Anisotropic stars for spherically symmetric spacetimes satisfying the Karmarkar condition

被引：60

作者：

Maurya, S. K. ^{[1
]}

Ratanpal, B. S. ^{[2
]}

Govender, M. ^{[3
]}

机构：

[1] Univ Nizwa, Dept Math & Phys Sci, Coll Arts & Sci, Nizwa, Oman

[2] Maharaja Sayajirao Univ Baroda, Fac Technol & Engn, Dept Appl Math, Vadodara 390001, India

[3] Durban Univ Technol, Fac Sci Appl, Dept Math, Durban, South Africa

来源：

ANNALS OF PHYSICS | 2017年 / 382卷

关键词：

General relativity; Pressure anisotropy; Karmarkar condition; Compact stars; CHARGED COMPACT STARS; EQUATION-OF-STATE; SUPERDENSE STAR; MAXIMUM MASS; NEW-MODEL; CRACKING; ENVELOPE; OBJECTS; SPHERES; ANALOG;

D O I：

10.1016/j.aop.2017.04.008

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A new class of solution describing an anisotropic stellar configuration satisfying Karmarkar's condition i.e. spherically symmetric metric of embedding class 1, is reported. It has been shown that the compact star model is physically well-behaved and meet all the physical requirements for a stable configuration in hydrostatic equilibrium. Our model describes compact stars like Vela X-1 and 4U1608-52 to a very good approximation. (C) 2017 Elsevier Inc. All rights reserved.

引用

页码：36 / 49

页数：14

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