Stability of Quark Star Model

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dc.contributor.authorMardan Azmi, Syed Ali
dc.contributor.authorRehman, Muhammad Aziz
dc.date.accessioned2018-10-15T07:29:46Z
dc.date.available2018-10-15T07:29:46Z
dc.date.issued2016-03-01
dc.description.abstractIn this paper, we investigate the stability of quark stars with four different types of inner matter configurations; isotropic, charged isotropic, anisotropic and charged anisotropic by using the concept of cracking. For this purpose, we have applied local density perturbations technique to the hydrostatic equilibrium equation as well as on physical parameters involved in the model. We conclude that quark stars become potentially unstable when inner matter configuration is changed and electromagnetic field is applied.en_US
dc.identifier.citationAzam, M., Mardan, S.A., & Rehman, M.A. (2016). Stability of Quark Star Model. Communications in Theoretical Physics, 65, 575–584. (Syed Ali Mardan Azmi (Mathematics /SSC), Muhammad Aziz-ur-Rehman, JCR LISTED (IF:0:948))en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/3213
dc.language.isoenen_US
dc.publisherCommunications in Theoretical Physics, IOP Sciencesen_US
dc.subjectMathematicsen_US
dc.subjectQuark stars, Cracking, Density perturbations, Electromagnetic field.en_US
dc.titleStability of Quark Star Modelen_US
dc.typeArticleen_US
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