English

STATIC FOUR-DIMENSIONAL ABELIAN BLACK HOLES IN KALUZA-KLEIN THEORY

High Energy Physics - Theory 2016-09-06 v1 General Relativity and Quantum Cosmology

Abstract

Static, four-dimensional (4-d) black holes (BH's) in (4+n4+n)-d Kaluza-Klein (KK) theory with Abelian isometry and diagonal internal metric have at most one electric (QQ) and one magnetic (PP) charges, which can either come from the same U(1)U(1)-gauge field (corresponding to BH's in effective 5-d KK theory) or from different ones (corresponding to BH's with U(1)M×U(1)EU(1)_M\times U(1)_E isometry of an effective 6-d KK theory). In the latter case, explicit non-extreme solutions have the global space-time of Schwarzschild BH's, finite temperature, and non-zero entropy. In the extreme (supersymmetric) limit the singularity becomes null, the temperature saturates the upper bound TH=1/4πQPT_H=1/4\pi\sqrt{|QP|}, and entropy is zero. A class of KK BH's with constrained charge configurations, exhibiting a continuous electric-magnetic duality, are generated by global SO(n)SO(n) transformations on the above classes of the solutions.

Keywords

Cite

@article{arxiv.hep-th/9502099,
  title  = {STATIC FOUR-DIMENSIONAL ABELIAN BLACK HOLES IN KALUZA-KLEIN THEORY},
  author = {Mirjam Cvetic and Donam Youm},
  journal= {arXiv preprint arXiv:hep-th/9502099},
  year   = {2016}
}

Comments

11 pages, 2 Postscript figures. uses RevTeX and psfig.sty (for figs) paper and figs also at ftp://dept.physics.upenn.edu/pub/Cvetic/UPR-645-T