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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…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Ramandeep Gill , Jonathan Granot , Pawan Kumar

The possible short gamma-ray burst (GRB) observed by {\it Fermi}/GBM in coincidence with the first gravitational wave (GW) detection, offers new ways to test GRB prompt emission models. Gravitational wave observations provide previously…

High Energy Astrophysical Phenomena · Physics 2016-08-31 P. Veres , R. D. Preece , A. Goldstein , P. Mészáros , E. Burns , V. Connaughton

Among the models used to explain the prompt emission of gamma-ray bursts (GRBs), internal shocks is a leading one. Its most basic ingredient is a collision between two cold shells of different Lorentz factors in an ultra-relativistic…

High Energy Astrophysical Phenomena · Physics 2025-07-09 A. Charlet , J. Granot , P. Beniamini

There is no complete description of the emission physics during the prompt phase in gamma-ray bursts. Spectral analyses, however, indicate that many spectra are narrower than what is expected for non-thermal emission models. Here, we…

High Energy Astrophysical Phenomena · Physics 2020-05-06 Zeynep Acuner , Felix Ryde , Asaf Pe'er , Daniel Mortlock , Björn Ahlgren

Forward shocks caused by the interaction between a relativistic blast wave and the circum-burst medium are thought to be responsible for the afterglow emission in Gamma-Ray Bursts (GRBs). We consider the hydrodynamics of a spherical…

High Energy Astrophysical Phenomena · Physics 2015-06-12 L. Nava , L. Sironi , G. Ghisellini , A. Celotti , G. Ghirlanda

Gamma-ray burst (GRB) engines are probed most intimately during the prompt gamma-ray luminous phase when the expanding blast wave is closest to the explosion center. Using GRBs 990123 and 940217 as guides, we briefly review observations of…

Astrophysics · Physics 2009-10-31 Charles D. Dermer , James Chiang

We perform simulations in a simple model that aims to mimic the hydrodynamic evolution of a relativistic fluid during a cosmological first-order phase transitions. The observable we are concerned with is hereby the spectrum of gravitational…

Cosmology and Nongalactic Astrophysics · Physics 2018-08-21 Thomas Konstandin

Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRBs) is obtained from few plausible assumptions consistent with observations. Model-independent requirements posed by these assumptions on the…

Astrophysics · Physics 2009-10-31 E. V. Derishev , V. V. Kocharovsky , Vl. V. Kocharovsky

The emission rate of photons from a hot, weakly coupled ultrarelativistic plasma is analyzed. Leading-log results, reflecting the sensitivity of the emission rate to scattering events with momentum transfers from $gT$ to $T$, have…

High Energy Physics - Phenomenology · Physics 2010-02-03 Peter Arnold , Guy D. Moore , Laurence G. Yaffe

We present calculations of the time evolution of the prompt spectra of gamma-ray burst models involving generic internal dissipation regions, including internal shocks, either by itself or in the presence of an external photon source such…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Katsuaki Asano , Peter Meszaros

The diffuse Galactic gamma-ray emission is produced by cosmic rays (CRs) interacting with the interstellar gas and radiation field. Measurements by the Energetic Gamma-Ray Experiment Telescope (EGRET) instrument on the Compton Gamma-Ray…

High Energy Astrophysical Phenomena · Physics 2010-04-23 LAT Collaboration

We consider the formation of photon spectrum at the photosphere of ultrarelativistically expanding outflow. We use the Fokker-Planck approximation to the Boltzmann equation, and obtain the generalized Kompaneets equation which takes into…

High Energy Astrophysical Phenomena · Physics 2013-11-05 A. G. Aksenov , R. Ruffini , G. V. Vereshchagin

We report on observations of correlated behavior between the prompt gamma-ray and optical emission from GRB 080319B, which confirm that (i) they occurred within the same astrophysical source region and (ii) their respective radiation…

The bright long gamma-ray burst GRB 141207A was observed by the {\it Fermi Gamma-ray Space Telescope} and detected by both instruments onboard. The observations show that the spectrum in the prompt phase is not well described by the…

High Energy Astrophysical Phenomena · Physics 2016-12-21 Makoto Arimoto , Katsuaki Asano , Masanori Ohno , Péter Veres , Magnus Axelsson , Elisabetta Bissaldi , Yutaro Tachibana , Nobuyuki Kawai

We discuss the preliminary results of spectral analysis simulations involving anticipated correlated multi-wavelength observations of gamma-ray bursts (GRBs) using Swift's Burst Alert Telescope (BAT) and the Gamma-Ray Large Area Space…

Astrophysics · Physics 2009-11-13 Michael Stamatikos , Takanori Sakamoto , David L. Band

We describe preliminary results of a global model of the radiatively-driven photoionized wind and accretion flow of the high-mass X-ray binary Vela X-1. The full model combines FLASH hydrodynamic calculations, XSTAR photoionization…

Astrophysics · Physics 2009-06-23 Christopher W. Mauche , Duane A. Liedahl , Shizuka Akiyama , Tomasz Plewa

Collapsars may be a source for the long Gamma Ray Bursts (GRBs) in the BATSE catalog. Collapsars may radiate gamma rays anisotropically by beamed jet emission close to the observer's line of sight. These jets must penetrate the…

Astrophysics · Physics 2007-05-23 E. A. Gomez , P. E. Hardee

Blazars are known to emit a broad band emission from radio to gamma-rays with rapid time variations, particularly, in X- and gamma-rays. Synchrotron radiation and inverse Compton scattering are thought to play an important role in emission…

Astrophysics · Physics 2009-10-31 M. Kusunose , F. Takahara , H. Li

We investigate the dynamics and radiation from a relativistic blast-wave which decelerates as it sweeps up ambient matter. The bulk kinetic energy of the blast-wave shell is converted into internal energy by the process of accreting…

Astrophysics · Physics 2016-08-30 J. Chiang , C. D. Dermer

Unsteady activity of gamma-ray burst sources leads to internal shocks in their emergent relativistic wind. We study the emission spectra from such shocks, assuming that they produce a power-law distribution of relativistic electrons and…

Astrophysics · Physics 2009-10-30 Ravi Pilla , Abraham Loeb
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