Possibility of radio-wave radiation production inside a pulsar

被引：4
|
作者：
Ahmedov, BJ
机构：
[1] Institute of Nuclear Physics, Ulughbek
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 1997年 / 6卷 / 03期
关键词：
D O I：
10.1142/S0218271897000182
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The influence of general-relativistic effects on charge distribution inside a neutron star is investigated. The qualitative distinction of space charge distribution inside the conducting crust from that inside the superconducting core allows us to propose a possible mechanism of radio-wave radiation produced in the intermediate medium inside a pulsar. The possibility of modeling this radiation in laboratory experiments in a rotating frame of reference is analyzed.
引用
收藏
页码：341 / 347
页数：7
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