Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10321647" target="_blank" >RIV/00216208:11320/15:10321647 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/67985840:_____/15:00441470

Výsledek na webu

<a href="http://dx.doi.org/10.1007/JHEP02(2015)045" target="_blank" >http://dx.doi.org/10.1007/JHEP02(2015)045</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/JHEP02(2015)045" target="_blank" >10.1007/JHEP02(2015)045</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class

Popis výsledku v původním jazyce

We study Robinson-Trautman spacetimes in the presence of an aligned p-form Maxwell field and an arbitrary cosmological constant in n a parts per thousand yen 4 dimensions. As it turns out, the character of these exact solutions depends significantly on the (relative) value of n and p. In odd dimensions the solutions reduce to static black holes dressed with an electric and a magnetic field, with an Einstein space horizon (further constrained by the Einstein-Maxwell equations) - both the Weyl and Maxwelltypes are D. Even dimensions, however, open up more possibilities. In particular, when 2p = n there exist non-static solutions describing black holes gaining (or losing) mass by receiving (or emitting) electromagnetic radiation. In this case the Weyl type is II (D) and the Maxwell type can be II (D) or N. Conditions under which the Maxwell field is self-dual (for odd p) are also discussed, and a few explicit examples presented. Finally, the case p = 1 is special in all dimensions and le

Název v anglickém jazyce

Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class

Popis výsledku anglicky

We study Robinson-Trautman spacetimes in the presence of an aligned p-form Maxwell field and an arbitrary cosmological constant in n a parts per thousand yen 4 dimensions. As it turns out, the character of these exact solutions depends significantly on the (relative) value of n and p. In odd dimensions the solutions reduce to static black holes dressed with an electric and a magnetic field, with an Einstein space horizon (further constrained by the Einstein-Maxwell equations) - both the Weyl and Maxwelltypes are D. Even dimensions, however, open up more possibilities. In particular, when 2p = n there exist non-static solutions describing black holes gaining (or losing) mass by receiving (or emitting) electromagnetic radiation. In this case the Weyl type is II (D) and the Maxwell type can be II (D) or N. Conditions under which the Maxwell field is self-dual (for odd p) are also discussed, and a few explicit examples presented. Finally, the case p = 1 is special in all dimensions and le

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BE - Teoretická fyzika

OECD FORD obor

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Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Journal of High Energy Physics [online]

ISSN

1029-8479

e-ISSN

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Svazek periodika

neuveden

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

DE - Spolková republika Německo

Počet stran výsledku

39

Strana od-do

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Kód UT WoS článku

000349328500001

EID výsledku v databázi Scopus

2-s2.0-84946076509