Quark star model with charged anisotropic matter
| dc.contributor.author | Sunzu, J. M. | |
| dc.contributor.author | Maharaj., S. D. | |
| dc.contributor.author | Ray, S. | |
| dc.date.accessioned | 2020-03-20T06:01:21Z | |
| dc.date.available | 2020-03-20T06:01:21Z | |
| dc.date.issued | 2014 | |
| dc.description | Full Text Article. Also available at: 10.1007/s10509-014-2131-4 | en_US |
| dc.description.abstract | We find two new classes of exact solutions to the Einstein-Maxwell system of equations. The matter distribution satisfies a linear equation of state consistent with quark matter. The field equations are integrated by specifying forms for the measure of anisotropy and a gravitational potential which are physically reasonable. The first class has a constant potential and is regular in the stellar interior. It contains the familiar Einstein model as a limiting case and we can generate finite masses for the star. The second class has a variable potential and singularity at the center. A graphical analysis indicates that the matter variables are well behaved. | en_US |
| dc.identifier.citation | Sunzu, J. M., Maharaj, S. D., & Ray, S. (2014). Quark star model with charged anisotropic matter. Astrophysics and Space Science, 354(2), 517-524. | en_US |
| dc.identifier.uri | 10.1007/s10509-014-2131-4 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12661/2231 | |
| dc.language.iso | en | en_US |
| dc.publisher | Springer | en_US |
| dc.subject | Gravitational potential | en_US |
| dc.subject | Linear equation | en_US |
| dc.subject | Quark matter | en_US |
| dc.subject | Anisotropy | en_US |
| dc.subject | Isotropic | en_US |
| dc.subject | Einstein-Maxwell equations | en_US |
| dc.subject | Einstein-Maxwell system | en_US |
| dc.subject | Einstein model | en_US |
| dc.title | Quark star model with charged anisotropic matter | en_US |
| dc.type | Article | en_US |