Finite size effects on the Poynting-Robertson effect: A fully general relativistic treatment

被引：9
|
作者：
Oh, Jae Sok [2 ]
Kim, Hongsu [1 ]
Lee, Hyung Mok [2 ]
机构：
[1] Korea Astron & Space Sci Inst, KVN, Taejon 305348, South Korea
[2] Seoul Natl Univ, FPRD, Dept Phys & Astron, Seoul 151742, South Korea
来源：
NEW ASTRONOMY | 2011年 / 16卷 / 03期
关键词：
Poynting-Robertson effect; General relativity; Finite size effects; Radiation pressure; Radiation drag; Eddington luminosity; Schwarzschild metric; BLACK-HOLES;
D O I：
10.1016/j.newast.2010.07.008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Even since the first discovery of Poynting and Robertson, the radiation source has been treated as merely a point. Even in a very few studies where the size of the source has been taken into account, the treatment of the problem remained largely non-relativistic. In the present work, we address the issue of the finite size effects on the Poynting-Robertson effect in a fully relativistic manner for the first time. As a result, the emergence and the characteristic of the critical point/suspension orbit can be studied in a systematic and detailed manner. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码：183 / 186
页数：4
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