.png){kind=icon}
返回
A generalized model for compact stars
.png){kind=icon}
OA
AI
DOI：10.1140/epjc/s10052-016-4090-0.png)
.png){kind=icon}
原文求助.png){kind=icon}
分享.png){kind=icon}
收藏
摘要
En 中文
By virtue of the maximum entropy principle, we get an Euler-Lagrange equation which is a highly nonlinear differential equation containing the mass function and its derivatives. Solving the equation by a homotopy perturbation method we derive a generalized expression for the mass which is a polynomial function of the radial distance. Using the mass function we find a partially stable configuration and its characteristics. We show that different physical features of the known compact stars, viz. Her X - 1, RX J 1856 - 37, SAX J (SS1), SAX J (SS2), and PSR J 1614 - 2230, can be explained by the present model.
Keyword:
HOMOTOPY PERTURBATION METHOD
ENTROPY
期刊
IF:
4.8
论文数:
1.8W
被引数:
4.7W
.png){kind=icon}
查看更多内容