Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

Kuan-Nan Lin; Evgenii Ievlev; Michael R. R. Good; Pisin Chen

Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

Kuan-Nan Lin, Evgenii Ievlev, Michael R. R. Good, Pisin Chen

School of Sciences and Humanities

Research output: Working paper › Preprint

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Abstract

We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find high-speed electrons, while having a high temperature, correspond to low-temperature analog remnants.

Original language	English
Publication status	Published - Feb 25 2024

Keywords

gr-qc
quant-ph

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2402.16137v1

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title = "Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation",

abstract = "We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find high-speed electrons, while having a high temperature, correspond to low-temperature analog remnants.",

keywords = "gr-qc, quant-ph",

author = "Kuan-Nan Lin and Evgenii Ievlev and Good, {Michael R. R.} and Pisin Chen",

note = "14 pages, 12 figures",

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T1 - Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

AU - Lin, Kuan-Nan

AU - Ievlev, Evgenii

AU - Good, Michael R. R.

AU - Chen, Pisin

N1 - 14 pages, 12 figures

PY - 2024/2/25

Y1 - 2024/2/25

N2 - We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find high-speed electrons, while having a high temperature, correspond to low-temperature analog remnants.

AB - We investigate the radiation from accelerating electrons with asymptotic constant velocity and their analog signatures as evaporating black holes with left-over remnants. We find high-speed electrons, while having a high temperature, correspond to low-temperature analog remnants.

KW - gr-qc

KW - quant-ph

M3 - Preprint

BT - Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

ER -

Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation

Abstract

Keywords

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