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
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.
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页码:341 / 347
页数:7
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