Late light curves of SN Ia

Details Late light curves of SN Ia Late light curves of SN Ia

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..522...85m&link_type=abstract

COSMIC EXPLOSIONS: Tenth Astrophysics Conference. AIP Conference Proceedings, Volume 522, pp. 85-89 (2000).

Physics

Nuclear Physics

1

Supernovae, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments

Scientific paper

A ``positron phase'' exists in type Ia supernovae, during which the energy deposition into the SN ejecta is dominated by the slowing of 56Co-->56Fe β+ decay positrons. Comparisons of model-generated bolometric light curves with V and B band photometry during this phase suggests that the magnetic field is either too weak to confine positrons, or is radially combed. In each case, positrons escape the ejecta leading to a deficit of energy deposition. Ramifications of this escape upon other studies of SN Ia emission is discussed. .

Affiliated with

Also associated with

No associations

Rating

Late light curves of SN Ia 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 Late light curves of SN Ia, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Late light curves of SN Ia will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1390474