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Related papers: Cosmic ray escape from supernova remnants

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Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Gamma-ray observations of both supernova remnants and associated molecular clouds have been used in several occasions to test (so far quite successfully) this…

High Energy Astrophysical Phenomena · Physics 2017-08-09 Stefano Gabici

We review the main observational and theoretical facts about acceleration of Galactic cosmic rays in supernova remnants, discussing the arguments in favor and against a connection between cosmic rays and supernova remnants, the so-called…

High Energy Astrophysical Phenomena · Physics 2017-08-23 Pasquale Blasi

Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular and robust, this conjecture still needs a conclusive proof. The strongest support to this idea is probably the fact that supernova remnants…

High Energy Astrophysical Phenomena · Physics 2015-06-15 P. Cristofari , S. Gabici , S. Casanova , R. Terrier , E. Parizot

The origin of cosmic rays holds still many mysteries hundred years after they were first discovered. Supernova remnants have for long been the most likely sources of Galactic cosmic rays. I discuss here some recent evidence that suggests…

High Energy Astrophysical Phenomena · Physics 2012-06-13 Jacco Vink

Galactic cosmic rays are widely believed to be accelerated in expanding shock waves initiated by supernova explosions. The theory of diffusive shock acceleration of cosmic rays is now well established, but two fundamental questions remain…

Astrophysics · Physics 2008-07-25 Vincent Tatischeff

Galactic cosmic rays are commonly believed to be accelerated at supernova remnants via diffusive shock acceleration. Despite the popularity of this idea, a conclusive proof for its validity is still missing. Gamma-ray astronomy provides us…

High Energy Astrophysical Phenomena · Physics 2019-08-13 F. Acero , A. Bamba , S. Casanova , E. de Cea , E. de Ona Wilhelmi , S. Gabici , Y. Gallant , D. Hadasch , A. Marcowith , G. Pedaletti , O. Reimer , M. Renaud , D. F. Torres , F. Volpe

The escape of charged particles accelerated by diffusive shock acceleration from supernova remnants is shown to be a more complex process than normally appreciated. Using a box model it is shown that the high-energy end of the spectrum can…

Astrophysics of Galaxies · Physics 2015-05-20 Luke O'C. Drury

The supernova paradigm for the origin of galactic cosmic rays has been deeply affected by the development of the non-linear theory of particle acceleration at shock waves. Here we discuss the implications of applying such theory to the…

High Energy Astrophysical Phenomena · Physics 2015-03-13 D. Caprioli , E. Amato , P. Blasi

Diffusive shock acceleration operating at expanding supernova remnant shells is by far the most popular model for the origin of galactic cosmic rays. Despite the general consensus received by this model, an unambiguous and conclusive proof…

Astrophysics · Physics 2008-11-07 Stefano Gabici

We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summarize observations of supernova remnants, covering the whole electromagnetic spectrum and describe what these obser- vations tell us about…

High Energy Astrophysical Phenomena · Physics 2015-06-05 E. A. Helder , J. Vink , A. M. Bykov , Y. Ohira , J. C. Raymond , R. Terrier

Diffusive shock acceleration is the prime candidate for efficient acceleration of cosmic rays. Galactic cosmic rays are believed to originate predominantly from this process in supernova remnant shock waves. Confinement of the cosmic rays…

High Energy Astrophysical Phenomena · Physics 2011-10-07 K. M. Schure , A. R. Bell

It is widely believe that galactic cosmic rays are originated in supernova remnants (SNRs) where they are accelerated by diffusive shock acceleration process at supernova blast waves driven by expanding SNRs. In recent theoretical…

High Energy Astrophysical Phenomena · Physics 2017-08-02 Prabir Banik , Arunava Bhadra

Recent high energy gamma-ray observations of both single supernova remnants and superbubbles, together with observations of supernovae, star formation regions, and local cosmic ray composition, now provide an integrated framework tying…

High Energy Astrophysical Phenomena · Physics 2018-10-31 Richard E. Lingenfelter

The origin of Galactic cosmic-ray ions has remained an enigma for almost a century. Although it has generally been thought that they are accelerated in the shock waves associated with powerful supernova explosions-for which there have been…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Yousaf Butt

It is presumed that the observed cosmic rays up to about $3\times 10^{18}$ eV are of Galactic origin, the particles being the ones which are found in the composition of the stellar winds of stars that explode as supernova into the…

Astrophysics · Physics 2007-05-23 Adrian Sabin Popescu

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Giovanni Morlino

It is thought that Galactic cosmic ray (CR) nuclei are gradually accelerated to high energies (up to ~300 TeV/nucleon, where 1TeV=10^12eV) in the expanding shock-waves connected with the remnants of powerful supernova explosions. However,…

The last decade has been dense with new developments in the search for the sources of Galactic cosmic rays. Some of these developments have confirmed the tight connection between cosmic rays and supernovae in our Galaxy, through the…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Pasquale Blasi

It is widely believed that supernova remnants are the best candidate sources for the observed cosmic ray flux up to the knee, i.e. up to ~PeV energies. Indeed, the gamma-ray spectra of some supernova remnants can be well explained by…

High Energy Astrophysical Phenomena · Physics 2015-09-02 Nils Nierstenhoefer , Philipp Graeser , Florian Schuppan , Julia Becker Tjus

Supernova remnants are known to accelerate cosmic rays on account of their non-thermal emission of radio waves, X-rays, and gamma rays. Although there are many models for the acceleration of cosmic rays in Supernova remnants, the escape of…

High Energy Astrophysical Phenomena · Physics 2020-02-19 Robert Brose , Martin Pohl , Iurii Sushch , Oleh Petruk , Taras Kuzyo
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