Evolution of an afterglow with a hard electron spectrum

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages, 2 figures, contribution to Rome 2002 GRB Workshop

Scientific paper

Diffusive shock acceleration theory suggests that the ``universal'' energy spectrum of electrons with a power-law index p approximately equal to 2.3, commonly used to model GRB afterglows, cannot extend below an electron lorentz factor gamma_e equal to the bulk lorentz factor of the blast wave multiplied by the ratio of proton and electron masses. We suggest that the electron energy distribution has a slope p < 2 below this limit, down to an appropriate gamma_m. A two-slope spectrum such as this provides a good model for the afterglow of GRB010222.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Evolution of an afterglow with a hard electron spectrum 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 Evolution of an afterglow with a hard electron spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of an afterglow with a hard electron spectrum will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-443906

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.