Fig. 8 from Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts

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Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts

Authors: Katsuaki Asano

Asano 2005 The Astrophysical Journal 623 967.

Provider: AAS Journals

Caption: Fig. 8.

Ratio of neutrino energy to the initial proton energy. Dashed lines are for neutrinos originated from pions only, and solid lines are the total fraction. The shell width is assumed to be 10¹⁰ (open circles), 10¹² (rectangles), and 10¹⁴ (filled circles) cm, respectively.

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