Relativistic model of radiating massive fluid sphere

被引：0
|
作者：
Neeraj Pant
R. N. Mehta
B. C. Tewari
机构：
[1] National Defence Academy Khadakwasla,Department of Mathematics
[2] Kumaun University,Department of Mathematics
来源：
Astrophysics and Space Science | 2010年 / 327卷
关键词：
General relativity; Quasar; Supernova burst;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
In this paper we present a new class of nonsingular solutions representing time dependent balls of perfect fluid with matter-radiation in general relativity. The solution of the class is suitable for interior modeling of a quasar i.e. a massive radiating star. The interior solution is matched with a zero pressure Vaidya metric. From this solution we constructed a quasar model by assuming the life time of the quasar of ≈107 year. We obtained a mass of the quasar of ≈109 Mθ, linear dimension ≈1017 km and a rate of emission L∞≈1047 erg/s.
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页码：279 / 283
页数：4
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