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Related papers: Jets and Gamma-Ray Burst Unification Schemes

200 papers

It is now generally accepted that long-duration gamma ray bursts (GRBs) are due to the collapse of massive rotating stars. The precise collapse process itself, however, is not yet fully understood. Strong winds, outbursts, and intense…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Robert A. Mesler , Daniel J. Whalen , Nicole M. Lloyd-Ronning , Chris L. Fryer , Ylva M. Pihlström

The X-ray light curves of hundreds of bursts are now available, thanks to the X-ray Telescope on board the Swift satellite, on time scales from ~1 minute up to weeks and in some cases months from the burst explosion. These data allow us to…

Astrophysics · Physics 2007-05-23 G. Tagliaferri

Gamma-ray bursts and their afterglows are thought to be produced by an ultra-relativistic jet. One of the most important open questions is the outflow composition: the energy may be carried out from the central source either as kinetic…

High Energy Astrophysical Phenomena · Physics 2016-06-22 Stefano Covino , Diego Gotz

Relativistic jets, or highly collimated and fast-moving outflows, are endemic to many astrophysical phenomena. The jets produced by gamma-ray bursts and tidal disruption events are accompanied by the accretion of material onto a black hole…

High Energy Astrophysical Phenomena · Physics 2020-10-07 Eric R. Coughlin , Mitchell C. Begelman

The energy release in gamma-ray bursts is one of the most interesting clues on the nature of their "inner engines". We show here that the total energy release in GRBs varies by less than one order of magnitude from one burst to another…

Astrophysics · Physics 2007-05-23 Tsvi Piran , Pawan Kumar , Alin Panaitescu , Luigi Piro

We consider gamma-ray burst (GRB) jets that are choked by extended material as sources of high-energy cosmic neutrinos. We take into account the jet propagation physics both inside the progenitor star and the surrounding dense medium.…

High Energy Astrophysical Phenomena · Physics 2018-10-12 Nicholas Senno , Kohta Murase , Peter Meszaros

The recent progress in the understanding the physical nature of neutron star equilibrium configurations and the first observational evidence of a genuinely short gamma-ray burst, GRB 090227B, allows to give an estimate of the gravitational…

High Energy Astrophysical Phenomena · Physics 2017-02-15 F. G. Oliveira , Jorge A. Rueda , Remo Ruffini

Gamma Ray Burst has been widely believed in last decade to be super-explosions: the Fireball. We are argue on the contrary that GRBs (as well as Soft Gamma Repeaters SGR) are precessing Gamma Jets. We remind the list of contradiction that…

Astrophysics · Physics 2014-10-13 Daniele Fargion

The cosmological gamma-ray burst (GRB) phenomenon is reviewed. The broad observational facts and empirical phenomenological relations of the GRB prompt emission and afterglow are outlined. A well-tested, successful fireball shock model is…

Astrophysics · Physics 2007-05-23 Bing Zhang , Peter Meszaros

Gamma-Ray Bursts (GRBs) are the strongest explosions in the Universe, which due to their extreme character likely involve some of the strongest magnetic fields in nature. This review discusses the possible roles of magnetic fields in GRBs,…

High Energy Astrophysical Phenomena · Physics 2016-08-08 Jonathan Granot , Tsvi Piran , Omer Bromberg , Judith L. Racusin , Frédéric Daigne

Striking similarities exist between high energy gamma ray emission from active galactic nuclei (AGN) and gamma ray bursts (GRBs). They suggest that GRBs are generated by inverse Compton scattering from highly relativistic electrons in…

Astrophysics · Physics 2009-10-22 Nir J. Shaviv , Arnon Dar

There is growing evidence that long and hard gamma-ray bursts (GRBs), discovered at redshifts between 0.4 and 3.4, are related to some type of supernova (SN) explosions. The GRB ejecta are ultra-relativistic, and possibly beamed. There is a…

Astrophysics · Physics 2007-05-23 Bohdan Paczynski

Gamma-ray bursts are the strongest explosions in the Universe since the Big Bang, believed to be produced either in forming black holes at the end of massive star evolution or merging of compact objects. Spectral and timing properties of…

Long gamma-ray bursts (GRBs) are believed to be related to the explosion of type Ic supernovae, which have been stripped of their hydrogen and helium envelopes. There appear to be two types of these explosions: those which are approximately…

Astrophysics · Physics 2009-11-10 B. Paczynski , P. Haensel

Highly relativistic jets from merger and accretion induced collapse of compact stellar objects, which may produce the cosmological gamma ray bursts (GRBs), are also very efficient and powerful cosmic ray accelerators. The expected…

Astrophysics · Physics 2007-05-23 Arnon Dar

Jet breaks in gamma ray burst (GRB) afterglows provide a direct probe of their collimation angle. Modeling a jet break requires an understanding of the "jet spreading" process, whereby the jet transitions from a collimated outflow into the…

High Energy Astrophysical Phenomena · Physics 2018-10-10 Paul C. Duffell , Tanmoy Laskar

Jet physics is again flourishing as a result of Chandra's ability to resolve high-energy emission from the radio-emitting structures of active galaxies and separate it from the X-ray-emitting thermal environments of the jets. These enhanced…

Astrophysics · Physics 2018-06-11 D. M. Worrall

Past years have brought an increasingly wider recognition of the ubiquity of relativistic outflows (jets) in galactic nuclei, which has turned jets into an effective tool for investigating the physics of nuclear regions in galaxies. A brief…

Astrophysics · Physics 2015-06-24 Andrei P. Lobanov , J. Anton Zensus

The central engine of gamma-ray bursts (GRBs) is believed to eject double-sided ultra-relativistic jets. For an observed GRB, one of the twin jets should point toward us, and is responsible for the prompt gamma-ray and subsequent afterglow…

Astrophysics · Physics 2009-11-10 Zhuo Li , Li-Ming Song

Gravitationally lensed Gamma-ray bursts (GRBs) offer critical advantages over other lensed sources. They can be detected via continuously operating detectors covering most of the sky. They offer extremely high time resolution to determine…

High Energy Astrophysical Phenomena · Physics 2025-03-27 A. J. Levan , B. P. Gompertz , G. P. Smith , M. E. Ravasio , G. P. Lamb , N. R. Tanvir
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