From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity

Abstract We obtain cosmological solutions with Kasner-like asymptotics in N $$ \mathcal{N} $$ = 2 gauged and ungauged supergravity by maximal analytic continuation of planar versions of non-extremal black hole solutions. Initially, we construct static solutions with planar symmetry by solving the ti...

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Main Authors: J. Gutowski, T. Mohaupt, G. Pope
Format: Article
Language:English
Published: SpringerOpen 2019-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP08(2019)172
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spelling doaj-276bac66c0054220aa6a6f674c88474d2020-11-25T03:49:36ZengSpringerOpenJournal of High Energy Physics1029-84792019-08-012019816610.1007/JHEP08(2019)172From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravityJ. Gutowski0T. Mohaupt1G. Pope2Department of Mathematics, University of SurreyDepartment of Mathematical Sciences, University of LiverpoolDepartment of Mathematical Sciences, University of LiverpoolAbstract We obtain cosmological solutions with Kasner-like asymptotics in N $$ \mathcal{N} $$ = 2 gauged and ungauged supergravity by maximal analytic continuation of planar versions of non-extremal black hole solutions. Initially, we construct static solutions with planar symmetry by solving the time-reduced field equations. Upon lifting back to four dimensions, the resulting static regions are incomplete and bounded by a curvature singularity on one side and a Killing horizon on the other. Analytic continuation reveals the existence of dynamic patches in the past and future, with Kasner-like asymptotics. For the ungauged STU-model, our solutions contain previously known solutions with the same conformal diagram as a subset. We find explicit lifts to five, six, ten and eleven dimensions which show that in the extremal limit, the underlying brane configuration is the same as for STU black holes. The extremal limit of the six-dimensional lift is shown to be BPS for special choices of the integration constants. We argue that there is a universal correspondence between spherically symmetric black hole solutions and planar cosmological solutions which can be illustrated using the Reissner-Nordström solution of Einstein-Maxwell theory.http://link.springer.com/article/10.1007/JHEP08(2019)172Black Holes in String TheorySupergravity Modelsp-branesM-Theory
collection DOAJ
language English
format Article
sources DOAJ
author J. Gutowski
T. Mohaupt
G. Pope
spellingShingle J. Gutowski
T. Mohaupt
G. Pope
From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
Journal of High Energy Physics
Black Holes in String Theory
Supergravity Models
p-branes
M-Theory
author_facet J. Gutowski
T. Mohaupt
G. Pope
author_sort J. Gutowski
title From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
title_short From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
title_full From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
title_fullStr From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
title_full_unstemmed From static to cosmological solutions of N $$ \mathcal{N} $$ = 2 supergravity
title_sort from static to cosmological solutions of n $$ \mathcal{n} $$ = 2 supergravity
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-08-01
description Abstract We obtain cosmological solutions with Kasner-like asymptotics in N $$ \mathcal{N} $$ = 2 gauged and ungauged supergravity by maximal analytic continuation of planar versions of non-extremal black hole solutions. Initially, we construct static solutions with planar symmetry by solving the time-reduced field equations. Upon lifting back to four dimensions, the resulting static regions are incomplete and bounded by a curvature singularity on one side and a Killing horizon on the other. Analytic continuation reveals the existence of dynamic patches in the past and future, with Kasner-like asymptotics. For the ungauged STU-model, our solutions contain previously known solutions with the same conformal diagram as a subset. We find explicit lifts to five, six, ten and eleven dimensions which show that in the extremal limit, the underlying brane configuration is the same as for STU black holes. The extremal limit of the six-dimensional lift is shown to be BPS for special choices of the integration constants. We argue that there is a universal correspondence between spherically symmetric black hole solutions and planar cosmological solutions which can be illustrated using the Reissner-Nordström solution of Einstein-Maxwell theory.
topic Black Holes in String Theory
Supergravity Models
p-branes
M-Theory
url http://link.springer.com/article/10.1007/JHEP08(2019)172
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