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A study on charged compact stars

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dc.contributor.authorMaurya, S. K.
dc.contributor.authorRay, S.
dc.contributor.authorAziz, A.
dc.contributor.authorChardonnet, P.
dc.contributor.authorKhlopov, M.
dc.contributor.authorХлопов, Максим Юрьевич
dc.date.accessioned2024-11-19T12:00:18Z
dc.date.available2024-11-19T12:00:18Z
dc.date.issued2019
dc.description.abstract© 2019 World Scientific Publishing Company. In this paper, the Einstein-Maxwell spacetime is considered for compact stellar system. To find out solutions of the field equations, we adopt a finite and positive well-behaved metric potential. Under this particular choice, we therefore develop the expressions of the physical features, such as mass, charge, density and pressure, for stellar system in embedding class 1 spacetime. It is observed that all these features are physically viable. In the model, some known compact stars, viz. 4U1820-30, 4U1608-52 and EXO1745-248(I)&(II) are studied successfully through physical analysis. It is also interesting to note that the obtained set of regular solutions to the Einstein-Maxwell equations represents an electromagnetic mass model for isotropic fluid without invoking any negative pressure.
dc.identifier.citationA study on charged compact stars / Maurya, S.K. [et al.] // International Journal of Modern Physics D. - 2019. - 28. - № 3. - 10.1142/S0218271819500536
dc.identifier.doi10.1142/S0218271819500536
dc.identifier.urihttps://www.doi.org/10.1142/S0218271819500536
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dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000458146700011
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/16400
dc.relation.ispartofInternational Journal of Modern Physics D
dc.titleA study on charged compact stars
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue3
oaire.citation.volume28
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