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Article: Anisotropic relativistic stellar models

TitleAnisotropic relativistic stellar models
Authors
Harko, TMak, MK
KeywordsAnisotropic Stars
Einstein's Field Equations
Static Interior Solutions
Issue Date2002
PublisherWiley - V C H Verlag GmbH & Co KGaA. The Journal's web site is located at http://www.wiley-vch.de/home/adp
Citation
Annalen der Physik (Leipzig), 2002, v. 11 n. 1, p. 3-13 How to Cite?
DOI: http://dx.doi.org/10.1002/1521-3889(200201)11:1<3::AID-ANDP3>3.0.CO;2-L
AbstractWe present a class of exact solutions of Einstein's gravitational field equations describing spherically symmetric and static anisotropic stellar type configurations. The solutions are obtained by assuming a particular form of the anisotropy factor. The energy density and both radial and tangential pressures are finite and positive inside the anisotropic star. Numerical results show that the basic physical parameters (mass and radius) of the model can describe realistic astrophysical objects like neutron stars.
Persistent Identifierhttp://hdl.handle.net/10722/91810
ISSN
0003-3804
2021 Impact Factor: 3.012
2020 SCImago Journal Rankings: 1.009
ISI Accession Number ID
WOS:000173290100001
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorHarko, Ten_HK
dc.contributor.authorMak, MKen_HK
dc.date.accessioned2010-09-17T10:27:16Z-
dc.date.available2010-09-17T10:27:16Z-
dc.date.issued2002en_HK
dc.identifier.citationAnnalen der Physik (Leipzig), 2002, v. 11 n. 1, p. 3-13en_HK
dc.identifier.issn0003-3804en_HK
dc.identifier.urihttp://hdl.handle.net/10722/91810-
dc.description.abstractWe present a class of exact solutions of Einstein's gravitational field equations describing spherically symmetric and static anisotropic stellar type configurations. The solutions are obtained by assuming a particular form of the anisotropy factor. The energy density and both radial and tangential pressures are finite and positive inside the anisotropic star. Numerical results show that the basic physical parameters (mass and radius) of the model can describe realistic astrophysical objects like neutron stars.en_HK
dc.languageengen_HK
dc.publisherWiley - V C H Verlag GmbH & Co KGaA. The Journal's web site is located at http://www.wiley-vch.de/home/adpen_HK
dc.relation.ispartofAnnalen der Physik (Leipzig)en_HK
dc.subjectAnisotropic Starsen_HK
dc.subjectEinstein's Field Equationsen_HK
dc.subjectStatic Interior Solutionsen_HK
dc.titleAnisotropic relativistic stellar modelsen_HK
dc.typeArticleen_HK
dc.identifier.emailHarko, TC:harko@hkucc.hku.hken_HK
dc.identifier.authorityHarko, TC=rp1333en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1002/1521-3889(200201)11:1<3::AID-ANDP3>3.0.CO;2-Len_HK
dc.identifier.scopuseid_2-s2.0-0036157363en_HK
dc.identifier.hkuros77010-
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0036157363&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume11en_HK
dc.identifier.issue1en_HK
dc.identifier.spage3en_HK
dc.identifier.epage13en_HK
dc.identifier.isiWOS:000173290100001-
dc.identifier.issnl0003-3804-

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