On the Universality of the Entropy-Area Relation
Seth A. Major, Kevin L. Setter

TL;DR
This paper argues that for many gravity models, canonical quantization naturally leads to the Bekenstein-Hawking entropy-area relation under certain conditions, linking thermodynamics and quantum gravity.
Contribution
It demonstrates that a broad class of gravity dynamics inherently satisfy the entropy-area relation through canonical quantization, connecting thermodynamic and geometric entropy calculations.
Findings
Entropy-area relation holds for low temperatures and large boundary areas.
Relates grand canonical ensemble approach to geometric entropy calculations.
Supports universality of the entropy-area relation in quantum gravity.
Abstract
We present an argument that, for a large class of possible dynamics, a canonical quantization of gravity will satisfy the Bekenstein-Hawking entropy-area relation. This result holds for temperatures low compared to the Planck temperature and for boundaries with areas large compared to Planck area. We also relate our description, in terms of a grand canonical ensemble, to previous geometric entropy calculations using area ensembles.
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