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Related papers: Cosmic Ray Origin, Acceleration and Propagation

200 papers

In 1990's Very High Energy Gamma-ray Astrophysics has dramatically advanced due to the Imaging Air \v{C}erenkov Telescopes(IACTs). After the first detection of TeV gamma-ray emission from the Crab nebula in 1989, several type of TeV…

Astrophysics · Physics 2009-11-07 Toru Tanimori

We revisit the idea that the Galactic center (GC) is the dominant source of Galactic cosmic rays (GCRs), based on a series of new observational evidence. A unified model is proposed to explain the new phenomena of GCRs and $\gamma$-rays…

High Energy Astrophysical Phenomena · Physics 2013-01-24 Yiqing Guo , Zhaoyang Feng , Qiang Yuan , Cheng Liu , Hongbo Hu

Cosmic rays represent one of the most important energy transformation processes of the universe. They bring information about the surrounding universe, our galaxy, and very probably also the extragalactic space, at least at the highest…

High Energy Astrophysical Phenomena · Physics 2022-06-07 G. Di Sciascio , INFN - Roma Tor Vergata

Cosmic rays and related measurements: IceTop overview; IceTop calibration; Cosmic ray composition; Air shower measurements; Studies of cosmic ray muons; Studies of PeV gamma rays; Cosmic ray anisotropy; Forbush decrease; Submitted papers to…

High Energy Astrophysical Phenomena · Physics 2012-08-27 The IceCube Collaboration

We discuss the relation between cosmic-ray induced interstellar gamma-ray and radio emission from our Galaxy, and emphasize the importance of their parallel study. We give an overview of results from Fermi-LAT on the interstellar gamma-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Elena Orlando , Andrew W. Strong

The recent success of a proposal from some time ago to explain the spectrum of cosmic rays allows some strong conclusions to be made on the physics of supernovae: In the context of this specific proposal to explain the origin of cosmic…

Astrophysics · Physics 2007-05-23 Peter L. Biermann , Sergej Moiseenko , Samvel Ter-Antonyan , Ana Vasile

We give an outline of possible extragalactic explanations of the highest energy cosmic ray events. We give a classification of the possible particles which could have caused the events and try to find suitable sources for each class. In…

Astrophysics · Physics 2011-04-15 Joerg P. Rachen

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,…

Recent efforts in cosmic ray (CR) confinement and transport theory are discussed. Three problems are addressed as being crucial for understanding the present day observations and their possible telltale signs of the CR origin. The first…

High Energy Astrophysical Phenomena · Physics 2016-10-11 M. A. Malkov

Cosmic rays at the Earth include a secondary component originating in collisions of primary particles with the diffuse interstellar gas. The secondary cosmic rays are relatively rare but carry important information on the Galactic…

The gamma-ray observations of molecular clouds associated with supernova remnants are considered one of the most promising ways to search for a solution of the problem of cosmic ray origin. Here we briefly review the status of the field,…

High Energy Astrophysical Phenomena · Physics 2015-12-16 S. Gabici , J. Krause , G. Morlino , L. Nava

We are constructing a model which aims to reproduce observational data of many kinds related to cosmic-ray origin and propagation: direct measurements of nuclei, antiprotons, electrons and positrons, gamma-rays, and synchrotron radiation.…

Astrophysics · Physics 2007-05-23 A. W. Strong , I. V. Moskalenko

We have studied the impact of cosmic-ray acceleration in SNR on the spectra of cosmic-ray nuclei in the Galaxy using a series expansion of the propagation equation, which allows us to use analytical solutions for part of the problem and an…

Astrophysics · Physics 2009-11-10 I. Buesching , A. Kopp , M. Pohl , R. Schlickeiser , C. Perrot , I. Grenier

In his Nobel Prize lecture Victor Hess urged that different instruments, working together, should be used to solve the problem of the origin of cosmic rays. I review some of the key developments that have opened up the new fields of direct…

Instrumentation and Methods for Astrophysics · Physics 2019-09-04 A A Watson

When examining the abundance of elements in the placid interstellar medium, a deep hollow between helium and carbon becomes apparent. Notably, the fragile light nuclei Lithium, Beryllium, and Boron (collectively known as LiBeB) are not…

High Energy Astrophysical Phenomena · Physics 2023-09-04 Carmelo Evoli , Ulyana Dupletsa

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

Highly relativistic jets from merger and accretion induced collapse of compact stellar objects, which may produce the cosmological gamma ray bursts (GRBs), are also very efficient and powerful cosmic ray accelerators. The expected…

Astrophysics · Physics 2007-05-23 Arnon Dar

This article is the write-up of a rapporteur talk given at the 34th ICRC in The Hague, Netherlands. It attempts to review the results and developments presented at the conference and associated to the vibrant field of ground-based gamma-ray…

High Energy Astrophysical Phenomena · Physics 2015-10-07 Marianne Lemoine-Goumard

Although several theories for the origin of cosmic rays in the region between the spectral `knee' and `ankle' exist, this problem is still unsolved. A variety of observations suggest that the transition from Galactic to extragalactic…

High Energy Astrophysical Phenomena · Physics 2018-06-06 Lukas Merten , Chad Bustard , Ellen G. Zweibel , Julia Becker Tjus

This paper has not yet been accepted for publication

Astrophysics · Physics 2010-01-15 M. Ave , P. J. Boyle , C. Hoeppner , J. Marshall , D. Muller
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