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Ultra-high-energy (UHE) cosmic rays (CRs) of energies $\sim (10^{18}-10^{20})~{\rm eV}$, accelerated in violent astrophysical environments, interact with cosmic background radiation fields via photo-hadronic processes, leading to strong…

High Energy Astrophysical Phenomena · Physics 2021-11-24 Ellis R. Owen , Qin Han , Kinwah Wu , Y. X. Jane Yap , Pooja Surajbali

In these three lectures I discuss the present status of high-energy astroparticle physics including Ultra-High-Energy Cosmic Rays (UHECR), high-energy gamma rays, and neutrinos. The first lecture is devoted to ultra-high-energy cosmic rays.…

High Energy Physics - Phenomenology · Physics 2010-10-14 D. Semikoz

We use a multimessenger approach to constrain realistic mixed composition models of ultrahigh energy cosmic ray sources using the latest cosmic ray, neutrino, and gamma-ray data. We build on the successful Unger-Farrar-Anchordoqui 2015…

High Energy Astrophysical Phenomena · Physics 2019-11-20 Marco Stein Muzio , Michael Unger , Glennys R. Farrar

We study the effects that the diffusion of the cosmic rays in the magnetic field of the Local Supercluster can have on the spectrum of a nearby extragalactic source at ultrahigh energies. We find that the strong enhancement of the flux…

High Energy Astrophysical Phenomena · Physics 2019-05-22 Silvia Mollerach , Esteban Roulet

We review basic constraints on the acceleration of ultra-high-energy (UHE) cosmic rays (CRs) in astrophysical sources, namely the geometrical (Hillas) criterion and restrictions from radiation losses in different acceleration regimes. Using…

Astrophysics · Physics 2014-11-18 Ksenia Ptitsyna , Sergey Troitsky

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

The recently observed ultra-high energy (UHE) cosmic rays beyond the Greisen-Zatsepin-Kuzmin bound can be explained by the decays of some superheavy $X$ particles forming a part of dark matter in our universe. We consider various discrete…

High Energy Physics - Phenomenology · Physics 2009-09-29 K. Hamaguchi , Yasunori Nomura , T. Yanagida

In theories with large extra dimensions, constraints from cosmology lead to non-trivial lower bounds on the fundamental scale M_F, corresponding to upper bounds on the radii of the compact extra dimensions. These constraints are especially…

High Energy Physics - Phenomenology · Physics 2008-11-26 Lawrence J. Hall , David Smith

We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrating on the experimental results obtained so far and on what, from these results, can be inferred about the sources of UHECRs.

Astrophysics · Physics 2007-05-23 Daniel De Marco

Many attempts have been made to provide catalogs of potential sources of ultra-high energy cosmic ray (UHECR) particles based on various astronomical tracers, such as observed radio or gamma-ray emission. A closer look reveals, however,…

High Energy Astrophysical Phenomena · Physics 2019-09-04 Jörg P. Rachen , Björn Eichmann

A flux of extra-terrestrial neutrinos at energies $\gg10^{15}$ eV has the potential to serve as a cosmological probe of the high-energy universe as well as tests of fundamental particle interactions. Cosmogenic neutrinos, produced from the…

High Energy Astrophysical Phenomena · Physics 2018-07-25 Andres Romero-Wolf , Maximo Ave

A new infinite family of examples of finite non-bicolorable configurations of rays in Hilbert space is described. Such configurations appear in the analysis of quantum mechanics in terms of Bell's inequalities and Kochen-Specker theorem and…

Quantum Physics · Physics 2015-05-13 Artur Ruuge

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…

High Energy Physics - Phenomenology · Physics 2014-11-17 Alejandro Ibarra , Ramon Toldra

Top-down models for the origin of ultra high energy cosmic rays (UHECR's) propose that these events are the decay products of relic superheavy metastable particles, usually called $X$ particles. These particles can be produced in the…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. H. Campos , L. L. Lengruber , H. C. Reis , R. Rosenfeld , R. Sato

We find stringent upper bound on the momentum scale in noncommutative phase space of canonical type on the basis of studies of perihelion shift of the Mercury planet with taking into account features of description of motion of macroscopic…

High Energy Physics - Theory · Physics 2019-09-04 Kh. P. Gnatenko , V. M. Tkachuk

Recent data from the Pierre Auger Observatory has revealed the presence of a large-scale dipole in the arrival direction distribution of ultra-high energy cosmic rays (UHECR). In this work, we build up an understanding of the diffusive…

High Energy Astrophysical Phenomena · Physics 2021-03-09 Rodrigo Guedes Lang , Andrew M. Taylor , Vitor de Souza

The gamma-ray burst (GRB) model for production of ultra-high-energy cosmic-rays (UHECRs) is based on the hypothesis that GRBs arise from the dissipation of the kinetic energy of relativistic fireballs at cosmological distances. Recent GRB…

Astrophysics · Physics 2009-10-31 E. Waxman

In the current paper we consider an inverse boundary value problem of electromagnetism in a nonlinear Kerr medium. We show the unique determination of the electromagnetic material parameters and the nonlinear susceptibility parameters of…

Analysis of PDEs · Mathematics 2020-09-15 Yernat M. Assylbekov , Ting Zhou

Measurements of Ultra-High Energy Cosmic Rays achieved remarkable progress in the last 10 years. Physicists, gathered from around the world in the symposium UHECR-2012 held at CERN on February 13-16 2012, reported their most up-to-date…

High Energy Astrophysical Phenomena · Physics 2015-06-15 M. Fukushima

A dipole anisotropy in ultra-high-energy cosmic ray (UHECR) arrival directions, of extragalactic origin, is now firmly established at energies E > 8 EeV. Furthermore, the UHECR angular power spectrum shows no power at smaller angular scales…

High Energy Astrophysical Phenomena · Physics 2024-05-01 Teresa Bister , Glennys R. Farrar