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Self Gravitating Spinning String Condensates
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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.
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Cited by 2 Pith papers
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Scalar Hair at the String-Black-Hole Correspondence
All static spherical axion-dilaton solutions are SL(2,R) images of the FJNW seed, and scalar hair increases the alpha-prime curvature diagnostic at the string-black-hole correspondence surface, selecting the hairless ...
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Self-gravitating strings and quantum effects in two-dimensional gravity
An exact analytic Horowitz-Polchinski winding-string solution is derived for two-dimensional dilaton gravity and for the quantum-corrected RST model, with a classification of singular, regular, and horizon branches.
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