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

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dc.contributor.authorLin Kuan-Nan
dc.contributor.authorIevlev Evgenii
dc.contributor.authorGood Michael R. R.
dc.contributor.authorChen Pisin
dc.date.accessioned2025-08-26T10:08:19Z
dc.date.available2025-08-26T10:08:19Z
dc.date.issued2024-06-25
dc.description.abstractWe 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.en
dc.identifier.citationLin Kuan-Nan; Ievlev Evgenii; Good Michael R. R.; Chen Pisin. (2024). Classical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiation. The European Physical Journal C. https://doi.org/10.1140/epjc/s10052-024-12991-4en
dc.identifier.doi10.1140/epjc/s10052-024-12991-4
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-024-12991-4
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/10170
dc.language.isoen
dc.publisherSpringer Science and Business Media LLC
dc.rightsAll rights reserveden
dc.source(2024)en
dc.titleClassical acceleration temperature from evaporated black hole remnants and accelerated electron-mirror radiationen
dc.typearticleen

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