Charged black holes in compactified space times.

J 2005

Charged black holes in compactified space times.

VON UNGE, Rikard a Max Erik KARLOVINI

Základní údaje

Originální název

Charged black holes in compactified space times.

Název česky

Nabite cerne diry v kompaktifikovane prostorucasy.

Autoři

VON UNGE, Rikard a Max Erik KARLOVINI

Vydání

Physical Review D, 2005, 1550-7998

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10301 Atomic, molecular and chemical physics

Stát vydavatele

Spojené státy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 4.852

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/05:00014357

Organizační jednotka

Přírodovědecká fakulta

UT WoS

000233608800055

Klíčová slova anglicky

black holes; compactification

Štítky

black holes, compactification

Změněno: 1. 4. 2010 12:14, prof. Rikard Sebastian von Unge, Ph.D.

Anotace

ORIG CZ

V originále

We construct and investigate a compactified version of the four-dimensional Reissner-Nordstrom-NUT solution, generalizing the compactified Schwarzschild black hole that has been previously studied by several workers. Our approach to compactification is based on dimensional reduction with respect to the stationary Killing vector, resulting in three-dimensional gravity coupled to a nonlinear sigma model. Using that the original non-compactified solution corresponds to a target space geodesic, the problem can be linearized much in the same way as in the case of no electric nor NUT charge. An interesting feature of the solution family is that for nonzero electric charge but vanishing NUT charge, the solution has a curvature singularity on a torus that surrounds the event horizon, but this singularity is removed when the NUT charge is switched on. We also treat the Schwarzschild case in a more complete way than has been done previously. In particular, the asymptotic solution (the Levi-Civita solution with the height coordinate made periodic) has to our knowledge only been calculated up to a determination of the mass parameter. The periodic Levi-Civita solution contains three essential parameters, however, and the remaining two are explicitly calculated here.

Česky

Studujeme nabite cerne diry v kompaktifikovanem prostorucase,

Návaznosti

MSM0021622409, záměr

Název: Matematické struktury a jejich fyzikální aplikace

Investor: Ministerstvo školství, mládeže a tělovýchovy ČR, Matematické struktury a jejich fyzikální aplikace

Citovat

VON UNGE, Rikard a Max Erik KARLOVINI. Charged black holes in compactified space times. Physical Review D. 2005, roč. 2005, č. 72, s. 104013-104033, 20 s. ISSN 1550-7998.

@article{598644,
   author = {von Unge, Rikard and Karlovini, Max Erik},
   article_number = {72},
   keywords = {black holes; compactification},
   language = {eng},
   issn = {1550-7998},
   journal = {Physical Review D},
   title = {Charged black holes in compactified space times.},
   url = {http://arXiv.org/pdf/gr-qc/0506073},
   volume = {2005},
   year = {2005}
}

TY  - JOUR
ID  - 598644
AU  - von Unge, Rikard - Karlovini, Max Erik
PY  - 2005
TI  - Charged black holes in compactified space times.
JF  - Physical Review D
VL  - 2005
IS  - 72
SP  - 104013-104033
EP  - 104013-104033
SN  - 15507998
KW  - black holes
KW  - compactification
UR  - http://arXiv.org/pdf/gr-qc/0506073
N2  - We construct and investigate a compactified version of the four-dimensional Reissner-Nordstrom-NUT solution, generalizing the compactified Schwarzschild black hole that has been previously studied by several workers. Our approach to compactification is based on dimensional reduction with respect to the stationary Killing vector, resulting in three-dimensional gravity coupled to a nonlinear sigma model. Using that the original non-compactified solution corresponds to a target space geodesic, the problem can be linearized much in the same way as in the case of no electric nor NUT charge. An interesting feature of the solution family is that for nonzero electric charge but vanishing NUT charge, the solution has a curvature singularity on a torus that surrounds the event horizon, but this singularity is removed when the NUT charge is switched on. We also treat the Schwarzschild case in a more complete way than has been done previously. In particular, the asymptotic solution (the Levi-Civita solution with the height coordinate made periodic) has to our knowledge only been calculated up to a determination of the mass parameter. The periodic Levi-Civita solution contains three essential parameters, however, and the remaining two are explicitly calculated here.
ER  -

VON UNGE, Rikard a Max Erik KARLOVINI. Charged black holes in compactified space times. \textit{Physical Review D}. 2005, roč.~2005, č.~72, s.~104013-104033, 20 s. ISSN~1550-7998.

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