Thin Static Charged Dust Majumdar?Papapetrou Shells with High Symmetry in D>=4

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F12%3A00060369" target="_blank" >RIV/00216224:14310/12:00060369 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68081723:_____/12:00377268

Výsledek na webu

<a href="http://www.springerlink.com/content/j42k542322j573h8/" target="_blank" >http://www.springerlink.com/content/j42k542322j573h8/</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/s10773-012-1126-6" target="_blank" >10.1007/s10773-012-1126-6</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Thin Static Charged Dust Majumdar?Papapetrou Shells with High Symmetry in D>=4

Popis výsledku v původním jazyce

We present a systematical study of static D>=4 spacetimes of high symmetry with the matter source being a thin charged dust hypersurface shell. The shell manifold is assumed to have the following structure S{beta}xR{D-2-beta}, {beta}in{0,...,D-2} is dimension of a sphere S{beta} . In case of {beta}=0, we assume that there are two parallel hyperplane shells instead of only one. The spacetime has MajumdarPapapetrou form and it inherits the symmetries of the shell manifold it is invariant under both rotations of the S{beta} and translations along R{D-2-beta} . We find a general solution to the EinsteinMaxwell equations with a given shell. Then, we examine some flat interior solutions with special attention paid to D=4. A connection to D=4 nonrelativistictheory is pointed out. We also comment on a straightforward generalisation to the case of KastorTraschen spacetime, i.e. adding a nonnegative cosmological constant to the charged dust matter source.

Název v anglickém jazyce

Thin Static Charged Dust Majumdar?Papapetrou Shells with High Symmetry in D>=4

Popis výsledku anglicky

We present a systematical study of static D>=4 spacetimes of high symmetry with the matter source being a thin charged dust hypersurface shell. The shell manifold is assumed to have the following structure S{beta}xR{D-2-beta}, {beta}in{0,...,D-2} is dimension of a sphere S{beta} . In case of {beta}=0, we assume that there are two parallel hyperplane shells instead of only one. The spacetime has MajumdarPapapetrou form and it inherits the symmetries of the shell manifold it is invariant under both rotations of the S{beta} and translations along R{D-2-beta} . We find a general solution to the EinsteinMaxwell equations with a given shell. Then, we examine some flat interior solutions with special attention paid to D=4. A connection to D=4 nonrelativistictheory is pointed out. We also comment on a straightforward generalisation to the case of KastorTraschen spacetime, i.e. adding a nonnegative cosmological constant to the charged dust matter source.

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

—

Návaznosti

S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2012

Kód důvěrnosti údajů

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

Název periodika

International Journal of Theoretical Physics

ISSN

0020-7748

e-ISSN

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Svazek periodika

51

Číslo periodika v rámci svazku

8

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

15

Strana od-do

2455-2469

Kód UT WoS článku

000305804300016

EID výsledku v databázi Scopus

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