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Relativistic outflows in the form of jets are common in many astrophysical objects. By their very nature, jets have angle dependent velocity profiles, Gamma = Gamma(r, theta, phi), where Gamma is the outflow Lorentz factor. In this work we…

高能天体物理现象 · 物理学 2015-06-11 Christoffer Lundman , Asaf Pe'er , Felix Ryde

We explore the spectral and polarization properties of photospheric emissions from stratified jets in which multiple components, separated by a sharp velocity shear regions, are distributed in lateral direction. Propagation of thermal…

高能天体物理现象 · 物理学 2015-06-19 Hirotaka Ito , Shigehiro Nagataki , Jin Matsumoto , Shiu-Hang Lee , Alexey Tolstov , Jirong Mao , Maria Dainotti , Akira Mizuta

Despite being hard to measure, GRB prompt $\gamma$-ray emission polarization is a valuable probe of the dominant emission mechanism and the outflow's composition and angular structure. During the prompt emission the outflow is…

高能天体物理现象 · 物理学 2020-01-08 Ramandeep Gill , Jonathan Granot , Pawan Kumar

(Abridged) We consider the polarization properties of optically thin synchrotron radiation emitted by relativistically moving electron--positron jets carrying large-scale helical magnetic fields. In our model, the jet is cylindrical, and…

天体物理学 · 物理学 2009-11-10 Maxim Lyutikov , Vladimir I. Pariev , Denise C. Gabuzda

We explore the properties of photospheric emission in the context of long gamma-ray bursts (LGRBs) using three numerical models that combine relativistic hydrodynamical simulations and Monte Carlo radiation transfer calculations in three…

高能天体物理现象 · 物理学 2023-07-20 Hirotaka Ito , Jin Matsumoto , Shigehiro Nagataki , Donald C. Warren , Maxim V. Barkov , Daisuke Yonetoku

We study the polarization properties of relativistic reconfinement shocks with chaotic magnetic fields. Using our hydrodynamical model of their structure, we calculate synthetic polarization maps, longitudinal polarization profiles and…

星系天体物理 · 物理学 2009-11-13 Krzysztof Nalewajko

The MeV spectral peak of gamma-ray bursts (GRBs) is best explained as photospheric emission from a dissipative relativistic jet. The observed non-blackbody spectrum shows that sub-photospheric dissipation involves both thermal plasma…

高能天体物理现象 · 物理学 2016-11-07 Christoffer Lundman , Indrek Vurm , Andrei M. Beloborodov

We review the physics of GRB production by relativistic jets that start highly opaque near the central source and then expand to transparency. We discuss dissipative and radiative processes in the jet and how radiative transfer shapes the…

高能天体物理现象 · 物理学 2017-04-05 A. M. Beloborodov , P. Mészáros

{\it Fermi Gamma-ray Space Telescope} observations of GRB110721A have revealed two emission components from the relativistic jet: emission from the photosphere, peaking at $\sim 100$ keV and a non-thermal component, which peaks at $\sim…

In this study, the light curves and spectrum of the photospheric thermal radiation from ultrarelativistic gamma-ray burst (GRB) jets are calculated using 2D relativistic hydrodynamic simulations of jets from a collapsar. As the jet…

高能天体物理现象 · 物理学 2011-04-13 Akira Mizuta , Shigehiro Nagataki , Junichi Aoi

Propagation of photons in relativistically expanding plasma outflows, characterized by steady Lorentz factor Gamma is considered. Photons that are injected in regions of high optical depth are advected with the flow until they escape at the…

天体物理学 · 物理学 2009-11-13 Asaf Pe'er

We explore photospheric emissions from stratified two-component jets, wherein a highly relativistic spine outflow is surrounded by a wider and less relativistic sheath outflow. Thermal photons are injected in regions of high optical depth…

The polarimetric measurement on the prompt phase of GRB 100826A shows that the polarization angle changes $\sim 90^{\circ}$ between two adjacent time intervals. We will show that this phenomenon can be naturally interpreted in the framework…

高能天体物理现象 · 物理学 2014-11-07 Zhe Chang , Hai-Nan Lin

We investigate the polarization and proper motion expected in a beamed Gamma-Ray Burst's ejecta. We find that even if the magnetic field has well defined orientation relative to the direction of motion of the shock, the polarization is not…

天体物理学 · 物理学 2009-10-31 Re'em Sari

A high energy power law is a common feature in the spectra of many astrophysical objects. We show that the photons in a relativistic plasma with a variable Lorentz factor go through repeated scattering with electrons to gain energy. The…

高能天体物理现象 · 物理学 2023-02-01 Mukesh K. Vyas , Asaf Pe'er

We present an overview of new HST imaging polarimetry of six nearby radio galaxies with optical jets. These observations triple the number of extragalactic jets with subarcsecond-resolution optical polarimetry. We discuss the polarization…

The low energy spectral slopes of the prompt emission of most gamma-ray bursts (GRBs) are difficult to reconcile with radiatively efficient optically thin emission models irrespective of the radiation mechanism. An alternative is to ascribe…

高能天体物理现象 · 物理学 2015-06-11 Indrek Vurm , Yuri Lyubarsky , Tsvi Piran

It has been observed that photons in the prompt emission of some gamma-ray bursts (GRBs) are highly polarized. The high polarization is used by some authors to give a strict constraint on the Lorentz invariance violation (LIV). If the…

高能物理 - 唯象学 · 物理学 2016-10-11 Hai-Nan Lin , Xin Li , Zhe Chang

Blazars are thought to possess a relativistic jet that is pointing toward the direction of the Earth and the elect of relativistic beaming enhances its apparent brightness. They radiate in all wavebands from the radio to the gamma-ray bands…

Linear polarization at the level of $\sim 1-3%$ has by now been measured in several gamma-ray burst afterglows. Whereas the degree of polarization, $P$, was found to vary in some sources, the position angle, $\theta_p$, was roughly constant…

天体物理学 · 物理学 2009-11-07 Jonathan Granot , Arieh Konigl
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