A revamped understanding of Cosmic Rays and Gamma-Ray Bursts

TL;DR

This paper reviews recent high-energy astrophysical data on Gamma Ray Bursts and Cosmic Rays, analyzing them through the CannonBall Model, which links these phenomena and is supported by current observations.

Contribution

It provides a new interpretation of recent data on GRBs and CRs within the CannonBall Model, validating this model against recent measurements.

Findings

GRB221009A has a record peak energy.

CR electron spectrum shows a knee at high energies.

IceCube has not detected neutrinos from GRBs.

Abstract

Interesting data on Gamma Ray Burts (GRBs) and Cosmic Rays (CRs) have recently been made public. GRB221009A has a record ``peak energy". The CR electron spectrum has been measured to unprecedented high energies and exhibits a ``knee" akin to the ones in all-particle or individual-element CR nuclei. IceCube has not seen high-energy neutrinos associated with GRBs. AMS has published a CR positron spectrum conducive to much speculation. We examine these data in the light of the ``CannonBall Model" of GRBs and CRs, in which they are intimately related and which they do strongly validate.