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Related papers: Black hole accretion in gamma ray bursts

200 papers

The accretion of hot, dense matter which consists of heavy nuclei, free nucleons, degenerated electrons, photons and neutrinos is studied. The composition of free nucleons and their chemical potentials are provided through the equation of…

Astrophysics · Physics 2007-05-23 M. Yokosawa , S. Uematsu , J. Abe

The generation of relativistic jets in active sources such as blazars is a complex problem with many aspects, most of them still not fully understood. Relativistic jets are likely produced by the accretion of matter and magnetic fields onto…

High Energy Astrophysical Phenomena · Physics 2020-07-21 Gustavo E. Romero , Eduardo M. Gutiérrez

GRS 1915+105 was the first stellar-mass black-hole in our Galaxy to display a superluminal radio jet, similar to those observed in active galactic nuclei with a supermassive black hole at the centre. It has been proposed that the radio…

High Energy Astrophysical Phenomena · Physics 2022-03-08 Mariano Mendez , Konstantinos Karpouzas , Federico Garcia , Liang Zhang , Yuexin Zhang , Tomaso M. Belloni , Diego Altamirano

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

The temporal properties of a sample of 498 bright gamma-ray bursts (GRBs) with durations between 0.05 s and 674 s were analysed. The large range in duration (T90) is accompanied by a similarly large range in the median values of the pulse…

Astrophysics · Physics 2009-11-07 S. McBreen , B. McBreen , F. Quilligan , L. Hanlon

In this study we explore the magnetic mechanism of hypernovae and relativistic jets of long duration gamma ray bursts within the collapsar scenario. This is an extension of our earlier work [1]. We track the collapse of massive rotating…

Astrophysics · Physics 2009-11-13 Maxim V. Barkov , Serguei S. Komissarov

The observations and theory of the exciting new class of galactic black hole X-ray transients is reviewed. Seven of these systems have measured mass functions or mass estimates in excess of stable neutron stars, making them excellent black…

Astrophysics · Physics 2007-05-23 J. Craig Wheeler

Black hole-neutron star (BHNS) binaries are expected to be among the leading sources of gravitational waves observable by ground-based detectors, and may be the progenitors of short-hard gamma ray bursts (SGRBs) as well. Here, we discuss…

The spectacular detection of gravitational waves (GWs) from GW 150914 and its reported association with a gamma-ray burst (GRB) offer new insights into the evolution of massive stars. Here it is shown that no single star of any mass and…

High Energy Astrophysical Phenomena · Physics 2016-06-15 S. E. Woosley

Active galaxies and quasers are believed to harbour Black Holes at their centers and at the same time produce cosmic radio jets through which immense amount of matter and energy are ejected out of the core of the galaxy. In our work we…

Astrophysics · Physics 2007-05-23 Tapas K. Das

An introduction is given to a meeting on the role of massive and stellar black holes in powering non-thermal activity in a rich variety of cosmic sources. Relevant properties of magnetized, spinning black holes are summarized and their…

High Energy Astrophysical Phenomena · Physics 2019-01-17 Roger Blandford

Accretion onto black holes often leads to the launch of outflows that significantly influence their surrounding environments. The two primary forms of these outflows are X-ray disk winds-hot, ionized gases ejected from the accretion…

We present the first numerical result of fully general relativistic axisymmetric simulations for the collapse of a rotating high-entropy stellar core to a black hole and an accretion disk. The simulations are performed taking into account…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Yuichiro Sekiguchi , Masaru Shibata

Many models of gamma-ray bursts (GRBs) involve accretion onto a compact object, usually a black hole, at a mass accretion rate of order a fraction of a solar mass per second. If the accretion disk is larger than a few tens or hundreds of…

Astrophysics · Physics 2009-11-06 Ramesh Narayan , Tsvi Piran , Pawan Kumar

We study the evolution in axisymmetry of accretion disks formed self-consistently through collapse of magnetized hypermassive neutron stars to black holes. Such stars can arise following the merger of binary neutron stars. They are…

Astrophysics · Physics 2008-12-18 Branson C. Stephens , Yuk Tung Liu , Stuart L. Shapiro

Long-duration gamma-ray bursts are thought to be associated with the core-collapse of massive, rapidly spinning stars and the formation of black holes. However, efficient angular momentum transport in stellar interiors, currently supported…

A population of binary stellar-mass black hole (BBH) mergers are believed to occur embedded in the accretion disk of active galactic nuclei (AGNs). In this {\em Letter}, we demonstrate that the jets from these BBH mergers can propagate…

High Energy Astrophysical Phenomena · Physics 2023-11-21 Jin-Ping Zhu

There are the two common candidates as the viable energy source for the central engine of long gamma-ray bursts (GRBs) and hypernovae (HNe), neutrino annihilation and magnetic fields. We investigate gravitational wave (GW) emission…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Yudai Suwa , Kohta Murase

Twenty five years have passed by since models of accretions and jets have separately emerged. Today, it is understood that these two objects are related to each other in a fundamental way. In a binary system, matter from an accretion disk…

Astrophysics · Physics 2009-09-25 Sandip K. Chakrabarti

We report results from simulations in general relativity of magnetized disks accreting onto merging black hole binaries, starting from relaxed disk initial data. The simulations feature an effective, rapid radiative cooling scheme as a…

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