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Related papers: Ultra High Energy Cosmic Rays from the Local Void

200 papers

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…

Astrophysics · Physics 2015-06-24 Pasquale Blasi , Rainer Dick , Edward W. Kolb

Observations of cosmic rays with energies above ~ 4 x 10^{10} GeV have inspired several speculative suggestions concerning their origin. The crucial question is whether or not the spectrum exhibits the expected `GZK cutoff' at this energy…

High Energy Physics - Phenomenology · Physics 2011-02-16 Subir Sarkar

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

In this article we examine the question of whether the highest energy cosmic ray primaries could be ultra relativistic magnetic monopoles. The analysis is performed within the framework of large compact dimensions and TeV scale quantum…

High Energy Physics - Phenomenology · Physics 2009-10-31 Luis A. Anchordoqui , Thomas P. McCauley , Stephen Reucroft , John Swain

The connection between the arrival directions of ultrahigh energy cosmic rays by using the EAS array data and point galactic sources of radio-and gamma-radiations, pulsars,is sought. At the mean particle energy of 10^{19} eV the correlation…

Astrophysics · Physics 2007-05-23 A. A. Mikhailov

We give a brief overview of the current experimental and theoretical status of cosmic rays above ~10**17 eV. We focus on the role of large scale magnetic fields and on multi-messenger aspects linking charged cosmic ray with secondary…

Astrophysics · Physics 2009-11-11 Guenter Sigl

Substantial amount of information both on the source and on characteristics of intercepting magnetic fields is encoded in the distribution in arrival times, directions, and energies of charged ultra-high energy cosmic rays from discrete…

Astrophysics · Physics 2009-10-30 Guenter Sigl

We discuss the production of ultra high energy neutrinos coming from the propagation of ultra high energy cosmic rays and in the framework of top-down models for the production of these extremely energetic particles. We show the importance…

High Energy Astrophysical Phenomena · Physics 2016-03-21 Roberto Aloisio

Cosmic rays with energies exceeding $10^{20}\eV$ have been detected. The origin of these highest energy cosmic rays remains unknown. Established astrophysical acceleration mechanisms encounter severe difficulties in accelerating particles…

Astrophysics · Physics 2009-10-22 P. Bhattacharjee , G. Sigl

We briefly review the status of cosmic ray studies between $10^{14}$ eV and the highest observed energies, namely a few times $10^{20}$ eV. Because of the rather low incident fluxes in this energy range, the studies mostly rely on ground…

Astrophysics · Physics 2009-10-31 Murat Boratav , Alan A. Watson

The origin and composition of ultra-high energy cosmic rays (UHECRs) remain a mystery. The common lore is that UHECRs are deflected from their primary directions by the Galactic and extragalactic magnetic fields. Here we describe an…

High Energy Astrophysical Phenomena · Physics 2021-10-20 Andres Aramburo Garcia , Kyrylo Bondarenko , Alexey Boyarsky , Dylan Nelson , Annalisa Pillepich , Anastasia Sokolenko

The apparent lack of suitable astrophysical sources for cosmic rays with E > 10^{19.7} eV (UHECRs) is the "GZK Paradox". We argue that whatever mechanism produces them must also account for events down to ~10^{18.7} eV, including their…

Astrophysics · Physics 2007-05-23 Glennys R. Farrar , Tsvi Piran

The measurement of ultra-high energy cosmic rays is an unique way to study article interactions at energies which are well above the capability of current accelerators. Significant progress in this field has occurred during last years,…

High Energy Astrophysical Phenomena · Physics 2010-01-12 R. Smida

In this Letter we examine the arrival directions of the most energetic cosmic rays (E > 2 * 10^19 eV) detected by several air shower experiments. We find that data taken by different air shower arrays show positive correlations, indicating…

Astrophysics · Physics 2008-11-26 Todor Stanev , Peter Biermann , Jeremy Lloyd-Evans , Joerg Rachen , Alan Watson

We describe the current situation of the data on the highest energy particles in the Universe - the ultrahigh energy cosmic rays. The new results in the field come from the Telescope Array experiment in Utah, U.S.A. For this reason we…

