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Related papers: A Possible Model for the Supernova/Gamma-Ray Burst…

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We present a new model for gamma-ray bursts (GRBs) that are not only associated with supernovae but also have small baryon contamination. In this model, we assume a newborn neutron star to move outward at a kick velocity of $\sim 10^3 {\rm…

Astrophysics · Physics 2007-05-23 K. S. Cheng , Z. G. Dai

It is known that Neutron Stars may be converted into more compact Strange Stars (SS) on capture/formation of a ``seed'' of strange matter. It is also known that the binding energy of the nascent hot SS is likely to be radiated as $\nu…

Astrophysics · Physics 2007-05-23 Abhas Mitra

There are about 2000 gamma ray burst (GRB) events known to us with data pouring in at the rate of one per day. While the afterglows of GRBs in radio, optical and X-ray bands are successfully explained by the fireball model, a significant…

Astrophysics · Physics 2007-05-23 Jishnu Dey , Subharthi Ray , Xiang-Dong Li , Mira Dey , Ignazio Bombaci

We discuss the possible connection between supernova explosions (SN) and gamma-ray bursters (GRB) from the perspective of our current understanding of SN physics. Recent evidence strongly suggests that the explosion mechanism of core…

Astrophysics · Physics 2009-09-25 P. Hoeflich , A. Khokhlov , S. Rosswog , L. Wang

We present a scenario of formation of strange stars due to spin-down of {\it rapidly rotating} neutron stars left after supernova explosions . By assuming a process where the total baryon mass is conserved but the angular momentum is lost…

Astrophysics · Physics 2009-11-10 Nobutoshi Yasutake , Masa-aki Hashimoto , Yoshiharu Eriguchi

In these proceedings, I discuss recent progress in understanding the nature of cosmic gamma-ray bursts (GRB), with the focus on the apparent relation of several GRBs with an energetic subclass of stellar explosions, type Ib/c core-collapse…

Astrophysics · Physics 2007-05-23 K. A. Postnov

Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously with core-collapse supernovae (SNe), thus linking by a common thread nature's two grandest explosions. We review here the growing evidence for and…

Astrophysics · Physics 2008-11-26 S. E. Woosley , J. S. Bloom

We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ray bursts. We use different recent models for the equation of state of neutron star matter and strange quark matter. We show that the total…

Astrophysics · Physics 2009-10-31 Ignazio Bombaci , Bhaskar Datta

We here discuss a new model of $\gamma$-ray bursts (GRBs) based on differentially rotating strange stars. Strange stars in this model and differentially rotating neutron stars in the Klu\'zniak-Ruderman model can produce extremely…

Astrophysics · Physics 2008-11-26 Z. G. Dai , T. Lu

A long-duration gamma-ray burst (GRB) marks the violent end of a massive star. GRBs are rare in the universe, and their progenitor stars are thought to possess unique physical properties such as low metal content and rapid rotation, while…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Z. Cano

A scenario is proposed that explains both the observed high pulsar velocities and extragalactic gamma-ray bursts (GRBs). The model involves an ultra- relativistic jet from a supernova (SN), that produces a GRB and its afterglow, whose…

Astrophysics · Physics 2009-10-30 Renyue Cen

Some gamma ray bursts may be produced by supernovae exploding in close massive binary systems (type Ib/c supernovae) as suggested by the recent observation of SN 1998bw/GRB 980425. We propose that high energy radiation observed in such…

Astrophysics · Physics 2007-05-23 R. J. Protheroe , W. Bednarek

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly relativistic jets emitted in core collapse supernova explosions (SNe). The result of the event, probably, is not just a compact object plus…

Astrophysics · Physics 2009-11-06 Arnon Dar

Current understanding of core collapse and thermonuclear supernovae is reviewed. Recent progress in unveiling the nature of cosmic gamma-ray bursts (GRB) is discussed, with the focus on the apparent link of several GRBs with an energetic…

Astrophysics · Physics 2007-05-23 Konstantin Postnov

One of the most dramatic possible consequences of stellar rotation is its influence on stellar death, particularly of massive stars. If the angular momentum of the iron core when it collapses is such as to produce a neutron star with a…

Astrophysics · Physics 2007-05-23 S. E. Woosley , A. Heger

We here propose a two-step model for gamma-ray bursts (GRBs) associated with supernovae. In the first step, the core collapse of a star with mass $\ge 19M_\odot$ leads to a massive neutron star and a normal supernova, and subsequently…

Astrophysics · Physics 2007-05-23 K. S. Cheng , Z. G. Dai

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…

High Energy Astrophysical Phenomena · Physics 2023-04-05 Yun-Wei Yu , He Gao , Fa-Yin Wang , Bin-Bin Zhang

The connection between long Gamma Ray Bursts (GRBs) and Supernovae (SNe), have been established through the well observed cases of GRB980425/SN 1998bw, GRB030329/SN 2003dh and GRB031203/SN 2003lw. These events can be explained as the prompt…

Astrophysics · Physics 2007-07-17 Ken'ichi Nomoto , Masaomi Tanaka , Nozomu Tominaga , Keiichi Maeda , Paolo A. Mazzali

Cosmic gamma-ray bursts (GRBs) have been firmly established as one of the most powerful phenomena in the Universe, releasing electromagnetic energy approaching the rest-mass energy of a neutron star in a few seconds. The two currently…

The observations suggest that $\gamma$-ray bursts (GRBs) are produced by jets of relativistic cannonballs (CBs), emitted in supernova (SN) explosions. The CBs, reheated by their collision with the SN shell, emit radiation and Doppler-boost…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. De Rujula
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