Uniqueness theorem for black hole space-times with multiple disconnected horizons

Jácome Saldanha N de O B Armas; Troels Harmark

doi:10.1007/jhep05(2010)093

Uniqueness theorem for black hole space-times with multiple disconnected horizons

Jácome Saldanha N de O B Armas, Troels Harmark

13 Citations (Scopus)

Abstract

We show uniqueness of stationary and asymptotically flat black hole spacetimes with multiple disconnected horizons and with two rotational Killing vector fields in the context of five-dimensional minimal supergravity (Einstein-Maxwell-Chern-Simons gravity). The novelty in this work is the introduction in the uniqueness theorem of intrinsic local charges measured near each horizon as well as the measurement of local fluxes besides the asymptotic charges that characterize a particular solution. A systematic method of defining the boundary conditions on the fields that specify a black hole space-time is given based on the study of its rod structure (domain structure). Also, an analysis of known solutions with disconnected horizons is carried out as an example of an application of this theorem.

Original language	English
Journal	Journal of High Energy Physics (Online)
Volume	2010
Issue number	5
Pages (from-to)	093
ISSN	1126-6708
DOIs	https://doi.org/10.1007/jhep05(2010)093
Publication status	Published - 1 May 2010

Access to Document

10.1007/jhep05(2010)093

Cite this

@article{1c7ac0c3b04a4c7d81992d031272c161,

title = "Uniqueness theorem for black hole space-times with multiple disconnected horizons",

abstract = "We show uniqueness of stationary and asymptotically flat black hole spacetimes with multiple disconnected horizons and with two rotational Killing vector fields in the context of five-dimensional minimal supergravity (Einstein-Maxwell-Chern-Simons gravity). The novelty in this work is the introduction in the uniqueness theorem of intrinsic local charges measured near each horizon as well as the measurement of local fluxes besides the asymptotic charges that characterize a particular solution. A systematic method of defining the boundary conditions on the fields that specify a black hole space-time is given based on the study of its rod structure (domain structure). Also, an analysis of known solutions with disconnected horizons is carried out as an example of an application of this theorem.",

author = "Armas, {J{\'a}come Saldanha N de O B} and Troels Harmark",

year = "2010",

month = may,

day = "1",

doi = "10.1007/jhep05(2010)093",

language = "English",

volume = "2010",

pages = "093",

journal = "Journal of High Energy Physics (Online)",

issn = "1126-6708",

publisher = "Springer",

number = "5",

}

TY - JOUR

T1 - Uniqueness theorem for black hole space-times with multiple disconnected horizons

AU - Armas, Jácome Saldanha N de O B

AU - Harmark, Troels

PY - 2010/5/1

Y1 - 2010/5/1

N2 - We show uniqueness of stationary and asymptotically flat black hole spacetimes with multiple disconnected horizons and with two rotational Killing vector fields in the context of five-dimensional minimal supergravity (Einstein-Maxwell-Chern-Simons gravity). The novelty in this work is the introduction in the uniqueness theorem of intrinsic local charges measured near each horizon as well as the measurement of local fluxes besides the asymptotic charges that characterize a particular solution. A systematic method of defining the boundary conditions on the fields that specify a black hole space-time is given based on the study of its rod structure (domain structure). Also, an analysis of known solutions with disconnected horizons is carried out as an example of an application of this theorem.

AB - We show uniqueness of stationary and asymptotically flat black hole spacetimes with multiple disconnected horizons and with two rotational Killing vector fields in the context of five-dimensional minimal supergravity (Einstein-Maxwell-Chern-Simons gravity). The novelty in this work is the introduction in the uniqueness theorem of intrinsic local charges measured near each horizon as well as the measurement of local fluxes besides the asymptotic charges that characterize a particular solution. A systematic method of defining the boundary conditions on the fields that specify a black hole space-time is given based on the study of its rod structure (domain structure). Also, an analysis of known solutions with disconnected horizons is carried out as an example of an application of this theorem.

U2 - 10.1007/jhep05(2010)093

DO - 10.1007/jhep05(2010)093

M3 - Journal article

SN - 1126-6708

VL - 2010

SP - 093

JO - Journal of High Energy Physics (Online)

JF - Journal of High Energy Physics (Online)

IS - 5

ER -

Uniqueness theorem for black hole space-times with multiple disconnected horizons

Abstract

Access to Document

Fingerprint

Cite this