Search For Gravitational Waves Through the Electromagnetic Faraday Rotation

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dc.creatorHalilsoy, Mustafa
dc.creatorGurtug, Ozay
dc.date2006-12-18
dc.date2007-06-13
dc.date.accessioned2026-07-07T11:01:31Z
dc.date.available2026-07-07T11:01:31Z
dc.descriptionA 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 non-linear process induces a detectable Faraday rotation in the polarization vector of the electromagnetic field.
dc.descriptionFinal version. Minor revision, new figures and references are added. To appear in Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0612107
dc.identifierhttp://arxiv.org/abs/gr-qc/0612107
dc.identifierPhys.Rev.D75:124021,2007
dc.identifierdoi:10.1103/PhysRevD.75.124021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187973
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSearch For Gravitational Waves Through the Electromagnetic Faraday Rotation
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