Dissipative spherical collapse of charged anisotropic fluid in f (r) gravity
| dc.contributor.author | H. Rizwana Kausar | |
| dc.contributor.author | Ifra Noureen | |
| dc.date.accessioned | 2014-04-10T10:36:10Z | |
| dc.date.available | 2014-04-10T10:36:10Z | |
| dc.date.issued | 2014 | |
| dc.description.abstract | This manuscript is devoted to study the combined effect of a viable f(R) = R + Rn model and electromagnetic field on the instability range of gravitational collapse. We assume charged anisotropic fluid that dissipate energy via heat flow and discuss that electromagnetic field, density inhomogeneity, shear and phase transition on astrophysi- cal bodies can be incorporated by locally anisotropic background. Dy- namical equations help to investigate the evolution of self-gravitating objects and leads to the conclusion that adiabatic index depend upon the electromagnetic background, mass and radius of the spherical ob- jects. | en_US |
| dc.identifier.citation | Kausar, H. R., & Noureen, I. (2014). Dissipative spherical collapse of charged anisotropic fluid in f (R) gravity. The European Physical Journal C, 74(2), 1-8. | en_US |
| dc.identifier.uri | https://escholar.umt.edu.pk/handle/123456789/1105 | |
| dc.language.iso | en | en_US |
| dc.publisher | The European Physical Journal C | en_US |
| dc.title | Dissipative spherical collapse of charged anisotropic fluid in f (r) gravity | en_US |
| dc.type | Article | en_US |