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相关论文: Two Populations and Models of Gamma Ray Bursts

200 篇论文

The motions of comets and neutron stars have been integrated over five billion years in the Galactic potential to determine a gamma-ray burst distribution, presuming that bursts are the result of interactions between these two families of…

天体物理学 · 物理学 2009-10-28 M. G. Higgins , R. N. Henriksen

If gamma-ray bursts originate in our Galaxy, they probably involve violent disturbances in the magnetospheres of neutron stars. Any event of this kind is likely to trigger the sudden expulsion of magnetic flux and plasma at relativistic…

天体物理学 · 物理学 2016-06-08 Mitchell C. Begelman , P. Meszaros , Martin J. Rees

We propose that the cosmological gamma ray bursts arise from the collapse of neutron stars to black holes triggered by collisions or mergers with main sequence stars. This scenario represents a cosmological history qualitatively different…

天体物理学 · 物理学 2009-10-30 Brad M. S. Hansen , Chigurupati Murali

The little we do know of the physical conditions in gamma-ray bursters makes them conducive to the acceleration of high-energy cosmic rays, especially if they are at cosmological distances. We find that, with the observed statistics and…

天体物理学 · 物理学 2008-11-26 Mordehai Milgrom , Vladimir Usov

$\gamma$-ray bursts have baffled theorists ever since their accidental discovery at the sixties. We suggest that these bursts originate in merger of neutron star binaries, taking place at cosmological distances. These mergers release…

天体物理学 · 物理学 2007-05-23 Tsvi Piran

The evolution of the comoving cosmic merger-rate density of neutron star binaries n_c(z) is calculated using a distribution of their merging times provided by population-synthesis computations of binary stars. We adopt an exponential law…

天体物理学 · 物理学 2007-05-23 Philippe Bagot , Simon F. Portegies Zwart , Lev R. Yungelson

We discuss the possibility that the sources for gamma ray bursts are hot neutron stars at cosmological distance scales. The temperature of such stars would be $T \sim 1 \MeV$. Such hot stars can produce an electromagnetic blast wave…

天体物理学 · 物理学 2016-08-30 Henning Heiselberg , Sangyong Jeon , Larry McLerran , Hua-Bin Tang

It is proposed that gamma-ray bursts are created in the mergers of double neutron star binaries and black hole neutron star binaries at cosmological distances. Bursts with complex profiles and relatively long durations are the result of…

天体物理学 · 物理学 2009-10-22 Ramesh Narayan , Bohdan Paczyński , Tsvi Piran

We report evidence from the 3B Catalogue that long ($T_{90} > 10$ s) and short ($T_{90} < 10$ s) gamma-ray bursts represent distinct source populations. Their spatial distributions are significantly different, with long bursts having…

天体物理学 · 物理学 2009-10-28 J. I. Katz , L. M. Canel

Gamma-ray bursts are short-lived, luminous explosions at cosmological distances, thought to originate from relativistic jets launched at the deaths of massive stars. They are among the prime candidates to produce the observed cosmic rays at…

高能天体物理现象 · 物理学 2015-10-15 Mauricio Bustamante , Philipp Baerwald , Kohta Murase , Walter Winter

The stellar origin of gamma-ray bursts can be explained by the rapid release of energy in a highly collimated, extremely relativistic jet. This in turn appears to require a rapidly spinning highly magnetised stellar core that collapses into…

太阳与恒星天体物理 · 物理学 2015-05-19 Christopher A. Tout , Dayal T. Wickramasinghe , Herbert H. -B. Lau , J. E. Pringle , Lilia Ferrario

We describe observational evidence and theoretical calculations which support the high velocity neutron star model of gamma-ray bursts. We estimate the energetic requirements in this model, and discuss possible energy sources. we also…

天体物理学 · 物理学 2009-10-28 Donald Q. Lamb , Tomasz Bulik , Paolo S. Coppi

Gamma-ray bursts are still not fully understood events. However, their exploration could provide a useful tool for a better understanding of the early Universe because they belong to the most distant and violent objects that astronomers…

高能天体物理现象 · 物理学 2011-05-13 Jakub Ripa

$\gamma$-ray bursts have baffled theorists ever since their accidental discovery at the sixties. We suggest that these bursts originate in merger of neutron star binaries, taking place at cosmological distances. These mergers release…

天体物理学 · 物理学 2009-10-22 Tsvi Piran

Due to their extreme luminosities, gamma-ray bursts (GRBs) can be detected in hostile regions of galaxies, nearby and at very high redshift, making them important cosmological probes. The investigation of galaxies hosting long-duration GRBs…

宇宙学与河外天体物理 · 物理学 2015-06-12 S. Savaglio

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars or black holes. Since these compact stellar remnants form…

天体物理学 · 物理学 2020-11-25 Ralph A. M. J. Wijers , Joshua S. Bloom , Jasjeet S. Bagla , Priyamvada Natarajan

Short-hard Gamma Ray Bursts (SGRBs) are currently thought to arise from gravitational wave driven coalescences of double neutron star systems forming either in the field or dynamically in globular clusters. For both channels we fit the peak…

天体物理学 · 物理学 2009-11-13 R. Salvaterra , A. Cerutti , G. Chincarini , M. Colpi , C. Guidorzi , P. Romano

The present common view about GRB origin is related to cosmology. There are two evidences in favour of this interpretation. The first is connected with statistics, the second is based on measurements of the redshifts in the GRB optical…

天体物理学 · 物理学 2009-11-06 G. S. Bisnovatyi-Kogan

The observed spatial distribution of $\gamma-$ray bursts indicates that they probably originate at cosmological distances. At this distance scale their variability timescale and flux above MeV imply an initial optical-depth to pair…

天体物理学 · 物理学 2010-01-06 Abraham Loeb

We study a cosmological scenario for gamma ray bursts (GRBs) where relativistic flows interact with dense radiation fields. It is shown that this scenario is plausible in very dense stellar regions which are known to exist in collapsed…

天体物理学 · 物理学 2015-06-24 Nir J. Shaviv , Arnon Dar
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