Scattering of spinning bodies by a radiation field in Schwarzschild spacetime

被引：0
|
作者：
Bini, D. [1 ,2 ,3 ]
Geralico, A. [2 ,4 ]
机构：
[1] CNR, Ist Applicazioni Calcolo M Picone, Via Manzoni,30, I-00185 Rome, Italy
[2] Univ Roma La Sapienza, ICRA, I-00185 Rome, Italy
[3] INFN, Sez Firenze, I-50019 Sesto Fiorentino, FI, Italy
[4] Univ Roma La Sapienza, I-00185 Rome, Italy
来源：
NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS | 2013年 / 36卷 / 01期
关键词：
D O I：
10.1393/ncc/i2013-11501-y
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We extend the analysis of Poynting-Robertson effect, i.e., the deviation from geodesic motion of test particles due to scattering by a superposed radiation field to the Schwarzschild background, to the case of spinning bodies. The extra contribution of the deviation due to spin can be relevant for astrophysical systems like the binary pulsar system PSR J0737- 3039 orbiting Sgr A*, but not for the Earth-Sun system.
引用
收藏
页码：37 / 42
页数：6
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