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A possible semiclassical bounce instead of a Schwarzschild singularity

dc.contributor.authorBolokhov, S. V.
dc.contributor.authorSkvortsova, M. V.
dc.contributor.authorBronnikov, K. A.
dc.contributor.authorБронников, Кирилл Александрович
dc.date.accessioned2024-11-25T16:18:51Z
dc.date.available2024-11-25T16:18:51Z
dc.date.issued2020
dc.description.abstract© 2020 World Scientific Publishing Company.We have previously shown that the singularity in a Schwarzschild black hole of stellar or larger mass may be avoided in a semiclassical manner by using as a source of gravity the stress-energy tensor (SET) corresponding to vacuum polarization of quantum fields, with a minimum spherical radius a few orders of magnitude larger than the Planck length. In this note we estimate the nonlocal contribution to the total SET due to particle creation from vacuum. We show that this contribution is negligibly small as compared to vacuum polarization and does not affect the previously suggested scenario.
dc.identifier.citationBolokhov, S. V. A possible semiclassical bounce instead of a Schwarzschild singularity / Bolokhov, S.V., Skvortsova, M.V., Bronnikov, K.A. // International Journal of Modern Physics A. - 2020. - 10.1142/S0217751X20400515
dc.identifier.doi10.1142/S0217751X20400515
dc.identifier.urihttps://www.doi.org/10.1142/S0217751X20400515
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dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/20288
dc.relation.ispartofInternational Journal of Modern Physics A
dc.titleA possible semiclassical bounce instead of a Schwarzschild singularity
dc.typeArticle
dspace.entity.typePublication
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