High Energy Astrophysical Phenomena · Physics 2012-10-04 Todor Stanev

In this review we discuss the important progress made in recent years towards understanding the experimental data on cosmic rays with energies $\agt 10^{19}$ eV. We begin with a brief survey of the available data, including a description of…

High Energy Physics - Phenomenology · Physics 2010-01-15 Luis Anchordoqui , Thomas Paul , Stephen Reucroft , John Swain

A review of the status of the knowledge in the field of High-energy cosmic particles is presented. The spectrum, arrival direction distribution and composition measurements are summarized, together with some implications for the…

High Energy Astrophysical Phenomena · Physics 2020-12-21 Silvia Mollerach

We consider the recent results on UHECR (Ultra High Energy Cosmic Ray) composition and their distribution in the sky from ten EeV energy (the dipole anisotropy) up to the highest UHECR energies and their clustering maps: UHECR have been…

High Energy Astrophysical Phenomena · Physics 2018-10-05 Daniele Fargion , Pier Giorgio De Sanctis Lucentini , Maxim Yu. Khlopov

We report an estimation of the injected mass composition of ultra-high energy cosmic rays (UHECRs) at energies higher than 10 EeV. The composition is inferred from an energy-dependent sky distribution of UHECR events observed by the…

High Energy Astrophysical Phenomena · Physics 2024-07-04 Telescope Array Collaboration , R. U. Abbasi , Y. Abe , T. Abu-Zayyad , M. Allen , Y. Arai , R. Arimura , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , I. Buckland , B. G. Cheon , M. Chikawa , T. Fujii , K. Fujisue , K. Fujita , R. Fujiwara , M. Fukushima , G. Furlich , N. Globus , R. Gonzalez , W. Hanlon , N. Hayashida , H. He , R. Hibi , K. Hibino , R. Higuchi , K. Honda , D. Ikeda , N. Inoue , T. Ishii , H. Ito , D. Ivanov , A. Iwasaki , H. M. Jeong , S. Jeong , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , S. Kasami , S. Kawakami , K. Kawata , I. Kharuk , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , S. W. Kim , Y. Kimura , I. Komae , V. Kuzmin , M. Kuznetsov , Y. J. Kwon , K. H. Lee , B. Lubsandorzhiev , J. P. Lundquist , H. Matsumiya , T. Matsuyama , J. N. Matthews , R. Mayta , K. Mizuno , M. Murakami , I. Myers , K. H. Lee , S. Nagataki , K. Nakai , T. Nakamura , E. Nishio , T. Nonaka , H. Oda , S. Ogio , M. Onishi , H. Ohoka , N. Okazaki , Y. Oku , T. Okuda , Y. Omura , M. Ono , A. Oshima , H. Oshima , S. Ozawa , I. H. Park , K. Y. Park , M. Potts , M. S. Pshirkov , J. Remington , D. C. Rodriguez , C. Rott , G. I. Rubtsov , D. Ryu , H. Sagawa , R. Saito , N. Sakaki , T. Sako , N. Sakurai , D. Sato , K. Sato , S. Sato , K. Sekino , P. D. Shah , N. Shibata , T. Shibata , J. Shikita , H. Shimodaira , B. K. Shin , H. S. Shin , D. Shinto , J. D. Smith , P. Sokolsky , B. T. Stokes , T. A. Stroman , Y. Takagi , K. Takahashi , M. Takamura , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , K. Tanaka , M. Tanaka , Y. Tanoue , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , R. Tsuda , Y. Tsunesada , S. Udo , F. Urban , D. Warren , T. Wong , K. Yamazaki , K. Yashiro , F. Yoshida , Y. Zhezher , Z. Zundel

In this article we examine the hypothesis that the highest energy cosmic rays are complex nuclei from extragalactic sources. Under reasonable physical assumptions, we show that the nearby metally rich starburst galaxies (M82 and NGC 253)…

High Energy Physics - Phenomenology · Physics 2009-11-07 Luis Anchordoqui , Haim Goldberg , Stephen Reucroft , John Swain
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