dc.contributor.author |
Murad, Mohammad Hassan |
|
dc.contributor.author |
Fatema, Saba |
|
dc.date.accessioned |
2018-10-16T06:17:59Z |
|
dc.date.accessioned |
2019-05-27T09:57:15Z |
|
dc.date.available |
2018-10-16T06:17:59Z |
|
dc.date.available |
2019-05-27T09:57:15Z |
|
dc.date.issued |
2013-08-24 |
|
dc.identifier.uri |
http://hdl.handle.net/20.500.11948/3396 |
|
dc.description.abstract |
In continuation of recent work done by the present authors (Int. J. Theor. Phys. 2013, doi: 10.1007/s10773-013-1538-y, hereafter paper I) some new exact families of static spherically symmetric perfect fluid solution of Einstein–Maxwell gravitational field equations are presented. These solutions and the corresponding equations of state, presented in parametric form, may be astrophysically significant in constructing relativistic stellar models of electrically charged self-bound stars.
Full Text Link:https://doi.org/10.1007/s10773-013-1752-7 |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Springer |
en_US |
dc.subject |
General relativity |
en_US |
dc.subject |
Astrophysics |
en_US |
dc.subject |
Einstein–Maxwell Exact solution |
en_US |
dc.subject |
Charged fluid sphere |
en_US |
dc.subject |
Schwarzschild coordinates |
en_US |
dc.subject |
Compact stars |
en_US |
dc.subject |
Reissner–Nordström |
en_US |
dc.subject |
Relativistic stars |
en_US |
dc.subject |
Self-bound stars |
en_US |
dc.subject |
Equation of state |
en_US |
dc.title |
Some Exact Relativistic Models of Electrically Charged Self-bound Stars |
en_US |
dc.type |
Article |
en_US |