Speaker
Hirotaka Ito
(RIKEN)
Description
In the current study, we present hydrodynamical simulations and post-process radiation transfer calculations of photospheric emission in GRBs. Our simulations show that the photospheric emission can reproduce the observed correlations among the spectral peak energy, $E_p$, peak luminosity, $L_p$, and isotropic energy, $E_{iso}$, as a consequence of the viewing angle dependence. We also find that the time-resolved property of the emission shows $E_p$–$L_{iso}$ tracking behavior that is consistent which the observation.
Primary author
Hirotaka Ito
(RIKEN)
Co-authors
Dr
Jin Matsumoto
Dr
Shigehiro Nagataki
Dr
Donald Warren
Dr
Maxim Barkov
Prof.
Daisuke Yonetoku
Dr
Oliver Just
Mr
Yuki Takei