Cosmic Ray Origin - Beyond the Standard Models
Omar Tibolla, Roger D. Blandford

TL;DR
This paper discusses the limitations of the standard model of cosmic ray origins, highlighting recent observations that suggest the need for alternative theories beyond Diffusive Shock Acceleration in Supernova Remnants.
Contribution
It reviews the motivation for re-evaluating cosmic ray origins and introduces alternative scenarios beyond the standard DSA model.
Findings
Standard model insufficient for recent observations
Alternative cosmic ray origin scenarios proposed
Need for revised theories in cosmic ray physics
Abstract
Given the success of the first meeting of "Cosmic Ray Origin - Beyond the Standard Models" (CRBTSM 2014), it was decided to hold a second meeting of this international conference. In these introductory remarks, we rehearse the motivation for reconsidering the origin(s) of cosmic rays (CR). We argue that the standard model, in which the majority of Galactic cosmic rays are produced through Diffusive Shock Acceleration (DSA) in SuperNova Remnants (SNR), is insufficient to account for recent observations. Some alternative scenarios are introduced and examined.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Gamma-ray bursts and supernovae
