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

页码：183 / 186

页数：4

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