Regular Phantom Black Holes

K. A. Bronnikov and J. C. Fabris
Phys. Rev. Lett. 96, 251101 – Published 27 June 2006

Abstract

We study self-gravitating, static, spherically symmetric phantom scalar fields with arbitrary potentials (favored by cosmological observations) and single out 16 classes of possible regular configurations with flat, de Sitter, and anti–de Sitter asymptotics. Among them are traversable wormholes, bouncing Kantowski-Sachs (KS) cosmologies, and asymptotically flat black holes (BHs). A regular BH has a Schwarzschild-like causal structure, but the singularity is replaced by a de Sitter infinity, giving a hypothetic BH explorer a chance to survive. It also looks possible that our Universe has originated in a phantom-dominated collapse in another universe, with KS expansion and isotropization after crossing the horizon. Explicit examples of regular solutions are built and discussed. Possible generalizations include k-essence type scalar fields (with a potential) and scalar-tensor gravity.

  • Received 24 November 2005

DOI:https://doi.org/10.1103/PhysRevLett.96.251101

©2006 American Physical Society

Authors & Affiliations

K. A. Bronnikov1,2,* and J. C. Fabris3,†

  • 1Center for Gravitation and Fundamental Metrology, VNIIMS, 46 Ozyornaya Street, Moscow 119361, Russia
  • 2Institute of Gravitation and Cosmology, PFUR, 6 Miklukho-Maklaya Street, Moscow 117198, Russia
  • 3Departamento de Física, Universidade Federal do Espírito Santo, Vitória, 29060-900, Espírito Santo, Brazil

  • *Email address: kb20@yandex.ru
  • Email address: fabris@cce.ufes.br

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Issue

Vol. 96, Iss. 25 — 30 June 2006

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