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相关论文: Ultra-high-energy cosmic rays from relic topologic…

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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

The topological defect scenario of origin of the observed highest energy cosmic rays is reviewed. Under a variety of circumstances, topological defects formed in the early Universe can be sources of very massive particles in the Universe…

天体物理学 · 物理学 2009-10-30 Pijushpani Bhattacharjee

Cosmic rays of energy higher than 10^19 eV may be explained by topological defects produced in the early stages of universe. Two suitable alternatives are: necklaces formed by magnetic monopoles connected by strings, and vortons which are…

天体物理学 · 物理学 2010-11-11 Luis Masperi , Milva Orsaria

We argue that due to various restrictions cosmic strings and monopole-string networks are not likely to produce the observed flux of ultra-high energy cosmic rays (UHECR). Among the topological defects studied so far, the most promising…

天体物理学 · 物理学 2016-08-25 V. S. Berezinsky , P. Blasi , A. Vilenkin

Cosmic necklaces are hybrid topological defects consisting of monopoles and strings, with two strings attached to each monopole. We argue that the cosmological evolution of necklaces may significantly differ from that of cosmic strings. The…

天体物理学 · 物理学 2009-10-30 Veniamin Berezinsky , Alexander Vilenkin

Ultra High Energy Cosmic Rays (UHECR) can be a signal from very early (post-inflationary) Universe. At this cosmological epoch Topological Defects (TD) and long-lived suprheavy (SH) particles are expected to be naturally and effectively…

天体物理学 · 物理学 2009-10-31 V. Berezinsky

The sky distribution of cosmic rays with energies above the 'GZK cutoff' holds important clues to their origin. The AGASA data, although consistent with isotropy, shows evidence for small-angle clustering, and it has been argued that such…

天体物理学 · 物理学 2011-02-16 N. Wyn Evans , Francesc Ferrer , Subir Sarkar

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 current status of Ultra High Energy Cosmic Rays (UHECR) is reviewed, with emphasis given to theoretical interpretation of the observed events. The galactic and extragalactic origin, in case of astrophysical sources of UHE particles,…

高能物理 - 唯象学 · 物理学 2009-10-31 V. Berezinsky

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

Using the propagation of ultra high energy nucleons, photons and electrons in the universal radiation backgrounds, we obtain limits on the luminosity of topological defects scenarios for the origin of the highest energy cosmic rays. The…

天体物理学 · 物理学 2011-05-12 R. J. Protheroe , Todor Stanev

We show that ``top-down'' mechanisms of Ultra-High Energy Cosmic Rays which involve heavy relic particle-like objects predict Galactic anisotropy of highest energy cosmic rays at the level of minimum $\sim 20%$. This anisotropy is large…

高能物理 - 唯象学 · 物理学 2010-11-30 S. L. Dubovsky , P. G. Tinyakov

Recent international efforts have brought us closer to unveiling the century old mystery of the origin of cosmic rays. Cosmic ray, gamma ray, and neutrino observatories are reaching the necessary sensitivity to study the highest energy…

高能天体物理现象 · 物理学 2012-03-16 Angela V. Olinto

The origin of the highest-energy cosmic rays remains a mystery. The lack of a high energy cutoff in the cosmic ray spectrum together with an apparently isotropic distribution of arrival directions have strongly constrained most models…

天体物理学 · 物理学 2010-12-03 A. V. Olinto

A sequence of two symmetry breaking transitions in the early universe may produce monopoles whose flux is confined into two strings each, which thus assemble into "necklaces" with monopoles as beads. Such "cosmic necklaces" have been…

天体物理学 · 物理学 2010-05-25 Jose J. Blanco-Pillado , Ken D. Olum

It is shown that Eddington-like accretion event in the Galactic center several million years ago and particle acceleration at accompanying shocks and jets could explain the observed cosmic ray spectrum at energies above 1 PeV. Cosmic ray…

高能天体物理现象 · 物理学 2026-02-02 V. N. Zirakashvili , S. I. Rogovaya

The decay of very heavy metastable relics of the Early Universe can produce ultra-high energy cosmic rays (UHECRs) in the halo of our own Galaxy. On distance scales of the order of the halo size, energy losses are negligible---no…

天体物理学 · 物理学 2011-08-23 Pasquale Blasi , Ravi Sheth

The electromagnetic decay and final annihilation of magnetic monopole-antimonopole pairs formed in the early universe has been proposed as a possible mechanism to produce the highest energy cosmic rays. We show that for a monopole abundance…

天体物理学 · 物理学 2009-10-31 J. J. Blanco-Pillado , Ken D. Olum

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

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
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