Quantum power: a Lorentz invariant approach to Hawking radiation
Good M.R.R. Linder E.V.
March 2022Springer Science and Business Media Deutschland GmbH
European Physical Journal C
2022#82Issue 3
Particle radiation from black holes has an observed emission power depending on the surface gravity κ= c4/ (4 GM) as Pblack hole∼ħκ26πc2=ħc696πG2M2,while both the radiation from accelerating particles and moving mirrors (accelerating boundaries) obey similar relativistic Larmor powers, Pelectron=q2α26πϵ0c3,Pmirror=ħα26πc2,where α is the Lorentz invariant proper acceleration. This equivalence between the Lorentz invariant powers suggests a close relation that could be used to understand black hole radiation. We show that an accelerating mirror with a prolonged metastable acceleration plateau can provide a unitary, thermal, energy-conserved analog model for black hole decay.
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Physics Department, Nazarbayev University, Nur-Sultan, Kazakhstan
Energetic Cosmos Lab, Nazarbayev University, Nur-Sultan, Kazakhstan
Berkeley Center for Cosmological Physics and Berkeley Lab, University of California, Berkeley, CA, United States
Physics Department
Energetic Cosmos Lab
Berkeley Center for Cosmological Physics and Berkeley Lab
10 лет помогаем публиковать статьи Международный издатель
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