Gravitational Radiation from Primordial Helical Turbulence

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dc.creatorKahniashvili, Tina
dc.date2005-08-22
dc.date.accessioned2026-07-07T02:18:29Z
dc.date.available2026-07-07T02:18:29Z
dc.descriptionIn present talk I show that primordial helical turbulence produced during a first-order phase transition induces circularly polarized cosmological gravitational waves (GWs). The degree of polarization as well as the characteristic frequency and the amplitude of these GWs depend crucially on phase-transition model of primordial turbulence. I present a brief discussion on the possibility of detection.
dc.descriptionTalk given at ICTP workshop "Nonlinear Cosmology", ICTP, Trieste, Italy (May 2005). To appear in special volume of International Journal of Modern Physics D
dc.identifierhttps://arxiv.org/abs/astro-ph/0508459
dc.identifierhttp://arxiv.org/abs/astro-ph/0508459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9505
dc.subjectAstrophysics
dc.titleGravitational Radiation from Primordial Helical Turbulence
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