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相关论文: Gamma Rays from Dark Matter

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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

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

Annihilation of clumped superheavy dark matter provides an interesting explanation for the origin of ultrahigh energy cosmic rays. The predicted anisotropy signal provides a unique signature for this scenario.

天体物理学 · 物理学 2009-11-07 R. Dick , P. Blasi , E. W. Kolb

A number of signals involving charged cosmic rays and high-energy photons have been interpreted as being due to annihilating dark matter. This article provides an overview of the experimental evidence and discusses in particular detections…

天体物理学 · 物理学 2007-05-23 U. Schwanke

The origin of Galactic cosmic rays (with energies up to 10^15 eV) remains unclear, though it is widely believed that they originate in the shock waves of expanding supernova remnants. Currently the best way to investigate their acceleration…

天体物理学 · 物理学 2012-08-27 The H. E. S. S. Collaboration , : , F. A. Aharonian

The article gives a brief overview, aimed at nonspecialists, about the goals and selected recent results of the detection of very-high energy gamma-rays (energies above 100 GeV) with ground based detectors. The stress is on the physics…

天体物理学 · 物理学 2009-09-25 R. Plaga

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

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

Gamma-ray bursts are known to be sources of high-energy gamma rays, and are likely to be sources of high-energy cosmic rays and neutrinos. Following a short review of observations of GRBs at multi-MeV energies and above, the physics of…

天体物理学 · 物理学 2007-05-23 Charles D. Dermer

It is commonly accepted that high energy cosmic rays up to $10^{19}$ eV can be produced in catastrophic astrophysical processes. However the source of a few observed events with higher energies remains mysterious. We propose that they may…

高能物理 - 唯象学 · 物理学 2025-01-30 E. V. Arbuzova

We discuss the possibility of observing ultra high energy cosmic ray sources inhigh energy gamma rays. Protons propagating away from their accelerators produce secondary electrons during interactions with cosmic microwave background…

天体物理学 · 物理学 2008-11-26 Stefano Gabici , Felix A. Aharonian

We consider decaying dark matter with masses $10^{7} \lesssim M \lesssim 10^{16}$ GeV, as a source of ultra-high energy (UHE) gamma rays. Using recent limits on UHE gamma-ray flux for energies $E_\gamma > 2 \cdot 10^{14}$ eV, provided by…

高能天体物理现象 · 物理学 2016-10-05 O. E. Kalashev , M. Yu. Kuznetsov

Bright gamma-ray flares observed from sources far beyond our Galaxy are best explained if enormous amounts of energy are liberated by black holes. The highest-energy particles in nature--the ultra-high energy cosmic rays--cannot be confined…

高能天体物理现象 · 物理学 2010-01-13 Charles D. Dermer , Govind Menon

During the last decades, increasingly precise astronomical observations of the Galactic Centre (GC) region at radio, infrared, and X-ray wavelengths laid the foundations to a detailed understanding of the high energy astroparticle physics…

高能天体物理现象 · 物理学 2015-05-25 Christopher van Eldik

Superheavy (SH) quasistable particles generated in the Early Universe could be responsable for Ultra High Energy Cosmic Rays (UHECR) and be a component of Cold Dark Matter (CDM) in the universe. These particles are likely to cluster in the…

天体物理学 · 物理学 2009-10-31 Pasquale Blasi

We argue that gamma-ray bursts (GRBs) may be the origin of the cosmic gamma-ray background radiation observed in GeV range. It has theoretically been discussed that protons may carry a much larger amount of energy than electrons in GRBs,…

天体物理学 · 物理学 2009-10-31 Tomonori Totani

Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such…

高能物理 - 唯象学 · 物理学 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

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 possibility that the Fermi scale is the only fundamental energy scale of Nature is under serious consideration at present, yet cosmic rays may already have provided direct evidence of new physics at a much higher scale. The recent…

高能物理 - 唯象学 · 物理学 2016-11-03 Subir Sarkar

Cosmic ray nuclei, cosmic ray electrons with energy above a few GeV, and the diffuse gamma-ray background radiation (GBR) above a few MeV, presumed to be extragalactic, could all have their origin or residence in our galaxy and its halo.…

天体物理学 · 物理学 2007-05-23 Arnon Dar , A. De Rújula , Nikos Antoniou
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