Gravitational magnetic shocks as a detector of gravitational waves

被引:19
作者
Ignatev, YG
机构
[1] Department of Geometry, Kazan State Pedagogical University, Kazan 420021
关键词
D O I
10.1016/S0375-9601(97)00236-3
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Gravitational magnetic shock waves, the effect of excitation of a gravitational wave (GW) on shock waves in a highly magnetized plasma, are studied as an effective means for the detection of GW radiated by neutron stars. It is shown that there is every reason to identify the giant impulses of the pulsar NP 0532 with GMSW. (C) 1997 Published by Elsevier Science B.V.
引用
收藏
页码:171 / 176
页数:6
相关论文
共 19 条
[1]   THE EFFECT OF A GRAVITATIONAL-WAVE AT THE CONTACT OF CONDUCTORS [J].
BALAKIN, AB ;
IGNATEV, JG .
PHYSICS LETTERS A, 1983, 96 (01) :10-12
[2]  
BALAKIN AB, 1984, PROBLEMS THEORY GRAV, P43
[3]  
Ignat'ev Yu. G., 1979, Ukrayins'kyi Fizychnyi Zhurnal, V24, P742
[4]  
IGNATEV YG, 1981, ZH EKSP TEOR FIZ+, V81, P3
[5]  
IGNATEV YG, 1995, GRAV COSMOL, V1, P287
[6]  
IGNATEV YG, 1981, IZV VUZ FIZ, V24, P20
[7]  
IGNATEV YG, 1996, GRAVITATION COSMOLOG, V2, P213
[8]  
IGNATEV YG, 1996, VESTNIK KGPU, V1, P313
[9]  
IGNATIEV YG, 1984, UKR FIZ ZH+, V29, P1025
[10]  
IGNATYEV YG, 1985, IZV VUZ FIZ+, V28, P74