Search for gravitational waves through the electromagnetic Faraday rotation

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dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Gürtuğ, Özay
dc.date.accessioned	2017-10-19T08:24:51Z
dc.date.available	2017-10-19T08:24:51Z
dc.date.issued	2007
dc.identifier.issn	1550-7998 (Online)
dc.identifier.issn	1550-2368 (Print)
dc.identifier.uri	http://dx.doi.org/10.1103/PhysRevD.75.124021
dc.identifier.uri	http://hdl.handle.net/11129/3432
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	A method is given which renders indirect detection of strong gravitational waves possible. This is based on the reflection (collision) of a linearly polarized electromagnetic shock wave from (with) a cross polarized impulsive and shock gravitational waves in accordance with the general theory of relativity. This highly nonlinear process induces a detectable Faraday rotation in the polarization vector of the electromagnetic field.	en_US
dc.language.iso	eng	en_US
dc.publisher	AMER PHYSICAL SOC	en_US
dc.relation.isversionof	10.1103/PhysRevD.75.124021	en_US
dc.rights	info:eu-repo/semantics/openAccess	en_US
dc.subject	Faraday rotation in the polarization vector of the electromagnetic field. Remove selected	en_US
dc.title	Search for gravitational waves through the electromagnetic Faraday rotation	en_US
dc.type	article	en_US
dc.relation.journal	Physical Review D - Particles, Fields, Gravitation and Cosmology	en_US
dc.contributor.department	Eastern Mediterranean University, Faculty of Art & Sciences, Department of Physics	en_US
dc.identifier.volume	75	en_US
dc.identifier.issue	12	en_US
dc.identifier.startpage	1	en_US
dc.identifier.endpage	4	en_US