Approximate Kerr-like interior and exterior solutions for a very slowly rotating star of perfect fluid

被引：0
|
作者：
Nikouravan, Bijan [1 ,2 ]
机构：
[1] IAU, Dept Phys & Astrophys, Varamin Pishva Branch, Tehran, Iran
[2] Univ Malaya, Dept Phys, Kuala Lumpur 50603, Malaysia
来源：
INTERNATIONAL JOURNAL OF THE PHYSICAL SCIENCES | 2011年 / 6卷 / 01期
关键词：
Slowly rotating oblate star; approximate Kerr-like metric; exterior interior solution; BODY;
D O I：
暂无
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
Approximate Kerr-like interior and exterior solutions for a very slowly rotating star of perfect fluid is presented here which is valid for a very slowly rotating and hence very slightly oblate star of perfect fluid rotating with a very small constant angular velocity. Corresponding approximate exterior metric represents approximate Kerr exterior metric for a perfect fluid. The aim here is to obtain Kerr-like approximate exterior and interior solutions for a very slowly rotating star of perfect fluid simply following standard procedure used to obtain Schwarzschild solutions.
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页码：93 / 97
页数：5
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