Nonlinear reflection from the surface of neutron stars and features of radio emission from the pulsar in the Crab nebula

被引：3
|
作者：
Kontorovich, V. M. [1 ,2 ]
机构：
[1] Natl Acad Sci Ukraine, Inst Radio Astron, Ul Iskusstv 4, UA-61002 Kharkov, Ukraine
[2] Kharkov Natl Univ, Pl Svobody 4, UA-61022 Kharkov, Ukraine
来源：
LOW TEMPERATURE PHYSICS | 2016年 / 42卷 / 08期
关键词：
SCATTERING;
D O I：
10.1063/1.4961488
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
There are no explanations for the high-frequency component of the emission from the pulsar in the Crab nebula, but it may be a manifestation of instability in nonlinear reflection from the star's surface. Radiation from relativistic positrons flying from the magnetosphere to the star and accelerated by the electric field of the polar gap is reflected. The instability involves stimulated scattering on surface waves. Published by AIP Publishing.
引用
收藏
页码：672 / 678
页数：7
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