Non-equilibrium thermodynamics of gravitational objective-collapse models

Fuente: arXiv
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Autori principali: Artini, Simone, Monaco, Gabriele Lo, Donadi, Sandro, Paternostro, Mauro
Natura: Preprint
Pubblicazione: 2025
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author Artini, Simone
Monaco, Gabriele Lo
Donadi, Sandro
Paternostro, Mauro
author_facet Artini, Simone
Monaco, Gabriele Lo
Donadi, Sandro
Paternostro, Mauro
contents We investigate the entropy production in the Diósi-Penrose (DP) model, one of the most extensively studied gravity-related collapse mechanisms, and one of its dissipative extensions. To this end, we analyze the behavior of a single harmonic oscillator, subjected to such collapse mechanisms, focusing on its phase-space dynamics and the time evolution of the entropy production rate, a central quantity in non-equilibrium thermodynamics. Our findings reveal that the original DP model induces unbounded heating, producing dynamics consistent with the Second Law of thermodynamics only under the assumption of an infinite-temperature noise field. In contrast, its dissipative extension achieves physically consistent thermalization in the regime of low dissipation strength. We further our study to address the complete dynamics of the dissipative extension, thus including explicitly non-Gaussian features in the state of the system that lack from the low-dissipation regime, using a short-time approach.
format Preprint
id arxiv_https___arxiv_org_abs_2502_03173
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Non-equilibrium thermodynamics of gravitational objective-collapse models
Artini, Simone
Monaco, Gabriele Lo
Donadi, Sandro
Paternostro, Mauro
Quantum Physics
We investigate the entropy production in the Diósi-Penrose (DP) model, one of the most extensively studied gravity-related collapse mechanisms, and one of its dissipative extensions. To this end, we analyze the behavior of a single harmonic oscillator, subjected to such collapse mechanisms, focusing on its phase-space dynamics and the time evolution of the entropy production rate, a central quantity in non-equilibrium thermodynamics. Our findings reveal that the original DP model induces unbounded heating, producing dynamics consistent with the Second Law of thermodynamics only under the assumption of an infinite-temperature noise field. In contrast, its dissipative extension achieves physically consistent thermalization in the regime of low dissipation strength. We further our study to address the complete dynamics of the dissipative extension, thus including explicitly non-Gaussian features in the state of the system that lack from the low-dissipation regime, using a short-time approach.
title Non-equilibrium thermodynamics of gravitational objective-collapse models
topic Quantum Physics
url https://arxiv.org/abs/2502.03173