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A Resource Theory for Work and Heat

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arxiv 1607.01302 v3 pith:ULNUPX4U submitted 2016-07-05 quant-ph cond-mat.stat-mechcs.ITmath.IT

classification quant-phcond-mat.stat-mechcs.ITmath.IT
keywords resourcetheorythermodynamicsstatesheatquantumtheoriesbackground
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Several recent results on thermodynamics have been obtained using the tools of quantum information theory and resource theories. So far, the resource theories utilised to describe thermodynamics have assumed the existence of an infinite thermal reservoir, by declaring that thermal states at some background temperature come for free. Here, we propose a resource theory of quantum thermodynamics without a background temperature, so that no states at all come for free. We apply this resource theory to the case of many non-interacting systems, and show that all quantum states are classified by their entropy and average energy, even arbitrarily far away from equilibrium. This implies that thermodynamics takes place in a two-dimensional convex set that we call the energy-entropy diagram. The answers to many resource-theoretic questions about thermodynamics can be read off from this diagram, such as the efficiency of a heat engine consisting of finite reservoirs, or the rate of conversion between two states. This allows us to consider a resource theory which puts work and heat on an equal footing, and serves as a model for other resource theories.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Maximum channel entropy principle and microcanonical channels

    quant-ph 2025-08 unverdicted novelty 7.0 of 10

    A maximum-entropy principle for quantum channels yields thermal channels with exponential form, analogous to thermal states.

  2. Random Quantum Batteries

    quant-ph 2019-08 conditional novelty 6.0 of 10

    Random quantum batteries have typical work extraction equal to the energy gap to the completely mixed state times a spectrum-dependent quantum efficiency factor, with fluctuations vanishing in large Hilbert spaces.

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