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相关论文: Transrelativistic pair plasmas in AGN jets

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As powerful gamma-ray engines, blazars -- relativistic plasma jets launched toward Earth from active galactic nuclei -- are manifestly high-energy particle accelerators. Yet, exactly how these jets accelerate particles as well as what they…

高能天体物理现象 · 物理学 2025-04-03 John Mehlhaff , Muni Zhou , Vladimir Zhdankin

The evolution of the particle distribution functions inside a relativistic jet containing an e^-e^+ pair plasma and of the resulting $\gamma$-ray and X-ray spectra is investigated. The first phase of this evolution is governed by heavy…

天体物理学 · 物理学 2008-02-03 M. Boettcher , H. Mause , R. Schlickeiser

The contribution of the pair annihilation process in relativistic electron-positron jets to the gamma-ray emission of blazars is calculated. Under the same assumptions as for the calculation of the yield of inverse Compton scattered…

天体物理学 · 物理学 2011-05-23 M. Boettcher , R. Schlickeiser

It is generally accepted that relativistic jet outflows power the nonthermal emission from active galactic nuclei (AGN). The composition of these jets -- leptonic versus hadronic -- is still under debate. We investigate the microphysical…

天体物理学 · 物理学 2009-11-07 R. Schlickeiser , R. Vainio , M. Boettcher , I. Lerche , M. Pohl , C. Schuster

Relativistic jets of plasma are a key ingredient of many types of Active Galactic Nuclei (AGN). Today we know that AGNs are powered by the accretion of inter stellar material into the gravitational field of a Super Massive Black Hole and…

Assuming that the enhanced MeV emission from the MeV blazar PKS 0208-512 observed by COMPTEL on occasions is due to annihilation in a pair plasma, we estimate parameters of the annihilation region: its size, the number density of particles,…

天体物理学 · 物理学 2007-05-23 I. V. Moskalenko , W. Collmar

X-ray emission from large scale extragalactic jets is likely to be due to inverse Compton scattering of relativistic particles off seed photons of both the cosmic microwave background field and the blazar nucleus. The first process…

天体物理学 · 物理学 2009-10-31 A. Celotti , G. Ghisellini , M. Chiaberge

The interaction of TeV photons from blazars with the extragalactic background light produces a relativistic beam of electron-positron pairs streaming through the intergalactic medium (IGM). The fate of the beam energy is uncertain. By means…

高能天体物理现象 · 物理学 2015-06-18 Lorenzo Sironi , Dimitrios Giannios

Broadband emission from relativistic outflows (jets) of active galactic nuclei (AGN) and gamma-ray bursts (GRBs) contains valuable information about the nature of the jet itself, and about the central engine which launches it. Using special…

高能天体物理现象 · 物理学 2015-06-12 Petar Mimica , Miguel Angel Aloy , Jesus M. Rueda-Becerril , Siham Tabik , Carmen Aloy

We have developed a model for gamma ray emission in jets of active galactic nuclei in which particle acceleration takes place at a shock in the relativistic jet plasma due to a massive star in the central region of the host galaxy moving…

天体物理学 · 物理学 2016-06-08 W. Bednarek , R. J. Protheroe

The photon spectrum emitted by a transrelativistic pair plasma is calculated in the presence of an ultrastrong magnetic field, and is shown to bear a remarkable resemblance to the rising hard X-ray spectra of quiescent magnetars. This…

高能天体物理现象 · 物理学 2020-12-09 Christopher Thompson , Alexander Kostenko

A recent progress in the study of $\gamma$-ray jets is reviewed, with a focus on some theoretical interpretations of the VHE emission from M87, and possibly other misaligned blazars; the connection betwe en the GeV breaks exhibited by…

高能天体物理现象 · 物理学 2015-05-20 Amir Levinson

Relativistic jets are one of the most powerful manifestations of the release of energy produced around supermassive black holes at the centre of active galactic nuclei (AGN). Their emission is observed across the entire electromagnetic…

高能天体物理现象 · 物理学 2015-06-17 M. Orienti , F. D'Ammando , M. Giroletti , D. Dallacasa , T. Venturi , G. Giovannini

(abridged) Relativistic jets, formed in the vicinity of central supermassive black holes in AGN, show ample evidence connecting them to physical conditions in the accretion disc and broad-line region. The jets are responsible for a large…

宇宙学与河外天体物理 · 物理学 2010-10-15 Andrei Lobanov

The propagation of a relativistic electron-positron beam in a magnetized electron-ion plasma is studied, focusing on the polarization of the radiation generated in this case. Special emphasis is laid on investigating the polarization of the…

等离子体物理 · 物理学 2020-06-11 Ujjwal Sinha , Naveen Kumar

The radiation we observe from blazars is most likely the product of the transformation of bulk kinetic energy into random energy. This process must have a relatively small efficiency (e.g. 10%) if jets are to power the extended…

天体物理学 · 物理学 2009-10-31 G. Ghisellini

Relativistic jets are one of the most powerful manifestations of the release of energy related to the supermassive black holes at the centre of active galactic nuclei (AGN). Their emission is observed across the entire electromagnetic…

高能天体物理现象 · 物理学 2015-04-14 M. Orienti

We investigate a novel mechanism of bulk acceleration for relativistic jets of pure electron-positron pair plasma.We assumed that relativistically hot plasma is optically thick for Compton scattering and then pair plasma coupled dynamically…

天体物理学 · 物理学 2009-11-07 S. Iwamoto , F. Takahara

It is commonly believed that blazar jets are relativistic magnetized plasma outflows from supermassive black holes. One key question is how the jets dissipate magnetic energy to accelerate particles and drive powerful multi-wavelength…

高能天体物理现象 · 物理学 2022-01-26 Haocheng Zhang , Xiaocan Li , Dimitrios Giannios , Fan Guo , Hannes Thiersen , Markus Böttcher , Tiffany Lewis , Tonia Venters

We study the effect of non-relativistic, thermal matter in the jets of active galaxies (AGN) on the low-frequency non-thermal emission and the variability thereof. In matter-dominated jets, sizable quantities of gas should exist, in…

天体物理学 · 物理学 2009-11-10 M. Siewert , M. Pohl , R. Schlickeiser
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