A Unified Model of Short and Long Gamma-Ray Bursts, X-Ray Rich Gamma-Ray   Bursts, and X-Ray Flashes
  Taking into account the recent suggestion that a short gamma-ray burst (GRB) looks like the first 1 sec of a long GRB, we propose that the jet of a GRB consists of multiple sub-jets or sub-shells (i.e., an inhomogeneous jet model). The multiplicity of the sub-jets along a line of sight n_s is an important parameter. If n_s is large (>> 1) the event looks like a long GRB, while if n_s is small (~1) the event looks like a short GRB. If our line of sight is off-axis to any sub-jets, the event looks like an X-ray flash or an X-ray rich GRB. The log-normal distribution of durations of short and long GRBs are also suggested in the same model. 
Ryo Yamazaki (1,2), Kunihito Ioka (2), Takashi Nakamura (1) ((1)Kyoto   University, (2)Osaka University)