Gamma-ray burst afterglows
JV Paradijs, C Kouveliotou… - Annual review of …, 2000 - annualreviews.org
▪ Abstract The discovery of counterparts in X-ray and optical to radio wavelengths has
revolutionized the study of γ-ray bursts, until recently the most enigmatic of astrophysical …
revolutionized the study of γ-ray bursts, until recently the most enigmatic of astrophysical …
Neutrino-dominated accretion flows as the central engine of gamma-ray bursts
Neutrino-dominated accretion flows (NDAFs) around rotating stellar-mass black holes (BHs)
are plausible candidates for the central engines of gamma-ray bursts (GRBs). NDAFs are …
are plausible candidates for the central engines of gamma-ray bursts (GRBs). NDAFs are …
Experimental entanglement purification of arbitrary unknown states
Distribution of entangled states between distant locations is essential for quantum
communication,, over large distances. But owing to unavoidable decoherence in the …
communication,, over large distances. But owing to unavoidable decoherence in the …
Properties of relativistic jets in gamma-ray burst afterglows
A Panaitescu, P Kumar - The Astrophysical Journal, 2002 - iopscience.iop.org
We extend our calculation of physical parameters of gamma-ray burst (GRB) jets by
modeling the broadband emission of the afterglows 970508, 980519, 991208, 000926 …
modeling the broadband emission of the afterglows 970508, 980519, 991208, 000926 …
Wind interaction models for gamma-ray burst afterglows: the case for two types of progenitors
RA Chevalier, ZY Li - The Astrophysical Journal, 2000 - iopscience.iop.org
Beginning with the γ-ray bursts GRB 970228 and GRB 970508, a standard model for the
interpretation of gamma-ray burst (GRB) afterglows emerged involving synchrotron emission …
interpretation of gamma-ray burst (GRB) afterglows emerged involving synchrotron emission …
[图书][B] Computer science handbook
AB Tucker - 2004 - taylorfrancis.com
When you think about how far and fast computer science has progressed in recent years, it's
not hard to conclude that a seven-year old handbook may fall a little short of the kind of …
not hard to conclude that a seven-year old handbook may fall a little short of the kind of …
Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002
W Coburn, SE Boggs - nature, 2003 - nature.com
Observations of the afterglows of γ-ray bursts (GRBs) have revealed that they lie at
cosmological distances, and so correspond to the release of an enormous amount of …
cosmological distances, and so correspond to the release of an enormous amount of …
Large scale magnetic fields and their dissipation in GRB fireballs
HC Spruit, F Daigne, G Drenkhahn - Astronomy & Astrophysics, 2001 - aanda.org
We consider possible geometries of magnetic fields in GRB outflows, and their evolution
with distance from the source. For magnetically driven outflows, with an assumed ratio of …
with distance from the source. For magnetically driven outflows, with an assumed ratio of …
Constraining gamma-ray burst initial Lorentz factor with the afterglow onset feature and discovery of a tight Γ0–Eγ, iso correlation
EW Liang, SX Yi, J Zhang, HJ Lü… - The Astrophysical …, 2010 - iopscience.iop.org
The onset of gamma-ray burst (GRB) afterglow is characterized by a smooth bump in the
early afterglow light curve as the GRB fireball is decelerated by the circumburst medium. We …
early afterglow light curve as the GRB fireball is decelerated by the circumburst medium. We …
GRB 990123: reverse and internal shock flashes and late afterglow behaviour
P Mészáros, MJ Rees - Monthly Notices of the Royal …, 1999 - academic.oup.com
Abstract The prompt (t≲ 0.16 d) light curve and initial 9th-magnitude optical flash from GRB
990123 can be attributed to a reverse external shock, or possibly to internal shocks. We …
990123 can be attributed to a reverse external shock, or possibly to internal shocks. We …