Neutrinos from SN1987A and current models of stellar-core collapse

Details Neutrinos from SN1987A and current models of stellar-core collapse Neutrinos from SN1987A and current models of stellar-core collapse

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvl..59..938b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 59, Aug. 24, 1987, p. 938-941.

Physics

71

Gravitational Collapse, Neutrinos, Stellar Cores, Supernovae, Stellar Luminosity, Stellar Models, Stellar Physics, Time Response

Scientific paper

Published observational data on neutrinos from the LMC supernova SN 1987A (Hirata et al., 1987; Bionta et al., 1987) are analyzed by comparing them with the neutrino signatures predicted by 1.6-sec stellar-core-collapse simulations coupling general relativistic hydrodynamics to multigroup transport of all neutrino types, as proposed by Bruenn (1985). The modeling techniques and assumptions are discussed in detail, and the data and results are presented in graphs. It is found that the observational data are best fit by a model of a delayed-shock SN initiated by the collapse of a small core (1.35 solar mass).

Affiliated with

Also associated with

No associations

Rating

Neutrinos from SN1987A and current models of stellar-core collapse does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Neutrinos from SN1987A and current models of stellar-core collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrinos from SN1987A and current models of stellar-core collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1342420