activity
20172021
most citedEvolution of hydromagnetic turbulence from the electroweak phase transition

120 citations · 162 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20211 cited

Leading-order nonlinear gravitational waves from reheating magnetogeneses

Yutong He, Alberto Roper Pol, Axel Brandenburg

We study the leading-order nonlinear gravitational waves (GWs) produced by an electromagnetic (EM) stress in reheating magnetogenesis scenarios. Both nonhelical and helical magneti…

gr-qc2021

The scalar, vector, and tensor modes in gravitational wave turbulence simulations

Axel Brandenburg, Grigol Gogoberidze, Tina Kahniashvili +3

We study the gravitational wave (GW) signal sourced by primordial turbulence that is assumed to be present at cosmological phase transitions like the electroweak and quantum chromo…

astro-ph.CO202041 cited

Circular Polarization of Gravitational Waves from Early-Universe Helical Turbulence

Tina Kahniashvili, Axel Brandenburg, Grigol Gogoberidze +2

We perform direct numerical simulations to compute the net circular polarization of gravitational waves from helical (chiral) turbulent sources in the early Universe for a variety…

astro-ph.CO2020

NANOGrav signal from MHD turbulence at QCD phase transition in the early universe

A. Neronov, A. Roper Pol, C. Caprini +1

The NANOGrav collaboration has recently reported evidence for the existence of a stochastic gravitational wave background in the 1-100 nHz frequency range. We argue that such backg…

astro-ph.SR2018

E and B polarizations from inhomogeneous and solar surface turbulence

Axel Brandenburg, Andrea Bracco, Tina Kahniashvili +4

Gradient- and curl-type or E- and B-type polarizations have been routinely analyzed to study the physics contributing to the cosmic microwave background polarization and galactic f…

astro-ph.CO2017120 cited

Evolution of hydromagnetic turbulence from the electroweak phase transition

Axel Brandenburg, Tina Kahniashvili, Sayan Mandal +3

We present new simulations of decaying hydromagnetic turbulence for a relativistic equation of state relevant to the early universe. We compare helical and nonhelical cases either…