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Classical-Quantum Correspondence and Hawking Radiation

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arxiv 1803.08919 v3 pith:FVP53LAY submitted 2018-03-23 hep-th gr-qc

Tanmay Vachaspati , George Zahariade This is my paper
classification hep-thgr-qc
keywords radiationclassical-quantumcorrespondencehawkingproblemsquantumbackgroundbackreaction
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A recently discovered classical-quantum correspondence (CQC) maps certain quantum problems to corresponding classical problems. We illustrate the CQC for a quantum scalar field in the gravitational background of a collapsing spherical shell. By truncating the problem to a small set of variables, we show how the CQC can yield Hawking radiation as well as the slow down of the collapse due to radiation backreaction.

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Cited by 1 Pith paper

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

  1. Quantum fields in boson star spacetime

    gr-qc 2026-01 conditional novelty 6.0 of 10

    In boson star spacetimes, the renormalized quantum stress tensor has mostly positive energy density and negative radial pressure that grow with curvature, rivaling the classical stress in the most compact solutions.

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