The stability of some viable stars and electromagnetic field.

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dc.contributor.authorSyed Ali Mardan Azmi
dc.contributor.authorMuhammad Aziz Ur Rehman
dc.date.accessioned2018-10-15T10:37:49Z
dc.date.available2018-10-15T10:37:49Z
dc.date.issued2016
dc.description.abstractWe examine the impact of electromagnetic field on the stability of compact stars corresponding to embedded class one metric using the concept of cracking. For this purpose, we develop the generalized hydrostatic equilibrium equation for charged perfect fluid distribution of compact stars and perturb it by means of local density perturbation scheme to check the stability of inner matter configuration. We investigate the cracking of Her X-1, PSR 1937+21, PSR J 1614-2230, PSR J 0348+0432 and RX J 1856-37. We conclude that PSR J 0348+0432 and RX J 1856-37 exhibit cracking when charge is introduced on these astrophysical objects.en_US
dc.identifier.citationAzam, M., Mardan, S. A., & Rehman, M. A. (2016). The stability of some viable stars and electromagnetic field. Chinese Physics Letters, 33(7), 1-4. (Syed Ali Mardan Azmi (Mathematics /SSC), Muhammad Aziz ur Rehman, JCR LISTED (IF:0:875))en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/3244
dc.language.isoenen_US
dc.publisherChinese Physics Letters, Springer Linken_US
dc.subjectMathematicsen_US
dc.titleThe stability of some viable stars and electromagnetic field.en_US
dc.typeArticleen_US
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