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Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class
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SYSNO ASEP 0441470 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Static and radiating p-form black holes in the higher dimensional Robinson-Trautman class Tvůrce(i) Ortaggio, Marcello (MU-W) RID, SAI, ORCID
Podolský, J. (CZ)
Žofka, M. (CZ)Zdroj.dok. Journal of High Energy Physics. - : Springer - ISSN 1029-8479
Roč. 2015, č. 2 (2015), 045Poč.str. 39 s. Jazyk dok. eng - angličtina Země vyd. US - Spojené státy americké Klíč. slova Einstein-Maxwell spacetimes ; classical theories of gravity ; black holes Vědní obor RIV BA - Obecná matematika CEP GB14-37086G GA ČR - Grantová agentura ČR Institucionální podpora MU-W - RVO:67985840 UT WOS 000349328500001 EID SCOPUS 84946076509 DOI 10.1007/JHEP02(2015)045 Anotace We study Robinson-Trautman spacetimes in the presence of an aligned p-form Maxwell field and an arbitrary cosmological constant in n ≥ 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 Maxwell types 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 leads to static metrics. Pracoviště Matematický ústav Kontakt Jarmila Štruncová, struncova@math.cas.cz, library@math.cas.cz, Tel.: 222 090 757 Rok sběru 2016
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