Static and spherically symmetric two-mass solutions of Einstein-Maxwell equations with cosmological constant based on Nariai spacetime

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • Michael Fennen
  • Domenico Giulini

Organisationseinheiten

Externe Organisationen

  • Universität Bremen
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer045008
Seitenumfang23
FachzeitschriftClassical and quantum gravity
Jahrgang32
Ausgabenummer4
Frühes Online-Datum21 Jan. 2015
PublikationsstatusVeröffentlicht - Feb. 2015

Abstract

We show the existence of static, spherically symmetric spacetimes containing two stars of incompressible matter, possibly oppositely charged. The stars are held apart by the negative pressure of a positive cosmological constant but there is no cosmological horizon separating them. The spacetime between the stars is given by the Nariai solution, or a slight generalization thereof in the charged case.

ASJC Scopus Sachgebiete

Zitieren

Static and spherically symmetric two-mass solutions of Einstein-Maxwell equations with cosmological constant based on Nariai spacetime. / Fennen, Michael; Giulini, Domenico.
in: Classical and quantum gravity, Jahrgang 32, Nr. 4, 045008, 02.2015.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Fennen M, Giulini D. Static and spherically symmetric two-mass solutions of Einstein-Maxwell equations with cosmological constant based on Nariai spacetime. Classical and quantum gravity. 2015 Feb;32(4):045008. Epub 2015 Jan 21. doi: 10.48550/arXiv.1408.2713, 10.1088/0264-9381/32/4/045008
Download
@article{67bac85ed07740698c12586271b88c51,
title = "Static and spherically symmetric two-mass solutions of Einstein-Maxwell equations with cosmological constant based on Nariai spacetime",
abstract = "We show the existence of static, spherically symmetric spacetimes containing two stars of incompressible matter, possibly oppositely charged. The stars are held apart by the negative pressure of a positive cosmological constant but there is no cosmological horizon separating them. The spacetime between the stars is given by the Nariai solution, or a slight generalization thereof in the charged case.",
keywords = "Exact solution, General relativity, Nariai spacetime",
author = "Michael Fennen and Domenico Giulini",
year = "2015",
month = feb,
doi = "10.48550/arXiv.1408.2713",
language = "English",
volume = "32",
journal = "Classical and quantum gravity",
issn = "0264-9381",
publisher = "IOP Publishing Ltd.",
number = "4",

}

Download

TY - JOUR

T1 - Static and spherically symmetric two-mass solutions of Einstein-Maxwell equations with cosmological constant based on Nariai spacetime

AU - Fennen, Michael

AU - Giulini, Domenico

PY - 2015/2

Y1 - 2015/2

N2 - We show the existence of static, spherically symmetric spacetimes containing two stars of incompressible matter, possibly oppositely charged. The stars are held apart by the negative pressure of a positive cosmological constant but there is no cosmological horizon separating them. The spacetime between the stars is given by the Nariai solution, or a slight generalization thereof in the charged case.

AB - We show the existence of static, spherically symmetric spacetimes containing two stars of incompressible matter, possibly oppositely charged. The stars are held apart by the negative pressure of a positive cosmological constant but there is no cosmological horizon separating them. The spacetime between the stars is given by the Nariai solution, or a slight generalization thereof in the charged case.

KW - Exact solution

KW - General relativity

KW - Nariai spacetime

UR - http://www.scopus.com/inward/record.url?scp=84921956625&partnerID=8YFLogxK

U2 - 10.48550/arXiv.1408.2713

DO - 10.48550/arXiv.1408.2713

M3 - Article

AN - SCOPUS:84921956625

VL - 32

JO - Classical and quantum gravity

JF - Classical and quantum gravity

SN - 0264-9381

IS - 4

M1 - 045008

ER -