Results 51 to 60 of about 1,204 (229)
Magnetogenesis in a Collisionless Plasma: From Weibel Instability to Turbulent Dynamo
We report on a first-principles numerical and theoretical study of plasma dynamo in a fully kinetic framework. By applying an external mechanical force to an initially unmagnetized plasma, we develop a self-consistent treatment of the generation of “seed”
Muni Zhou +4 more
doaj +1 more source
Influence of structured extragalactic magnetic fields on the propagation of UHECRs
The origin of the highest energy cosmic rays (UHECRs, E ≥ $10^19$ eV) remains a mystery. The Pierre Auger experiment will collect an unprecendented statistics at those energies, and therefore allow to detect potential sources. We discuss the influence of extragalactic magnetic fields, which are still poorly known, on the propagation of UHECRs and ...
Armengaud, E.
openaire +2 more sources
Extragalactic Magnetic Field and the Highest Energy Cosmic Rays [PDF]
11 pages with 3 postscript figures; LaTeX with AASTeX macros; uuencoded 3 .eps figures; submitted to the ApJL; a postscript version of the paper also available at http://astro.uchicago.edu/home/web/sjlee/pub ...
Sangjin Lee +2 more
openalex +3 more sources
Constraints on the Intergalactic Magnetic Field Using Fermi-LAT and H.E.S.S. Blazar Observations
Magnetic fields in galaxies and galaxy clusters are believed to be the result of the amplification of intergalactic seed fields during the formation of large-scale structures in the universe.
F. Aharonian +137 more
doaj +1 more source
Recently CRPropa 2.0 has been released as a public software package to simulate the extragalactic propagation of ultra-high energy nuclei. It includes deflections by extragalactic magnetic fields and all relevant interactions with ambient photon ...
Nierstenhoefer Nils +6 more
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Fast Radio Bursts as Probes of Magnetic Fields in Galaxies at z < 0.5
We present a sample of nine fast radio bursts (FRBs) from which we derive magnetic field strengths of the host galaxies represented by normal, z < 0.5 star-forming galaxies with stellar masses M _* ≈ 10 ^8 –10 ^10.5 M _⊙ .
Alexandra G. Mannings +8 more
doaj +1 more source
On irregularities in the cosmic ray spectrum of \(10^{16}-10^{18}\) eV range
Existing small, medium and large arrays for the study of cosmic rays of ultra-high energies are aimed for obtaining information about our galaxy and extragalactic space, namely to search and study astronomical objects that produce the flux of ...
Stanislav P. Knurenko, Igor S. Petrov
doaj +1 more source
Turbulence in the interstellar medium [PDF]
Turbulence is ubiquitous in the insterstellar medium and plays a major role in several processes such as the formation of dense structures and stars, the stability of molecular clouds, the amplification of magnetic fields, and the re-acceleration and ...
Chian, A. C. -L. +9 more
core +1 more source
Sensitivity of Cross-Correlation Studies by Using Xmax Information
The investigation about cosmic-ray sources through the study of the arrival direction of the particles is completely dependent on primary mass compositions.
Cynthia V. Ventura +3 more
doaj +1 more source
CRPropa high statistics simulations for UHECR anisotropy studies [PDF]
Despite the great progress made by modern cosmic ray observatories, the origin and acceleration mechanism of ultra-high-energy cosmic rays (UHECRs) remains unsolved problems to this day.
Rossoni Simone, Sigl Günter
doaj +1 more source

