A smooth road to bumpy horizons: shaping black holes with non-linear sigma models, from supergravity to higher dimensions

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Canfora, Fabrizio, Grandi, Nicolás, Henríquez-Báez, Carla, Oliva, Julio
Format: Preprint
Veröffentlicht: 2026
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866915835372634112
author Canfora, Fabrizio
Grandi, Nicolás
Henríquez-Báez, Carla
Oliva, Julio
author_facet Canfora, Fabrizio
Grandi, Nicolás
Henríquez-Báez, Carla
Oliva, Julio
contents We construct new families of solutions for General Relativity coupled to a general class of non-linear sigma models, some of which can be embedded in supergravity. The solutions include neutral, charged and magnetized black holes with bumpy horizons, bumpy stars, and anisotropic cosmologies in $d\geq 4$ dimensions, as well as black strings and black $p$-branes. We also present a family of time-dependent solutions in $2+1$-dimensions. The construction relies on a set of first-order Bogomol'nyi-Prasad-Sommerfield relations for the coset scalars, that were recently exploited for the construction of bumpy black holes on the non-linear sigma model with homogenous target $SU(2)/U(1)$ in 2601.22914 [hep-th].
format Preprint
id arxiv_https___arxiv_org_abs_2603_04611
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle A smooth road to bumpy horizons: shaping black holes with non-linear sigma models, from supergravity to higher dimensions
Canfora, Fabrizio
Grandi, Nicolás
Henríquez-Báez, Carla
Oliva, Julio
High Energy Physics - Theory
We construct new families of solutions for General Relativity coupled to a general class of non-linear sigma models, some of which can be embedded in supergravity. The solutions include neutral, charged and magnetized black holes with bumpy horizons, bumpy stars, and anisotropic cosmologies in $d\geq 4$ dimensions, as well as black strings and black $p$-branes. We also present a family of time-dependent solutions in $2+1$-dimensions. The construction relies on a set of first-order Bogomol'nyi-Prasad-Sommerfield relations for the coset scalars, that were recently exploited for the construction of bumpy black holes on the non-linear sigma model with homogenous target $SU(2)/U(1)$ in 2601.22914 [hep-th].
title A smooth road to bumpy horizons: shaping black holes with non-linear sigma models, from supergravity to higher dimensions
topic High Energy Physics - Theory
url https://arxiv.org/abs/2603.04611