Gravitational magnetic shocks as a detector of gravitational waves

dc.contributor.author	Ignat'ev Y.
dc.date.accessioned	2018-09-17T20:42:36Z
dc.date.available	2018-09-17T20:42:36Z
dc.date.issued	1997
dc.identifier.issn	0375-9601
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/133920
dc.description.abstract	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. © 1997 Published by Elsevier Science B.V.
dc.relation.ispartofseries	Physics Letters, Section A: General, Atomic and Solid State Physics
dc.title	Gravitational magnetic shocks as a detector of gravitational waves
dc.type	Article
dc.relation.ispartofseries-issue	3-4
dc.relation.ispartofseries-volume	230
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	171
dc.source.id	SCOPUS03759601-1997-230-34-SID0001248287

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Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.