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相关论文: Relativistic Precessing Jets and Cosmological Gamm…

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In the collapsar scenario, gamma ray bursts are caused by relativistic jets expelled along the rotation axis of a collapsing stellar core. We discuss how the structure and time-dependence of such jets depends on the stellar envelope and…

天体物理学 · 物理学 2009-11-06 P. Meszaros , M. J. Rees

New two- and three-dimensional calculations are presented of relativistic jet propagation and break out in massive Wolf-Rayet stars. Such jets are thought responsible for gamma-ray bursts. As it erupts, the jet is surrounded by a cocoon of…

天体物理学 · 物理学 2009-11-10 Weiqun Zhang , S. E. Woosley , A. Heger

Gamma-ray bursts (GRB) are short and intense bursts of $\sim$100 keV$-$1MeV photons, usually followed by long-lasting decaying afterglow emission in a wide range of electromagnetic wavelengths from radio to X-ray and, sometimes, even to GeV…

高能天体物理现象 · 物理学 2023-04-05 Yun-Wei Yu , He Gao , Fa-Yin Wang , Bin-Bin Zhang

There are several lines of evidence indicating that the ultra-relativistic outflows powering gamma-ray bursts (GRBs) are collimated into narrow jets. However, these are indirect, and the jet structure is rather poorly constrained. What is…

高能天体物理现象 · 物理学 2010-12-24 Jonathan Granot , Enrico Ramirez-Ruiz

The observational diversity of ``gamma-ray bursts'' (GRBs) has been increasing, and the natural inclination is a proliferation of models. We explore the possibility that at least part of this diversity is a consequence of a single basic…

天体物理学 · 物理学 2008-11-26 S. E. Woosley , Weiqun Zhang

After many years of speculation, recent observations have confirmed the association of gamma-ray bursts with core-collapse supernova explosions from massive stars. This association carries with it important consequences. The burst…

天体物理学 · 物理学 2007-05-23 D. Lazzati , M. Begelman , G. Ghirlanda , G. Ghisellini , C. Firmani

We propose that gamma-ray burst pulses are produced when highly-relativistic jets sweep across an observer's line-of-sight. We hypothesize that axisymmetric jet profiles, coupled with special relativistic effects, produce the time-reversed…

高能天体物理现象 · 物理学 2024-03-19 Jon Hakkila , Geoffrey N. Pendleton , Robert D. Preece , Timothy W. Giblin

A phenomenological model is presented to explain the light curves of gamma-ray bursts. Gamma-rays are produced in a narrow beam which sweeps through space due to the precession of a slaved accretion disc. The light curve expected from such…

天体物理学 · 物理学 2009-10-31 Simon Portegies Zwart

Growing observational evidence supports the proposition that gamma-ray bursts (GRBs) are powered by relativistic jets from massive helium stars whose cores have collapsed to black holes and an accretion disk (collapsars). We model the…

天体物理学 · 物理学 2007-05-23 Weiqun Zhang , S. E. Woosley

We propose that gamma ray bursts (GRBs) are produced by a shower of heavy blobs running into circumstellar material at highly relativistic speeds. The gamma ray emission is produced in the shocks these bullets drive into the surrounding…

天体物理学 · 物理学 2009-10-31 S. Heinz , M. C. Begelman

If gamma ray bursts are highly collimated, the energy requirements of each event may be reduced by several (~ 4-6) orders of magnitude, and the event rate increased correspondingly. Extreme conditions in gamma ray bursters lead to highly…

天体物理学 · 物理学 2009-10-30 James E. Rhoads

According to the collapsar model, gamma-ray bursts are thought to be produced in shocks that occur after the relativistic jet has broken free from the stellar envelope. If the mass density of the collimated outflow is less than that of the…

天体物理学 · 物理学 2009-11-07 Enrico Ramirez-Ruiz , Annalisa Celotti , Martin J. Rees

The relativistic outflows from gamma-ray bursts are now thought to be narrowly collimated into jets. After correcting for this jet geometry there is a remarkable constancy of both the energy radiated by the burst and the kinetic energy…

天体物理学 · 物理学 2009-11-10 D. A. Frail

In almost any scenario for 'cosmological' gamma-ray bursts (and in many models where they originate in our own Galaxy), the initial energy density is so large that the resulting relativistic plasma expands with $v\sim c$ producing a blast…

天体物理学 · 物理学 2009-10-22 P. Meszaros , M. J. Rees

We present an internal shock model with external characteristics for explaining the complicated light curves of gamma-ray bursts. Shocks produce gamma-rays in the interaction between a precessing beam of relativistic particles and the…

天体物理学 · 物理学 2009-10-31 Simon Portegies Zwart , Tomonori Totani

We provide a comprehensive review of major developments in our understanding of gamma-ray bursts, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered. We describe the…

高能天体物理现象 · 物理学 2015-06-03 Pawan Kumar , Bing Zhang

Cosmological GRBs are discussed with an emphasis on their plausible connection with black holes. GRBs can be triggered by collapse of stellar-mass objects that leads to formation of a black hole and a transient debris disk with a huge…

天体物理学 · 物理学 2008-11-26 Andrei M. Beloborodov

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced in star formation regions in distant galaxies by highly relativistic jets that happen to point in our direction. Relativistic beaming collimates the…

天体物理学 · 物理学 2007-05-23 Arnon Dar

It is generally believed that cosmological Gamma Ray Bursts (GRBs) are produced by the deceleration of relativistic objects with Lorentz factor (Gamma) >~ 100. We study the possibility that some GRBs are produced along with relativistic…

天体物理学 · 物理学 2016-08-30 Hideyuki Umeda

Jets in long-duration $\gamma$-ray bursts (GRBs) have to drill through the collapsing star in order to break out of it and produce the $\gamma$-ray signal while the central engine is still active. If the breakout time is shorter for more…

高能天体物理现象 · 物理学 2017-10-11 Maria Petropoulou , Rodolfo Barniol Duran , Dimitrios Giannios
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