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We study the role of the quasi-linear diffusion (QLD) in producing X-ray emission by means of ultra-relativistic electrons in AGN magnetospheric flows. We examined two regions: (a) an area close to the black hole and (b) the outer…

High Energy Astrophysical Phenomena · Physics 2016-11-25 Z. Osmanov , G. Machabeli

Quasi-linear diffusion (QLD), driven by the cyclotron instability, is proposed as a mechanism for the possible generation of synchrotron emission in the nearby zone of SgrA$^*$. For physically reasonable parameters, the QLD, by causing…

High Energy Astrophysical Phenomena · Physics 2021-04-01 G. Gogaberishvili , Z. N. Osmanov , S. M. Mahajan

In order to understand the role of the synchrotron emission in the high energy gamma-ray flares from PKS 1510-089, we study generation of the synchrotron emission by means of the feedback of cyclotron waves on the particle distribution via…

Astrophysics of Galaxies · Physics 2022-01-14 Z. N. Osmanov

For active galactic nuclei (AGNs) we study the role of the mechanism of quasi-linear diffusion (QLD) in producing the high energy emission in the MeV-GeV domains strongly connected with the submillimeter/infrared radiation. Considering the…

High Energy Astrophysical Phenomena · Physics 2010-12-17 Z. Osmanov

We consider relativistic electrons in magnetospheric flows close to a supermassive black hole and study the mechanism of quasi-linear diffusion (QLD) to investigate the correlation between $\gamma$-ray and radio emission in active galactic…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Z. Osmanov

In this, paper we study the possibility of generation of electromagnetic waves in the magnetospheres of radio magnetars by means of the quasi-linear diffusion (QLD). Considering the magnetosphere composed of the so-called beam and the…

Solar and Stellar Astrophysics · Physics 2015-06-22 Zaza Osmanov

In the present paper we study the possibility of a simultaneous generation of radio waves and soft $X$-rays by means of the quasi-linear diffusion (QLD) in the anomalous pulsar AXP 4U 0142+61. Considering the magnetosphere composed of the…

High Energy Astrophysical Phenomena · Physics 2021-08-24 Z. N. Osmanov

Emission of a charged particle propagating in a medium with a curved magnetic field is reconsidered stressing the analogy between this emission mechanism and collective Cherenkov-type plasma emission. It is explained how this mechanism…

Astrophysics · Physics 2016-08-30 Maxim Lyutikov , George Machabeli , Roger Blandford

Electromagnetic processes associated with a charged particle moving in a strong circular magnetic field is considered in cylindrical coordinates. We investigate the relation between the vacuum curvature emission and Cherenkov emission and…

Astrophysics · Physics 2009-10-30 Maxim Lyutikov , George Machabeli , Roger Blandford

A theory of pulsar radio emission generation, in which the observed waves are produced directly by maser-type plasma instabilities operating at the anomalous cyclotron-Cherenkov resonance $\omega- k_{\parallel} v_{\parallel} + \omega_B/…

Astrophysics · Physics 2009-10-30 Maxim Lyutikov , Roger D. Blandford , George Machabeli

We examine linear and quasi-liner stages of Cherenkov-drift instability in the relativistic magnetized electron-positron plasma. The external magnetic field lines are assumed to be slightly curved. In this case the curvature drift of…

Astrophysics · Physics 2007-05-23 David Shapakidze , George Machabeli , George Melikidze , David Khechinashvili

For Crab-like pulsars we consider the synchrotron mechanism influenced by relativistic effects of rotation to study the production of the very high energy (VHE) pulsed radiation. The process of quasi-linear diffusion (QLD) is applied to…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Z. Osmanov

Electrons traveling along magnetic field lines from Jupiter to Io, driven by quasi-linear diffusion (QLD), emit synchrotron radiation. By using the small angle approximation, the kinematic equation for the particle distribution gives us the…

High Energy Astrophysical Phenomena · Physics 2023-12-05 Akaki Chkhaidze , Erekle Kalichava

Both radiative and mechanical feedback from Active Galactic Nuclei have been found to be important for the evolution of elliptical galaxies. We compute how a shock may be driven from a central black hole into the gaseous envelope of an…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Y. -F. Jiang , L. Ciotti , J. P. Ostriker , A. Spitkovsky

In the present paper we construct a self-consistent theory, interpreting the observational properties of RBS1774. It is well known that the distribution function of relativistic particles is one-dimensional at the pulsar surface. However,…

Solar and Stellar Astrophysics · Physics 2015-05-20 Nino Chkheidze

Emission process of a charged particle propagating in a medium with a curved magnetic field is considered. This mechanism combines features of conventional Cherenkov and curvature emission. Thus, presence of a medium with the index of…

High Energy Astrophysical Phenomena · Physics 2015-06-22 George Machabeli , Nino Chkheidze

Non-thermal X-ray emission in some supernova remnants originates from synchrotron radiation of ultra-relativistic particles in turbulent magnetic fields. We address the effect of a random magnetic field on synchrotron emission images and…

Astrophysics · Physics 2011-02-22 Andrei M. Bykov , Yury A. Uvarov , Donald C. Ellison

A quasiclassical theory of the synchrotron-like gluon emission is discussed. We show that the synchrotron emission may be important in the jet quenching if the plasma instabilities generate a chromomagnetic field about $m^{2}_{D}/g$. Our…

High Energy Physics - Phenomenology · Physics 2009-07-16 B. G. Zakharov

We have theoretically shown that the yield of diffuse radiation generated by relativistic electrons passing random multilayered systems can be increased when a resonant condition is met. Resonant condition can be satisfied for the…

Accelerator Physics · Physics 2009-11-11 Zh. S. Gevorkian , J. Verhoeven

When ultrafast noncritical cascaded second-harmonic generation of energetic femtosecond pulses occur in a bulk lithium niobate crystal optical Cherenkov waves are formed in the near- to mid-IR. Numerical simulations show that the few-cycle…

Optics · Physics 2011-10-27 M. Bache , O. Bang , B. B. Zhou , J. Moses , F. W. Wise
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