▪ 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 …

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 …

Distribution of entangled states between distant locations is essential for quantum
communication,, over large distances. But owing to unavoidable decoherence in the …

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 …

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 …

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 …

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 …

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 …

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 …

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 …