Rotating black holes in the FI-gauged N = 2, D = 4 ℂ P ¯ n $$ {\overline{\mathbb{C}\mathrm{P}}}^{\mathrm{n}} $$ model

Rotating black holes in the FI-gauged N = 2, D = 4 ℂ P ¯ n $$ {\overline{\mathbb{C}\mathrm{P}}}^{\mathrm{n}} $$ model

Abstract We construct supersymmetric black holes with rotation or NUT charge for the ℂ P ¯ n $$ {\overline{\mathbb{C}\mathrm{P}}}^n $$ — and the t3 model of N = 2, D = 4 U(1) FI-gauged supergravity. The solutions preserve 2 real supercharges, which are doubled for their near-horizon geometry. For th...

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Bibliographic Details
Main Authors: Nicoletta Daniele, Federico Faedo, Dietmar Klemm, Pedro F. Ramírez
Format: Article
Language:English
Published: SpringerOpen 2019-03-01
Series:Journal of High Energy Physics
Subjects:
AdS-CFT Correspondence
Black Holes
Classical Theories of Gravity
Supergravity Models
Online Access:http://link.springer.com/article/10.1007/JHEP03(2019)151

Internet

http://link.springer.com/article/10.1007/JHEP03(2019)151

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