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2010-07-13

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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/131718

New class of accelerating black hole solutions

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https://doi.org/10.1103/PhysRevD.82.024009

Abstract

We construct several new families of vacuum solutions that describe black holes in uniformly accelerated motion. They generalize the C metric to the case where the energy density and tension of the strings that pull (or push) on the black holes are independent parameters. These strings create large curvatures near their axis and when they have infinite length they modify the asymptotic properties of the spacetime, but we discuss how these features can be dealt with physically, in particular, in terms of "wiggly cosmic strings." We comment on possible extensions and extract lessons for the problem of finding higher-dimensional accelerating black hole solutions.

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Física de partícules, Experiments, Forats negres (Astronomia)

Subject (English)

Particle physics, Experiments, Black holes (Astronomy)

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Articles publicats en revistes (Física Quàntica i Astrofísica)
Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))

Citation

CAMPS, Joan and EMPARAN GARCÍA DE SALAZAR, Roberto A. New class of accelerating black hole solutions. Physical Review D. 2010. Vol. 82, num. 2, pags. 024009. ISSN 1550-7998. [consulted: 9 of June of 2026]. Available at: https://hdl.handle.net/2445/131718

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