| dc.contributor.author |
Thirukkanesh, S. |
|
| dc.contributor.author |
Ragel, F. C. |
|
| dc.date.accessioned |
2019-08-07T04:45:53Z |
|
| dc.date.available |
2019-08-07T04:45:53Z |
|
| dc.date.issued |
2014 |
|
| dc.identifier.issn |
0004-640X |
|
| dc.identifier.uri |
http://www.digital.lib.esn.ac.lk/handle/123456789/3924 |
|
| dc.description.abstract |
We report a general solution in one of the gravitational potentials to the Einstein system in static spherically symmetric spacetime, modeling anisotropic strange quark matter by imposing a linear barotropic equation of state. The model generated by choosing Tolmann IV form for the gravitational potential is shown to contain the previously known anisotropic dark energy star model of Lobo (Class. Quantum Gravity 23:1525, 2006) and isotropic models of de Sitter and Einstein. Moreover, the model is shown to be physically admissible and corroborate with experimental observations on strange star candidates such as SAX J1808.4-3658 and 4U 1820-30. |
en_US |
| dc.language.iso |
en |
en_US |
| dc.publisher |
Astrophysics and Space Science |
en_US |
| dc.subject |
Einstein field equations |
en_US |
| dc.subject |
Equation of state |
en_US |
| dc.subject |
Strange star |
en_US |
| dc.title |
Strange star model with Tolmann IV type potential |
en_US |
| dc.type |
Article |
en_US |
| dc.identifier.sslno |
06 |
en_US |
| dc.identifier.doi |
https://link.springer.com/article/10.1007%2Fs10509-014-1960-5 |
en_US |