["languages_typename_ge" not defined]Clear Cookie - decide language by browser settings

Polarized Cosmological Gravitational Waves from Primordial Helical Turbulence

Kahniashvili, Tina and Gogoberidze, Grigol and Ratra, Bharat (2005) Polarized Cosmological Gravitational Waves from Primordial Helical Turbulence. Physical Review Letters, 95.

[img]
Preview
 Text
kgr05.pdf
Download (160kB) | Preview

Abstract

We show that helical turbulence produced during a first-order phase transition generates circularly polarized cosmological gravitational waves (GWs). The characteristic frequency of these GWs for an extreme case of the phase transition model is around 10-3-10-2Hz with an energy density parameter as high as 10-12-10-11. The possibility of detection is briefly discussed.

Item Type: Article
Subjects: Q Science > QC Physics
Depositing User: Prof. Tina Kahniashvili
Date Deposited: 27 Jan 2014 20:08
Last Modified: 27 Mar 2015 06:56
URI: http://eprints.iliauni.edu.ge/id/eprint/725

Actions (login required)

View Item View Item
eprints is powered by EPrints 3 which is developed by the School of Electronics and Computer Science at the University of Southampton. More information and software credits.