Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts
Authors: Katsuaki Asano
Asano
2005 The Astrophysical Journal623967.
Provider: AAS Journals
Caption: Fig. 1.
Proton cooling efficiencies τπ, τSY, and τIC for ﹩R=10^{13}﹩ cm and ﹩E_{\gamma }=10^{51}﹩ ergs. The proton energies are measured in the observer frame.