Exact solutions for supersymmetric stationary black hole composites

From MaRDI portal
Publication:2261078

DOI10.1007/JHEP11(2011)127zbMATH Open1306.83040arXivhep-th/0304094OpenAlexW2152395291MaRDI QIDQ2261078

Author name not available (Why is that?)

Publication date: 6 March 2015

Published in: (Search for Journal in Brave)

Abstract: Four dimensional N=2 supergravity has regular, stationary, asymptotically flat BPS solutions with intrinsic angular momentum, describing bound states of separate extremal black holes with mutually nonlocal charges. Though the existence and some properties of these solutions were established some time ago, fully explicit analytic solutions were lacking thus far. In this note, we fill this gap. We show in general that explicit solutions can be constructed whenever an explicit formula is known in the theory at hand for the Bekenstein-Hawking entropy of a single black hole as a function of its charges, and illustrate this with some simple examples. We also give an example of moduli-dependent black hole entropy.


Full work available at URL: https://arxiv.org/abs/hep-th/0304094



No records found.


No records found.








This page was built for publication: Exact solutions for supersymmetric stationary black hole composites

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q2261078)