Computer Science – Numerical Analysis
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..139s&link_type=abstract
ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 139-140 (2005).
Computer Science
Numerical Analysis
Gamma-Ray Sources (Astronomical), Astronomical Photometry, Shock Waves, Numerical Analysis, Gamma-Ray Sources, Gamma-Ray Bursts
Scientific paper
We present a numerical GRB shock model, where the specific characteristics of a shock wave have been taken into account. The model have been used to simulate collision between faster and slower shock wave. We assumed that slower shock wave can be represented by Gaussian function. The model was applied to simulate the peaks in the light curve for tree different GRB events in all four BATSE channels. By fitting those curves we are able to extract the basic parameters for shock waves, which we present in the table.
Andersen Michael I.
Christensen Lise
Popovic Luka C.
Simić Sasa
No associations
LandOfFree
A model for temporal variability of the GRB light curve 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 A model for temporal variability of the GRB light curve, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A model for temporal variability of the GRB light curve will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1834709