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Related papers: Cosmic Rays from Decaying Vortons

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A simple model is exhibited in which the remnant density of charged vortons is used to provide candidates for explaining the observed ultra high energy cosmic rays (above $10^{20}$ eV). These vortons would be accelerated in active galaxies…

High Energy Physics - Phenomenology · Physics 2011-05-23 Silvano Bonazzola , Patrick Peter

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…

High Energy Physics - Phenomenology · Physics 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

It has been speculated that cosmic string networks could produce ultra-high energy cosmic rays as a by-product of their evolution. By making use of recent work on the evolution of such networks, it will be shown that the flux of cosmic rays…

High Energy Physics - Phenomenology · Physics 2014-11-17 A. J. Gill , T. W. B. Kibble

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…

Astrophysics · Physics 2009-10-30 Pijushpani Bhattacharjee

We show that the flux of the high-energy cosmic ray positrons observed near Earth is that expected from the decay of mesons produced by the primary cosmic rays (CRs) in the local interstellar medium.

High Energy Astrophysical Phenomena · Physics 2015-10-16 Shlomo Dado , Arnon Dar

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Giovanni Morlino

Topological defects, particularly cosmic strings, can provide a mechanism to produce particles with energies of the order 10^21 eV and higher. Here, we report on order of magnitude calculations of fluxes from a cosmic string network which…

High Energy Physics - Phenomenology · Physics 2007-05-23 U. F. Wichoski , R. H. Brandenberger , J. H. MacGibbon

We re-visit the production of cosmic rays by cusps on cosmic strings. If a scalar field (``Higgs'') has a linear interaction with the string world-sheet, such as would occur if there is a bosonic condensate on the string, cusps on string…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Tanmay Vachaspati

It is proposed that the highest energy $\sim 10^{20}$eV cosmic ray primaries are protons, decay products of a long-lived progenitor which has propagated from typically $\sim 100$Mpc. Such a scenario can occur in e.g. SU(15) grand…

Astrophysics · Physics 2015-06-24 Paul H. Frampton , Bettina Keszthelyi , Y. Jack Ng

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…

Astrophysics · Physics 2007-05-23 A. G. Doroshkevich , P. D. Naselsky

Decaying topological defects, in particular cosmic strings, can produce a significant flux of high energy neutrinos, photons and cosmic rays. According to the prevailing understanding of cosmic string dynamics in an expanding Universe, the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ubi F. Wichoski , Jane H. MacGibbon , Robert H. Brandenberger

It is proposed that the highest energy $\sim 10^{20}$eV cosmic ray primaries are protons, decay products of a long-lived progenitor whose high kinetic energy arises from decay of a distant (cosmological) superheavy particle, G. Such a…

Astrophysics · Physics 2007-05-23 Paul H. Frampton

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…

High Energy Physics - Phenomenology · Physics 2024-05-22 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

We investigate the cosmological consequences of particle physics theories that admit stable loops of superconducting cosmic string - {\it vortons}. General symmetry breaking schemes are considered, in which strings are formed at one energy…

High Energy Physics - Phenomenology · Physics 2009-10-28 R. Brandenberger , B. Carter , A. -C. Davis , M. Trodden

The bulk of observed ultrahigh energy cosmic rays could be light or heavier elements, and originate from an either steady or transient population of sources. This leaves us with four general categories of sources. Energetic requirements set…

High Energy Astrophysical Phenomena · Physics 2016-11-21 Ke Fang , Kumiko Kotera

In this paper we review the hypothesis that a considerable part of the cosmic ray flux observed above about $10^{19}\eV$ may be produced by decaying or annihilating topological defects left over from phase transitions in the early universe…

Astrophysics · Physics 2010-11-01 G. Sigl

Considerations of the collision losses for protons traversing the 2.7 K black body microwave radiation field have led to the conclusion that the highest energy cosmic rays, those observed at $\geq 10^{20}$ eV, must come from sources within…

Astrophysics · Physics 2011-02-21 Elihu Boldt , Pranab Ghosh

Ultra-high energy cosmic rays are mostly charged particles and they are therefore deflected by magnetic fields on their path from their sources to Earth. An interesting phenomenon arising from these deflections is the appearance of multiple…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Geraldina Golup , Diego Harari , Silvia Mollerach , Esteban Roulet

The search for the origin of cosmic rays is a quest of almost a hundred years. A recent theoretical proposal gives quantitative predictions, which can be tested with data. Specifically, it has been suggested, that all cosmic rays can be…

Astrophysics · Physics 2016-08-30 Peter L. Biermann

We calculate the flux of ultra high energy photons from individual ordinary (i.e. non-superconducting) cosmic strings and compare the results with the sensitivity of current and proposed TeV and EeV telescopes. Our calculations give only…

Astrophysics · Physics 2009-10-22 Jane H. MacGibbon , Robert H. Brandenberger
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