paper

Black holes and black strings in the Einstein -non-linear sigma model

arXiv:2208.14239

Abstract

We construct analytical solutions describing black holes and black strings in the Einstein -non-linear sigma model in dimensions. This construction is carried out using the maximal embbeding ansatz of together with the Euler parameterization of the group, in such a way that the non-linear sigma model equations are automatically satisfied for arbitrary values of the flavor number while the Einstein equations can be solved analytically. In particular, we construct black holes with spherical and flat horizons as well as black strings that present the geometry of a three-dimensional charged Bañados-Teitelboim-Zanelli black hole on the transverse section of the string. These configurations are not trivial embeddings of into , which allow us to explicitly show the role that the flavor number plays on the geometry and thermodynamics of the black holes and black strings. Finally, we perform a thermal comparison between these configurations.

18 pages, 5 figures, accepted for publication in Phys. Rev. D