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Propagation of gravitational waves in strong magnetic fields

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dc.contributor.author Bamba K.
dc.contributor.author Nojiri S.
dc.contributor.author Odintsov S.
dc.date.accessioned 2019-01-22T20:58:51Z
dc.date.available 2019-01-22T20:58:51Z
dc.date.issued 2018
dc.identifier.issn 2470-0010
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/149730
dc.description.abstract © 2018 American Physical Society. The propagation of gravitational waves is explored in the cosmological context. It is explicitly demonstrated that the propagation of gravitational waves could be influenced by the medium. It is shown that in the thermal radiation, the propagation of gravitational waves in general relativity is different from that in the scalar-tensor theory. The propagation of gravitational waves is investigated in the uniform magnetic field. As a result, it is found that cosmic magnetic fields could influence the propagation of gravitational waves to a non-negligible extent. The corresponding estimation for the spiral galaxy NGC 6946 effect is made.
dc.relation.ispartofseries Physical Review D
dc.title Propagation of gravitational waves in strong magnetic fields
dc.type Article
dc.relation.ispartofseries-issue 2
dc.relation.ispartofseries-volume 98
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS24700010-2018-98-2-SID85051138539


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  • Публикации сотрудников КФУ Scopus [17617]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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