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Bibliographic Details
Main Authors: Santos, Jorge E., Zigdon, Yoav
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2403.20332
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author Santos, Jorge E.
Zigdon, Yoav
author_facet Santos, Jorge E.
Zigdon, Yoav
contents In the context of the black hole/string transition, it is useful to produce Euclidean string backgrounds representing hot and self-gravitating strings. We utilise analytical and numerical methods to find a smooth, stationary rotating solution in the heterotic string theory at high temperatures. The solution describes a spinning winding-momentum condensate living in three non-compact dimensions, and its backreaction on the thermal cycle. At low temperatures, we expect a transition between our solution to an analytical continuation of an axionic Kerr black hole.
format Preprint
id arxiv_https___arxiv_org_abs_2403_20332
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Self Gravitating Spinning String Condensates
Santos, Jorge E.
Zigdon, Yoav
High Energy Physics - Theory
In the context of the black hole/string transition, it is useful to produce Euclidean string backgrounds representing hot and self-gravitating strings. We utilise analytical and numerical methods to find a smooth, stationary rotating solution in the heterotic string theory at high temperatures. The solution describes a spinning winding-momentum condensate living in three non-compact dimensions, and its backreaction on the thermal cycle. At low temperatures, we expect a transition between our solution to an analytical continuation of an axionic Kerr black hole.
title Self Gravitating Spinning String Condensates
topic High Energy Physics - Theory
url https://arxiv.org/abs/2403.20332