Related Experiment Video
Updated: Aug 7, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Polarized cosmological gravitational waves from primordial helical turbulence
Tina Kahniashvili1, Grigol Gogoberidze, Bharat Ratra
1Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, Kansas 66506, USA.
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(-2) Hz with an energy density parameter as high as 10(-12)-10(-11). The possibility of detection is briefly discussed.
Related Concept Videos
The Wave Nature of Light
Detection of Black Holes
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Electromagnetic Waves
Potential Due to a Polarized Object
Divergence and Curl of Magnetic Field
The Principle of Superposition and the Gravitational Field

