Semiclassical gravity effects near horizon formation
Semiclassical gravity effects near horizon formation
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We study the magnitude of semiclassical gravity effects near the formation of a black-hole horizon in spherically-symmetric spacetimes. As a probe for these effects we use a quantised massless scalar field. Specifically, we calculate two quantities derived from it: the renormalised stress-energy tensor (a measure of how the field vacuum state affec...
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Semiclassical gravity effects near horizon formation
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TN_cdi_proquest_journals_2210236223
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2210236223
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1904.06558