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Related papers: Ultra High Energy Cosmic Rays and Inflation

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There are two processes of matter creation after inflation that may be relevant to the resolution of the puzzle of cosmic rays observed with energies beyond GZK cut-off: 1) gravitational creation of superheavy (quasi)stable particles, and…

High Energy Physics - Phenomenology · Physics 2014-11-17 Vadim A. Kuzmin , Igor I. Tkachev

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…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. A. Kuzmin , I. I. Tkachev

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…

Astrophysics · Physics 2009-10-30 V. Berezinsky

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…

Astrophysics · Physics 2009-10-31 V. Berezinsky

The phase of inflationary expansion in the early universe produces superheavy relics in a mass window between 10^{12} GeV and 10^{14} GeV. Decay or annihilation of these superheavy relics can explain the observed ultrahigh energy cosmic…

High Energy Physics - Phenomenology · Physics 2009-11-11 R. Dick , K. M. Hopp , K. E. Wunderle

In inflationary cosmology, the particles constituting the Universe are created after inflation in the process of reheating due to the interaction with the oscillating inflaton field. We briefly review the basics of the slow reheating, and…

Astrophysics · Physics 2007-05-23 Lev Kofman

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…

High Energy Physics - Phenomenology · Physics 2014-11-17 V. Berezinsky

A continuous process of creation of particles is investigated as a possible connection between the inflationary stage with late cosmic acceleration. In this model, the inflationary era occurs due to a continuous and fast process of creation…

General Relativity and Quantum Cosmology · Physics 2016-04-27 Rafael C. Nunes

We discuss theoretical issues and experimental data that brought the ultra high energy cosmic rays in the list of Nature's greatest puzzles. After many years of research we still do not know how astrophysical acceleration processes can…

Astrophysics · Physics 2016-08-30 Todor Stanev

We study the gravitational production of super-Hubble-mass dark matter in the very early universe. We first review the simplest scenario where dark matter is produced mainly during slow roll inflation. Then we move on to consider the cases…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-04 Lingfeng Li , Tomohiro Nakama , Chon Man Sou , Yi Wang , Siyi Zhou

We review the physics of the highest energy cosmic rays. The discovery of their sources, still unknown, will reveal the most energetic astrophysical objects in the universe and could unveil new physics beyond the standard model of particle…

High Energy Astrophysical Phenomena · Physics 2017-11-30 Roberto Aloisio

Reheating is an important part of inflationary cosmology. It describes the production of Standard Matter particles after the phase of accelerated expansion. We give a review of the reheating process, focusing on an in-depth discussion of…

High Energy Physics - Theory · Physics 2011-02-03 Rouzbeh Allahverdi , Robert Brandenberger , Francis-Yan Cyr-Racine , Anupam Mazumdar

We conjecture that the highest energy cosmic rays beyond the Greisen-Zatsepin-Kuzmin cut-off may provide a unique window into the very early epoch of the Universe, namely, that of reheating after inflation, provided these cosmic rays are…

Astrophysics · Physics 2011-04-15 V. A. Kuzmin , V. A. Rubakov

It has been suggested that the origin of cosmic rays above the GZK limit might be explained by the decay of particles, X, with mass of the order of 10^{12} GeV. Generation of heavy particles from inflationary quantum fluctuations is a prime…

High Energy Physics - Phenomenology · Physics 2016-09-06 John McDonald

Cosmic rays of the highest energy, above the Greisen-Zatsepin-Kuzmin cut-off of the spectrum, may originate in decays of superheavy long-living X-particles. These particles may be produced in the early Universe from vacuum fluctuations…

High Energy Physics - Phenomenology · Physics 2009-10-31 V. A. Kuzmin , I. I. Tkachev

In the inflationary scenario all the matter constituting the universe was created from the process of reheating after inflation. Recent development of the theory of reheating is briefly reviewed. The list of topics includes elementary…

Astrophysics · Physics 2007-05-23 Lev Kofman

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…

Astrophysics · Physics 2010-12-03 A. V. Olinto

Top-down models assume that the still unexplained Ultra High Energy Cosmic Rays (UHECR's) are the decay products of superheavy particles. Such particles may have been produced by one of the post-inflationary reheating mechanisms and may…

Astrophysics · Physics 2009-11-10 A. H. Campos , J. M. F. Maia , R. Rosenfeld

The primary ultrahigh energy particles which produce giant extensive air showers in the Earth's atmosphere present an intriguing mystery from two points of view: (1) How are these particles produced with such astounding energies, eight…

Astrophysics · Physics 2007-05-23 F. W. Stecker

We discuss the gravitational creation of superheavy particles $\chi$ in an inflationary scenario with a quartic potential and a non-minimal coupling between the inflaton $\varphi$ and the Ricci curvature: $\xi \varphi^2 R/2$. We show that…

High Energy Physics - Phenomenology · Physics 2020-10-14 E. Babichev , D. Gorbunov , S. Ramazanov , L. Reverberi
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