GRB 970228 and Its Associated Supernova within the EMBH Model

Details GRB 970228 and Its Associated Supernova within the EMBH Model GRB 970228 and Its Associated Supernova within the EMBH Model

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.2465r&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

The γ-ray burst of 1997 February 28 is analyzed within the Electromagnetic Black Hole model. We first estimate the value of the total energy deposited in the dyadosphere, Edya, and the amount of baryonic matter left over by the EMBH progenitor star, B = MBc2/Edya. We then consider the role of the interstellar medium number density nISM and of the ratio R between the effective emitting area and the total surface area of the γ-ray burst source, in reproducing the prompt emission and the X-ray afterglow of this burst. Some considerations are also done concerning the possibility of explaining, within the theory, the observed evidence for a supernova in the optical afterglow.

Affiliated with

Also associated with

No associations

Rating

GRB 970228 and Its Associated Supernova within the EMBH Model 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 GRB 970228 and Its Associated Supernova within the EMBH Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GRB 970228 and Its Associated Supernova within the EMBH Model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1841651