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Please use this identifier to cite or link to this item: https://hdl.handle.net/10321/1455
DC FieldValueLanguage
dc.contributor.authorThirukkanesh, S.
dc.contributor.authorGovender, M.
dc.contributor.authorLortan, Darren Brendan
dc.date.accessioned2016-04-07T05:24:28Z
dc.date.available2016-04-07T05:24:28Z
dc.date.issued2015
dc.identifier.citationThirukkanesh, S.; Govender, M. and Lorton, D.B. 2015. Spherically symmetric static matter configurations with vanishing radial pressure. International Journal of Modern Physics D. Vol 24(1) :en_US
dc.identifier.issn0218-2718
dc.identifier.urihttp://hdl.handle.net/10321/1455
dc.descriptionCopyright: 2015.WorldScientific Publishing. Due to copyright restrictions, only the abstract is available. For access to the full text item, please consult the publisher's website. The definitive version of the work is published in International Journal of Modern Physics D, vol 24, Issue 1, January 2015en_US
dc.description.abstractWe present a new family of spherically symmetric, static solutions of the Einstein field equations in isotropic, comoving coordinates. The radial pressure at each interior point of these models vanishes yet equilibrium is still possible. The constant density Florides solution which describes the gravitational field inside an Einstein cluster is obtained as a special case of our solution-generating method. We show that our solutions can be utilized to model strange star candidates such as Her. X-1, SAX J1808.4-3658(SS2), SAX J1808.4-3658(SS1) and PSR J1614-2230.en_US
dc.language.isoenen_US
dc.publisherWorld Scientific Publishingen_US
dc.relation.ispartofInternational journal of modern physics D-
dc.subjectStatic spheresen_US
dc.subjectPressure anisotropyen_US
dc.subjectHydrostatic equilibriumen_US
dc.titleSpherically symmetric static matter configurations with vanishing radial pressureen_US
dc.typeArticleen_US
dc.dut-rims.pubnumDUT-004867en_US
dc.description.availabilityCopyright: 2015.WorldScientific Publishing. Due to copyright restrictions, only the abstract is available. For access to the full text item, please consult the publisher's website. The definitive version of the work is published in International Journal of Modern Physics D, vol 24, Issue 1, January 2015
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.languageiso639-1en-
item.openairetypeArticle-
item.grantfulltextnone-
item.cerifentitytypePublications-
Appears in Collections:Research Publications (Applied Sciences)
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