| dc.contributor.author |
Thirukkanesh, S. |
|
| dc.contributor.author |
Ragel, F. C. |
|
| dc.date.accessioned |
2019-08-07T04:21:41Z |
|
| dc.date.available |
2019-08-07T04:21:41Z |
|
| dc.date.issued |
2017 |
|
| dc.identifier.issn |
1674-1137 |
|
| dc.identifier.uri |
http://www.digital.lib.esn.ac.lk/handle/123456789/3920 |
|
| dc.description.abstract |
e report a general approach to solve an Einstein-Maxwell system to describe a static spherically symmetric anisotropic strange matter distribution with linear equation of state in terms of two generating functions. It is examined by choosing Tolmann IV type potential for one of the gravitational potentials and a physically reasonable choice for the electric field. Hence, the generated model satisfies all the required major physical properties of a realistic star. The effect of electric charge on physical properties is highlighted. |
en_US |
| dc.language.iso |
en |
en_US |
| dc.publisher |
CHINESE PHYSICAL SOC, PEOPLES R CHINA and IOP Publishing Ltd |
en_US |
| dc.title |
A realistic model for charged strange quark star |
en_US |
| dc.type |
Article |
en_US |
| dc.identifier.sslno |
02 |
en_US |
| dc.identifier.doi |
https://iopscience.iop.org/article/10.1088/1674-1137/41/1/015102 |
en_US |