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Motivated by relativistic jets observed in active galactic nuclei (AGN), we simulate outflows of electron-positron pairs strongly coupled with photons from normal electron-proton plasmas. Using multi-fluid approximation and a Monte Carlo…

Astrophysics · Physics 2008-11-26 Katsuaki Asano , Fumio Takahara

We study steady and spherically symmetric outflows of pure electron-positron pair plasma as a possible acceleration mechanism of relativistic jets up to the bulk Lorentz factor of greater than 10. These outflows are initiated by the ``Wien…

Astrophysics · Physics 2009-11-10 S. Iwamoto , F. Takahara

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…

Astrophysics · Physics 2009-11-07 S. Iwamoto , F. Takahara

We present the first general relativistic hydrodynamic models of the launch and evolution of relativistic jets and winds, driven by thermal energy deposition, possibly due to neutrino-antineutrino annihilation, in the close vicinity of…

Astrophysics · Physics 2015-06-24 M. A. Aloy , H. -T. Janka , E. Mueller

On December 27, 2004, a giant flare from SGR 1806$-$20 was detected on earth. Its thermal spectrum and temperature suggest that the flare resulted from an energy release of about $10^{47}$ erg/sec close to the surface of a neutron star in…

Astrophysics · Physics 2009-11-10 Ehud Nakar , Tsvi Piran , Re'em Sari

The matter content of extragalactic relativistic jets is still an unsolved issue. There are strong arguments against pure electron-positron pair jets, but pairs could outnumber the electrons associated with protons by a factor 10-20. This…

High Energy Astrophysical Phenomena · Physics 2015-06-05 G. Ghisellini

The evolution of a dilute electron-positron fireball is calculated in the regime of strong magnetization and very high compactness (l ~10^3-10^8). Heating is applied at a low effective temperature (< 25 keV), and the fireball is allowed to…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Christopher Thompson , Ramandeep Gill

An X-ray short burst associated with a Galactic fast radio burst was observed in 2020, distinguished by its X-ray cut-off energy significantly exceeding that of other X-ray short bursts. X-ray photons of these short bursts are believed to…

High Energy Astrophysical Phenomena · Physics 2025-03-14 Tomoki Wada , Katsuaki Asano

The mass symmetry between the two species in electron-positron (pair) plasmas has interesting consequences for collisionless magnetic reconnection because the Hall term, which plays a crucial role in supporting fast reconnection in…

Astrophysics · Physics 2009-11-13 M. Swisdak , Y. H. Liu , J. F. Drake

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…

Astrophysics · Physics 2009-11-07 R. Schlickeiser , R. Vainio , M. Boettcher , I. Lerche , M. Pohl , C. Schuster

Sufficiently strong electric fields in plasmas can accelerate charged particles to relativistic energies. In this paper we describe the dynamics of positrons accelerated in such electric fields, and calculate the fraction of created…

Plasma Physics · Physics 2018-11-07 Ola Embréus , Linnea Hesslow , Mathias Hoppe , Gergely Papp , Katya Richards , Tünde Fülöp

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…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Lorenzo Sironi , Dimitrios Giannios

Radiation spectrum of extreme relativistic electrons and a probability of electron-positron pair production by energetic photons in a strong plasma wakefield are derived in the framework of a semiclassical approach. It is shown that that…

Plasma Physics · Physics 2009-11-13 E. Nerush , I. Kostyukov

We study relativistic magnetized outflows using relativistic equation of state having variable adiabatic index ($\Gamma$) and composition parameter $(\xi)$. We study the outflow in special relativistic magneto-hydrodynamic regime, from…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Kuldeep Singh , Indranil Chattopadhyay

We study the dynamics of relativistic electromagnetic explosions as a possible mechanism for the production of Gamma-Ray Bursts. We propose that a rotating relativistic stellar-mass progenitor loses much of its spin energy in the form of an…

Astrophysics · Physics 2007-05-23 Maxim Lyutikov , Roger Blandford

The expansion of a charge-neutral cloud of electrons and positrons with the temperature 1 MeV into an unmagnetized ambient plasma is examined with a 2D particle-in-cell (PIC) simulation. The pair outflow drives solitary waves in the ambient…

High Energy Astrophysical Phenomena · Physics 2018-08-01 ME Dieckmann , A Alejo , G Sarri

In this paper we model the emission from a relativistically expanding electron-positron pair plasma fireball originating near the surface of a heated neutron star. This pair fireball is deposited via the annihilation of neutrino pairs…

Astrophysics · Physics 2009-10-31 Jay D. Salmonson , James R. Wilson , Grant J. Mathews

The expansion dynamics of hot electron-positron-photon plasma droplets is dealt with within relativistic hydrodynamics. Such droplets, envisaged to be created in future experiments by irradiating thin foils with counter-propagating…

Plasma Physics · Physics 2011-04-07 R. Yaresko , Munshi G. Mustafa , B. Kampfer

Previously, we showed that, owing to effects arising from quantum electrodynamics (QED), magnetohydrodynamic fast modes of sufficient strength will break down to form electron-positron pairs while traversing the magnetospheres of strongly…

Astrophysics · Physics 2009-11-10 Jeremy S. Heyl , Lars Hernquist

We investigate a scenario of photons scattering by electrons within a relativistic outflow. The outflow is composed of discrete shells with different speeds. One shell emits radiation for a short duration. Some of this radiation is…

Astrophysics · Physics 2014-03-11 R. -F. Shen , R. Barniol Duran , P. Kumar
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