TY - JOUR
T1 - Quantum power
T2 - a Lorentz invariant approach to Hawking radiation
AU - Good, Michael R.R.
AU - Linder, Eric V.
N1 - Publisher Copyright:
© 2022, The Author(s).
PY - 2022/3
Y1 - 2022/3
N2 - 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.
AB - 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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U2 - 10.1140/epjc/s10052-022-10167-6
DO - 10.1140/epjc/s10052-022-10167-6
M3 - Article
AN - SCOPUS:85126238226
SN - 1434-6044
VL - 82
JO - European Physical Journal C
JF - European Physical Journal C
IS - 3
M1 - 204
ER -