activity
20042021
most citedThe Spectrum of Gravitational Radiation from Primordial Turbulence

219 citations · 886 across the 29 of their papers we have counts for

collaborators

29 papers

gr-qc2021★ 21 cited

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.CO2020★ 41 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.HE2017

Generation of nanoflares in the Crab pulsar

G. Machabeli, I. Malov, G. Gogoberidze

We study dynamics of drift waves in the pair plasma of pulsar magnetosphere. It is shown that nonlinear of the drift waves with plasma particles leads to the formation of small sca…

physics.space-ph2016

Imbalanced magnetohydrodynamic turbulence modified by velocity shear in the solar wind

Grigol Gogoberidze, Yuriy Voitenko

We study incompressible imbalanced magnetohydrodynamic turbulence in the presence of background velocity shears. Using scaling arguments, we show that the turbulent cascade is sign…

astro-ph.SR2013★ 12 cited

Electrostatic plasma instabilities driven by neutral gas flows in the solar chromosphere

G. Gogoberidze, Y. Voitenko, S. Poedts +1

We investigate electrostatic plasma instabilities of Farley-Buneman (FB) type driven by quasi-stationary neutral gas flows in the solar chromosphere. The role of these instabilitie…

astro-ph.SR2013★ 21 cited

Yaglom law in the expanding solar wind

G. Gogoberidze, S. Perri, V. Carbone

We study the Yaglom law, which relates the mixed third order structure function to the average dissipation rate of turbulence, in a uniformly expanding solar wind by using the two…