relevant to cosmic microwave background as well as the radiative heat transfer and noncontact friction between relatively moving bodies.

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Cited by 2 Pith papers

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  1. Gaussian generally covariant hydrodynamics

    hep-th 2025-04 conditional novelty 6.0 of 10

    A Gaussian stochastic partition function constrained by gravitational Ward identities yields a proposed generally covariant fluctuating hydrodynamics in which flow is an approximate Killing vector.

  2. Lorentz Transformation of the Energy Spectrum of the Equilibrium State of Massive Free Fields

    cond-mat.stat-mech 2024-12 accept novelty 6.0 of 10

    Massive free-field spectra in moving frames cannot be represented by a scalar temperature with dipole anisotropy, forcing the use of a four-vector temperature.

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