Black hole and cosmos with multiple horizons and multiple singularities in vector-tensor theories - INSPIRE

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Black hole and cosmos with multiple horizons and multiple singularities in vector-tensor theories

Changjun Gao
(
- NAOC, Beijing
)
,
Youjun Lu
(
- NAOC, Beijing
)
,
Shuang Yu
(
- NAOC, Beijing
)
,
You-Gen Shen
(
- Shanghai, Astron. Observ.
)

Nov 2, 2017

14 pages

Published in:

Phys.Rev.D 97 (2018) 10, 104013

Published: May 15, 2018

e-Print:

1711.00996 [gr-qc]

DOI:

10.1103/PhysRevD.97.104013

View in:

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Abstract: (APS)

A stationary and spherically symmetric black hole (e.g., Reissner-Nordström black hole or Kerr-Newman black hole) has, at most, one singularity and two horizons. One horizon is the outer event horizon and the other is the inner Cauchy horizon. Can we construct static and spherically symmetric black hole solutions with N horizons and M singularities? The de Sitter cosmos has only one apparent horizon. Can we construct cosmos solutions with N horizons? In this article, we present the static and spherically symmetric black hole and cosmos solutions with N horizons and M singularities in the vector-tensor theories. Following these motivations, we also construct the black hole solutions with a firewall. The deviation of these black hole solutions from the usual ones can be potentially tested by future measurements of gravitational waves or the black hole continuum spectrum.

Note:

14 pages, 7 figures. The Penrose diagrams are corrected. PRD accepted

04.70.Bw
04.20.Jb
04.40.-b
11.27.+d
symmetry: rotation
horizon: multiple
black hole: Kerr-Newman
singularity
gravitational radiation
black hole: Reissner-Nordstroem

References(110)

Figures(7)

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