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相关论文: Supernova-Remnant Origin of Cosmic Rays?

200 篇论文

We develop a theory to account for the cosmic ray spectrum between 1 GeV and 10^4 GeV following the earlier papers of this series. We use the basic concept that the cosmic ray particles are accelerated in a supernova shock that travels…

天体物理学 · 物理学 2007-05-23 Peter L. Biermann , Richard G. Strom

Supernova remnants (SNRs) are thought to be the most promising sources of Galactic cosmic rays. One of the principal questions is whether they are accelerating particles up to the maximum energy of Galactic cosmic rays ($\sim$ PeV). In this…

高能天体物理现象 · 物理学 2022-01-19 Hiromasa Suzuki , Aya Bamba , Ryo Yamazaki , Yutaka Ohira

Supernova remnants (SNRs) have long been hypothesized as the main source of Galactic Cosmic Rays up to PeV energies. Some of them have indeed been shown to accelerate protons to TeV energies and above. But which of them are indeed efficient…

高能天体物理现象 · 物理学 2019-07-22 Henrike Fleischhack

Cosmic rays are a sample of solar, galactic and extragalactic matter. Their origin and properties are one of the most intriguing question in modern astrophysics. The most energetic events and active objects in the Universe: supernovae…

高能天体物理现象 · 物理学 2012-08-30 Piergiorgio Picozza , Mirko Boezio

The proof of cosmic ray (CR) origin in supernova remnants (SNR) must hinge on full consistency of the CR acceleration theory with the observations; direct proof is impossible because of the orbit stochasticity of CR particles. Recent…

星系天体物理 · 物理学 2016-10-11 M. A. Malkov , P. H. Diamond , R. Z. Sagdeev

A complete model for the origin of high-energy >~10^{14} eV) cosmic rays from gamma-ray bursts (GRBs) and implications of this hypothesis are described. Detection of high-energy neutrinos from GRBs provide an unambiguous test of the model.…

天体物理学 · 物理学 2010-11-11 C. Dermer

Abbreviated Abstract: A kinetic model of particle acceleration in supernova remnants (SNRs) is extended to study the cosmic ray (CR) and associated high energy gamma-ray production during SN shock propagation through the inhomogeneous…

天体物理学 · 物理学 2007-05-23 Evgeny G. Berezhko , Heinrich J. Voelk

A review is given of the main properties of the charged component of galactic cosmic rays, particles detected at Earth with an energy spanning from tens of MeV up to about 10^19 eV. After a short introduction to the topic and an historical…

星系天体物理 · 物理学 2011-10-24 Antonella Castellina , Fiorenza Donato

Recently, gamma-ray telescopes AGILE and Fermi observed several middle-aged supernova remnants (SNRs) interacting with molecular clouds. It is likely that their gamma rays arise from the decay of neutral pions produced by the inelastic…

高能天体物理现象 · 物理学 2015-05-19 Yutaka Ohira , Kohta Murase , Ryo Yamazaki

Several lines of evidence point to a relationship between gamma-ray bursts (GRBs) and the high mass stars that explode as supernovae. Arguments that GRB sources accelerate cosmic rays (CRs) are summarized. High-energy neutrino detection…

天体物理学 · 物理学 2009-11-10 C. D. Dermer , A. Atoyan

It is argued that there are three `origins' of cosmic rays; the origin of the particles, the origin of the energy, and the site of the acceleration. The evidence for each origin is discussed and a plausible synthesis outlined for the…

高能天体物理现象 · 物理学 2012-03-20 Luke O'C. Drury

Cosmic rays could be produced via shock acceleration powered by supernovae. The supernova hypothesis implies that each supernova injects on average some 1e50 erg in cosmic rays, while the shock acceleration model predicts a powerlaw cosmic…

高能天体物理现象 · 物理学 2017-11-22 Andrii Neronov

Star-forming and starburst galaxies are considered as one of the viable candidate sources of the high-energy cosmic neutrino background detected in IceCube. We revisit contributions of supernova remnants (SNRs) and hypernova remnants (HNRs)…

高能天体物理现象 · 物理学 2016-09-27 Di Xiao , Peter Mészáros , Kohta Murase , Zi-gao Dai

It is shown that the acceleration of particles by a powerful relativistic jet associated with the activity of a supermassive black hole in the Galactic center several million years ago may explain the observed cosmic ray spectrum at…

高能天体物理现象 · 物理学 2024-06-05 V. N. Zirakashvili , V. S. Ptuskin , S. I. Rogovaya

Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 10^15 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock…

We derive observational consequences of the hypothesis that cosmic rays (CR's) of energy $>10^{19}eV$ originate in the same cosmological objects producing gamma-ray bursts (GRB's). Inter-galactic magnetic fields $\gtrsim 10^{-12} G$ are…

天体物理学 · 物理学 2009-10-28 Jordi Miralda-Escude , Eli Waxman

New evidence that cosmic rays (hadronic component) are accelerated by supernova remnant shocks all the way from low energies to high energies, has come from recent works combining gamma-ray observations in the sub-GeV to TeV domain on the…

高能天体物理现象 · 物理学 2015-10-09 Stefano Gabici , Thierry Montmerle

An overview is given on the present status of the understanding of the origin of galactic cosmic rays. Recent measurements of charged cosmic rays and photons are reviewed. Their impact on the contemporary knowledge about the sources and…

天体物理学 · 物理学 2009-09-29 Joerg R. Hoerandel

One century ago Viktor Hess carried out several balloon flights that led him to conclude that the penetrating radiation responsible for the discharge of electroscopes was of extraterrestrial origin. One century from the discovery of this…

高能天体物理现象 · 物理学 2015-06-18 Pasquale Blasi

Galactic cosmic rays (CRs) are accelerated at the forward shocks of supernova remnants (SNRs) via diffusive shock acceleration (DSA), an efficient acceleration mechanism that predicts power-law energy distributions of CRs. However,…

高能天体物理现象 · 物理学 2021-11-24 Rebecca Diesing , Damiano Caprioli