AdS5 black strings in the stu model of FI-gauged N = 2 supergravity

Author:

Azzola Matteo,Klemm Dietmar,Rabbiosi Marco

Abstract

Abstract We analytically construct asymptotically AdS5 black string solutions starting from the four-dimensional domain wall black hole of [1]. It is shown that its uplift gives a black string in d = 5 minimal gauged supergravity, with momentum along the string. Applying instead the residual symmetries of N = 2, d = 4 Fayet-Iliopoulos-gauged super-gravity discovered in [2] to the domain wall seed leads, after uplifting, to a dyonic black string that interpolates between AdS5 and AdS3 × H2 at the horizon. A Kaluza-Klein reduction of the latter along an angular Killing direction ϕ followed by a duality transformation yields, after going back to five dimensions, a black string with both momentum along the string and rotation along ϕ. This is the first instance of using solution-generating techniques in gauged supergravity to add rotation to a given seed. These solutions all have constant scalar fields. As was shown in [3], the construction of supersymmetric static magnetic black strings in the FI-gauged stu model amounts to solving the SO(2, 1) spinning top equations, which descend from an inhomogeneous version of the Nahm equations. We are able to solve these in a particular case, which leads to a generalization of the Maldacena-Nuñez solution.

Publisher

Springer Science and Business Media LLC

Subject

Nuclear and High Energy Physics

Cited by 11 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. New supersymmetric $$AdS_5$$ black strings from 5D $$N=4$$ gauged supergravity;The European Physical Journal C;2023-05-23

2. c-functions in flows across dimensions;Journal of High Energy Physics;2022-10-13

3. N=(0,4) black string chains;Physical Review D;2022-04-19

4. Black hole superpotential as a unifying entropy function and BPS thermodynamics;Journal of High Energy Physics;2022-03-09

5. $$ \mathcal{N} $$ = (2, 2) AdS3 from D3-branes wrapped on Riemann surfaces;Journal of High Energy Physics;2022-02

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