Kinematic Origin OF Correlations Between Gamma Ray Burst Observables

Details Kinematic Origin OF Correlations Between Gamma Ray Burst Observables Kinematic Origin OF Correlations Between Gamma Ray Burst Observables

2010-01-12

arxiv.org/abs/1001.1865v3

ApJ, 749, 100 (2012)

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Accepted for publication in ApJ

Scientific paper

Recently, several new correlations between gamma ray burst (GRB) observables have been discovered. Like previously well established correlations, they challenge GRB models. Here we show that in the cannonball (CB) model of GRBs, these newly discovered correlations have the same simple kinematic origin as those discovered earlier. They all result from the strong dependence of the observed radiations on the Lorentz and Doppler factors of the jet of highly relativistic plasmoids (CBs) that produces the observed radiations by interaction with the medium through which it propagates.

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