Please use this identifier to cite or link to this item: http://hdl.handle.net/10321/2948
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dc.contributor.authorSingh, K.N.-
dc.contributor.authorPant, N.-
dc.contributor.authorGovender, Megandhren-
dc.date.accessioned2018-04-09T07:41:37Z-
dc.date.available2018-04-09T07:41:37Z-
dc.date.issued2016-05-12-
dc.identifier.citationSingh, K.N., Pant, N. and Govender M. 2016. Some analytic models of relativistic compact stars. Indian Journal of Physics. 90(11): 1215–1223.en_US
dc.identifier.issn0019-5480 (print)-
dc.identifier.issn0974-9845 (online)-
dc.identifier.urihttp://hdl.handle.net/10321/2948-
dc.description.abstractWe present charged anisotropic Durgapal IV interior solutions of the general relativistic field equations in curvature coordinates. These exact solutions can be used to model stable and well-behaved compact stars. Using these solutions we have presented models of well-known neutron and quark stars such as PSR J1903?0327, RX-J1856.5-3754, PSR B1913?16, PSR J0737-3039A and Cyg X-2. The equation of state (EoS) corresponding to the modeled objects are studied using their compression moduli. According to our solutions it is found that the EoS for Cyg X-2 (neutron star) is stiffer than any other object presented and therefore more massive. Furthermore, the EoS for RX J1856.5-3754 (Quark star) is the softest one, rendering it least massive. These solutions satisfy all the energy conditions. Finally, all our presented stellar models satisfy the equilibrium condition of Cooperstock and de la Cruz i.e. M2 [Q2.en_US
dc.format.extent9 pen_US
dc.language.isoenen_US
dc.publisherSpringer Verlagen_US
dc.subjectGeneral relativityen_US
dc.subjectExact solutionsen_US
dc.subjectCold staren_US
dc.subjectAnisotropyen_US
dc.titleSome analytic models of relativistic compact starsen_US
dc.typeArticleen_US
dc.publisher.urihttps://link.springer.com/content/pdf/10.1007%2Fs12648-016-0870-5.pdfen_US
dc.dut-rims.pubnumDUT-005783en_US
dc.description.availabilityCopyright: 2016. Springer Verlag. 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 Indian Journal of Physics, Vol 90, No. 1. Pp 1215-1223. https://link.springer.com/content/pdf/10.1007%2Fs12648-016-0870-5.pdfen_US
item.grantfulltextnone-
item.fulltextNo Fulltext-
Appears in Collections:Research Publications (Applied Sciences)
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