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On the role of injection in kinetic approaches to nonlinear particle acceleration at non-relativistic shock waves

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TLDR
In this article, the role of injection in selecting the real solution, in the framework of a simple phenomenological recipe, is discussed, which is a variation of what is sometimes referred to as thermal leakage.
Abstract
The dynamical reaction of the particles accelerated at a shock front by the first order Fermi process can be determined within kinetic models that account for both the hydrodynamics of the shocked fluid and the transport of the accelerated particles. These models predict the appearance of multiple solutions, all physically allowed. We discuss here the role of injection in selecting the real solution, in the framework of a simple phenomenological recipe, which is a variation of what is sometimes referred to as thermal leakage. In this context we show that multiple solutions basically disappear and when they are present they are limited to rather peculiar values of the parameters. We also provide a quantitative calculation of the efficiency of particle acceleration at cosmic ray modified shocks and we identify the fraction of energy which is advected downstream and that of particles escaping the system from upstream infinity at the maximum momentum. The consequences of efficient particle acceleration for shock heating are also discussed.

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Supernova remnants: the X-ray perspective

TL;DR: In particular, the advances made in X-ray imaging spectroscopy over the last two decades has greatly increased our knowledge about supernova remnants as mentioned in this paper, and it has made it possible to map the products of fresh nucleosynthesis, and resulted in the identification of regions near shock fronts that emit Xray synchrotron radiation.
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Simulations of Ion Acceleration at Non-relativistic Shocks. I. Acceleration Efficiency

TL;DR: In this article, the authors used two-dimensional and three-dimensional hybrid (kinetic ions-fluid electrons) simulations to investigate particle acceleration and magnetic field amplification at nonrelativistic astrophysical shocks.
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The origin of galactic cosmic rays

TL;DR: In this article, the authors present a review of the ideas that have been and are being explored in order to account for the observable quantities related to cosmic rays and summarize the numerous new pieces of observation that are becoming available.
Journal ArticleDOI

Simulations of Ion Acceleration at Non-relativistic Shocks. I. Acceleration Efficiency

TL;DR: In this article, the authors used 2D and 3D hybrid (kinetic ions - fluid electrons) simulations to investigate particle acceleration and magnetic field amplification at nonrelativistic astrophysical shocks.
Journal ArticleDOI

Strong evidence for hadron acceleration in Tycho’s supernova remnant

TL;DR: In this paper, a semi-analytical approach to nonlinear diffusive shock acceleration was proposed, including magnetic field amplification due to resonant streaming instability and the dynamical backreaction on the shock of both cosmic rays (CRs) and self-generated magnetic turbulence.
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