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相关论文: The Ultra High Energy Cosmic Ray Spectrum from Rel…

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It has been speculated that the recently detected ultra-high energy cosmic rays may originate from the decays of relic particles with mass of order $10^{12}$ GeV clustered in the halo of our Galaxy. This hypothesis can be tested through…

高能物理 - 唯象学 · 物理学 2014-11-17 Subir Sarkar , Ramon Toldra

We calculate the cosmic ray spectrum of ultra high energy neutralinos that one should expect provided that the observed ultra high energy cosmic rays are produced by the decay of superheavy particles X, M_X>10^{12} GeV, in supersymmetric…

高能物理 - 唯象学 · 物理学 2014-11-17 Alejandro Ibarra , Ramon Toldra

The energy losses and spectra of Ultra High Energy Cosmic Rays (UHECR) are calculated for protons as primary particles. The attention is given to the energy losses due to electron-positron production in collisions with the microwave 2.73 K…

高能物理 - 唯象学 · 物理学 2007-05-23 V. Berezinsky , A. Z. Gazizov , S. I. Grigorieva

We investigate the possibility that ultra-high energy cosmic rays (UHECRs) originate from the annihilation of relic superheavy (SH) dark matter in the Galactic halo. In order to fit the data on UHECRs, a cross section of $<\sigma_Av>\sim…

天体物理学 · 物理学 2015-06-24 Pasquale Blasi , Rainer Dick , Edward W. Kolb

The harmonic analysis of anisotropy of Ultra High Energy Cosmic Rays is performed for the Dark Matter halo model. In this model the relic superheavy particles comprise part of the Dark Matter and are concentrated in the Galactic halo. The…

天体物理学 · 物理学 2016-08-30 V. Berezinsky , A. Mikhailov

In this talk, I present the last and more precise results obtained in the computation of the final spectra of stable particles issued from the decay of super-heavy X particles (M_X ~ 10^21 to 10^25 eV). Such very energetic decay products,…

高能物理 - 唯象学 · 物理学 2007-05-23 Barbot Cyrille

In this paper we briefly discuss the problem of the origin of Ultra High Energy Cosmic Rays in the framework of Top-Down models. We show that, for high energy of decays and in a wide range of spectra of injected protons, their extragalactic…

天体物理学 · 物理学 2007-05-23 A. G. Doroshkevich , P. D. Naselsky

The supersymmetric evolution of the fragmentation functions (or timelike evolution) within N=1 $QCD$ is discussed and predictions for the fragmentation functions of the theory (into final protons) are given. We use a backward running of the…

高能物理 - 唯象学 · 物理学 2014-11-17 Claudio Coriano' , Alon E. Faraggi

In this work we present a detailed computation of the spectra of UHECR in the top-down scenario. We compare the spectra of hadrons obtained by two different methods in QCD and supersymmetric (SUSY) QCD with large primary energies $\sqrt{s}$…

天体物理学 · 物理学 2009-11-10 R. Aloisio , V. Berezinsky , M. Kachelriess

The origin of Ultra--High Energy ($E \gsim 10^{20}$ eV) Cosmic Rays (UHECR) remains mysterious. I discuss ``top--down'' models, where UHECR originate from the decay of very massive, long--lived particles. I summarize the calculation of the…

高能物理 - 唯象学 · 物理学 2014-11-17 Manuel Drees

We consider the possibility that ultra-high energy cosmic rays originate from the annihilation of relic superheavy dark-matter particles. We find that a cross section of <sigma_A v> ~ 10^{-26}cm^2 (M_X/10^{12}GeV)^{3/2} is required to…

天体物理学 · 物理学 2015-06-24 Pasquale Blasi , Rainer Dick , Edward W. Kolb

Decaying superheavy particles can be produced by Topological Defects or, in case they are quasi-stable, as relics from the early Universe. The decays of these particles can be the sources of observed Ultra High Energy Cosmic Rays ($E \sim…

天体物理学 · 物理学 2009-10-30 V. Berezinsky

If decays of superheavy relic particles in the galactic halo are responsible for ultrahigh-energy cosmic rays, these particles must be clustered to account for small-scale anisotropy in the AGASA data. We show that the masses of such…

天体物理学 · 物理学 2014-10-13 Alexander Kusenko , Vadim A. Kuzmin

The origin of the ultra high energy cosmic rays via annihilation of heavy stable, fermions "f", of the cosmological dark matter (DM) is studied. The particles in question are supposed to be created by the scalaron decays in $R^2$ modified…

高能物理 - 唯象学 · 物理学 2024-05-22 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

Simple arguments concerning power and acceleration efficiency show that ultra-high energy cosmic rays (UHECRS) with energies >~ 10^{19} eV could originate from GRBs. Neutrons formed through photo-pion production processes in GRB blast waves…

天体物理学 · 物理学 2009-11-06 C. D. Dermer

The current status of origin of Ultra High Energy Cosmic Rays (UHECR) is reviewed, with emphasis given to elementary particle solutions to UHECR problem, namely to Topological Defects and Super-Heavy Dark Matter (SHDM) particles. The relic…

高能物理 - 唯象学 · 物理学 2014-11-17 V. Berezinsky

Several explanations for the existence of Ultra High Energy Cosmic Rays invoke the idea that they originate from the decay of massive particles created in the reheating following inflation. It has been suggested that the decay products can…

天体物理学 · 物理学 2009-10-31 Gustavo Medina Tanco , Alan A. Watson

The highest energy cosmic rays, above the Greisen-Zatsepin-Kuzmin cut-off of cosmic ray spectrum, may be produced in decays of superheavy long-living X-particles. We conjecture that these particles may be produced naturally in the early…

高能物理 - 唯象学 · 物理学 2008-11-26 V. A. Kuzmin , I. I. Tkachev

Several explanations for the existence of Ultra High Energy Cosmic Rays (UHECR) invoke the idea that they originate from the decay of massive particles created in the reheating following inflation. It has been suggested that the decay…

天体物理学 · 物理学 2007-05-23 Gustavo Medina Tanco , Alan A. Watson

We consider the astrophysical implications of the diffusion equation solution for Ultra-High Energy Cosmic Rays (UHECR) in the expanding universe, obtained in paper I (V.Berezinsky & A.Gazizov, ApJ 643 (2006) 8). The UHECR spectra are…

天体物理学 · 物理学 2009-03-19 V. Berezinsky , A. Z. Gazizov
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