activity
19962018
most citedCherenkov-Curvature Radiation and Pulsar Radio Emission Generation

56 citations · 191 across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2018★ 2 cited

Self-trapping as the possible beaming mechanism for FRB

George Machabeli, Andria Rogava, Beka Tevdorashvili

Mysterious Fast Radio Bursts (FRB), still eluding a rational explanation, are astronomical radio flashes with durations of milliseconds. They are thought to be of an extragalactic…

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…

astro-ph.HE2016

Emission of extremely bright gamma-ray pulsar in the Large Magellanic Cloud

George Machabeli, Andria Rogava, Nino Chkheidze

In the present paper a theoretical interpretation of observational characteristics of the pulsar PSR J0540-6919 is suggested. In particular, we provide a theoretical model explaini…

astro-ph.HE2015

Millisecond newly born pulsars as efficient accelerators of electrons

Z. Osmanov, S. Mahajan, G. Machabeli +1

The newly born millisecond pulsars are investigated as possible energy sources for creating ultra-high energy electrons. The transfer of energy from the star rotation to high energ…

astro-ph.HE2015

On the origin and physics of Gamma Flares in Crab Nebula

George Machabeli, Andria Rogava, David Shapakidze

We consider parametric generation of electrostatic waves in the magnetosphere of the pulsar PSR0531. It is shown that in the framework of this mechanism it is possible to convert t…

astro-ph.HE2014★ 26 cited

Extremely efficient Zevatron in rotating AGN magnetospheres

Zaza Osmanov, Swadesh Mahajan, George Machabeli +1

A novel model of particle acceleration in the magnetospheres of rotating active galactic nuclei (AGN) is constructed.The particle energies may be boosted up to eV in a two…