Hairy black holes in scalar extended massive gravity

Andrew J. Tolley, De-Jun Wu, and Shuang-Yong Zhou
Phys. Rev. D 92, 124063 – Published 29 December 2015

Abstract

We construct static, spherically symmetric black hole solutions in scalar extended ghost-free massive gravity and show the existence of hairy black holes in this class of extension. While the existence seems to be a generic feature, we focus on the simplest models of this extension and find that asymptotically flat hairy black holes can exist without fine-tuning the theory parameters, unlike the bi-gravity extension, where asymptotical flatness requires fine-tuning in the parameter space. Like the bi-gravity extension, we are unable to obtain asymptotically dS regular black holes in the simplest models considered, but it is possible to obtain asymptotically AdS black holes.

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  • Received 30 October 2015

DOI:https://doi.org/10.1103/PhysRevD.92.124063

© 2015 American Physical Society

Authors & Affiliations

Andrew J. Tolley1,*, De-Jun Wu2,†, and Shuang-Yong Zhou1,‡

  • 1Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA
  • 2School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China

  • *andrew.j.tolley@case.edu
  • wudejun10@mails.ucas.ac.cn
  • sxz353@case.edu

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Issue

Vol. 92, Iss. 12 — 15 December 2015

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