2003ApJ...591.1104P

Query : 2003ApJ...591.1104P

2003ApJ...591.1104P - Astrophys. J., 591, 1104-1109 (2003/July-2)

Neutrinos from the propagation of a relativistic jet through a star.

PRUET J.

Abstract (from CDS):

We discuss the neutrino signature of a relativistic jet propagating through a stellar envelope, a scenario realized in the collapsar model for gamma-ray bursts (GRBs). It is shown that the dramatic slowing of the jet deep within the star is accompanied by inelastic neutron-nucleon collisions and the conversion of a substantial fraction of the jet kinetic energy to neutrinos. These neutrinos have observed energies in the range from 2 to tens of GeV and an estimated detection rate comparable to or larger than the detection rate of GeV neutrinos from other GRB-related processes. The time delay between the arrival of these neutrinos and the GRB photons is tens of seconds. An observation of this delay would provide an indication that the GRB jet originated in a massive star.

Abstract Copyright: ∼

Journal keyword(s): Gamma Rays: Bursts - Neutrinos

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2

Query : 2003ApJ...591.1104P

Basic data :
SN 1998bw -- SuperNova
Other object types: otypes_help 		gB (GRB,Trigger,...), SN* (2016ApJ,SN), V* (AAVSO)
ICRS coord. (ep=J2000) : 		19 35 03.17 -52 50 46.1 [ ] D 2008yCat.2283....0B
FK4 coord. (ep=B1950 eq=1950) : 		19 31 08.21 -52 57 22.2 [ ]
Gal coord. (ep=J2000) : 		344.99305 -27.71686 [ ]
Radial velocity / Redshift / cz : 		V(km/s) 2537 [~] / z(~) 0.0085 [~] / cz 2548 [~]
   D 1998IAUC.6896Q...1T
Spectral type: 		SNIc C 2008yCat....1.2024B
Fluxes (1) :
B 14.09 [~] D 2008yCat.2283....0B
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Hierarchy : number of linked objects
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Identifiers (6) :
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SN 1998bw Trigger 6707 [STK2001] 10928c
GRB 980425 XRF 980425 AAVSO 1927-53

References (1928 between 1850 and 2026) (Total 1928)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Velocities : 2    SpT : 1   

   

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