Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces
We show that the horizon geometry for supersymmetric black hole solutions of minimal five-dimensional gauged supergravity is that of a particular Einstein-Cartan-Weyl (ECW) structure in three dimensions, involving the trace and traceless part of both torsion and nonmetricity, and obeying some precis...
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2019-06-01
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doaj-5e954b440f3746aa892db407025041ae2020-11-25T02:03:36ZengElsevierPhysics Letters B0370-26932019-06-01793265270Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spacesDietmar Silke Klemm0Lucrezia Ravera1Dipartimento di Fisica, Università di Milano, Via Celoria 16, 20133 Milano, Italy; INFN, Sezione di Milano, Via Celoria 16, I-20133 Milano, ItalyINFN, Sezione di Milano, Via Celoria 16, I-20133 Milano, Italy; Corresponding author.We show that the horizon geometry for supersymmetric black hole solutions of minimal five-dimensional gauged supergravity is that of a particular Einstein-Cartan-Weyl (ECW) structure in three dimensions, involving the trace and traceless part of both torsion and nonmetricity, and obeying some precise constraints. In the limit of zero cosmological constant, the set of nonlinear partial differential equations characterizing this ECW structure reduces correctly to that of a hyper-CR Einstein-Weyl structure in the Gauduchon gauge, which was shown by Dunajski, Gutowski and Sabra to be the horizon geometry in the ungauged BPS case. Keywords: Supersymmetry, Supergravity, Near horizon geometry, Metric affine gravityhttp://www.sciencedirect.com/science/article/pii/S0370269319302953 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Dietmar Silke Klemm Lucrezia Ravera |
spellingShingle |
Dietmar Silke Klemm Lucrezia Ravera Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces Physics Letters B |
author_facet |
Dietmar Silke Klemm Lucrezia Ravera |
author_sort |
Dietmar Silke Klemm |
title |
Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces |
title_short |
Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces |
title_full |
Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces |
title_fullStr |
Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces |
title_full_unstemmed |
Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces |
title_sort |
supersymmetric near-horizon geometry and einstein-cartan-weyl spaces |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2019-06-01 |
description |
We show that the horizon geometry for supersymmetric black hole solutions of minimal five-dimensional gauged supergravity is that of a particular Einstein-Cartan-Weyl (ECW) structure in three dimensions, involving the trace and traceless part of both torsion and nonmetricity, and obeying some precise constraints. In the limit of zero cosmological constant, the set of nonlinear partial differential equations characterizing this ECW structure reduces correctly to that of a hyper-CR Einstein-Weyl structure in the Gauduchon gauge, which was shown by Dunajski, Gutowski and Sabra to be the horizon geometry in the ungauged BPS case. Keywords: Supersymmetry, Supergravity, Near horizon geometry, Metric affine gravity |
url |
http://www.sciencedirect.com/science/article/pii/S0370269319302953 |
work_keys_str_mv |
AT dietmarsilkeklemm supersymmetricnearhorizongeometryandeinsteincartanweylspaces AT lucreziaravera supersymmetricnearhorizongeometryandeinsteincartanweylspaces |
_version_ |
1724947065768771584 |