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Self gravitating spinning string condensates
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DOI：10.1007/JHEP07(2024)217.png)
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Abstract
En 中文
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.
Keywords:
Black Holes in String Theory
Effective Field Theories
Long Strings
Tachyon Condensation
Journal
IF:
5.5
Papers:
3.9W
Citations:
13.7W