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Cosmic ray studies, in particular UHECR, can be in general supported by a directional, easy deployable, simple and robust detector. The design of this detector is based on the time of flight between two parallel tiles of scintillator, to…

Astrophysics · Physics 2008-11-26 M. Iori , A. Sergi

We investigate a possible new technique for microwave measurements of ultra-high energy cosmic ray (UHECR) extensive air showers which relies on detection of expected continuum radiation in the microwave range, caused by free-electron…

The origin and nature of the cosmic rays is still uncertain. However, a big progress has been achieved in recent years due to the good quality data provided by current and recent cosmic-rays observatories. The cosmic ray flux decreases very…

High Energy Astrophysical Phenomena · Physics 2021-02-09 A. D. Supanitsky

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory observes atmospheric showers produced by incident gamma rays and cosmic rays with energy from 300 GeV to more than 100 TeV. A crucial phase in analyzing gamma-ray sources using…

High Energy Astrophysical Phenomena · Physics 2022-08-25 R. Alfaro , C. Alvarez , J. D. Álvarez , J. R. Angeles Camacho , J. C. Arteaga-Velázquez , D. Avila Rojas , H. A. Ayala Solares , R. Babu , E. Belmont-Moreno , C. Brisbois , K. S. Caballero-Mora , T. Capistrán , A. Carramiñana , S. Casanova , O. Chaparro-Amaro , U. Cotti , J. Cotzomi , S. Coutiño de León , E. De la Fuente , C. de León , R. Diaz Hernandez , B. L. Dingus , M. A. DuVernois , M. Durocher , J. C. Díaz-Vélez , R. W. Ellsworth , K. Engel , C. Espinoza , K. L. Fan , M. Fernández Alonso , N. Fraija , D. Garcia , J. A. García-González , F. Garfias , M. M. González , J. A. Goodman , J. P. Harding , S. Hernandez , B. Hona , D. Huang , F. Hueyotl-Zahuantitla , P. Hüntemeyer , A. Iriarte , A. Jardin-Blicq , V. Joshi , S. Kaufmann , G. J. Kundem A. Lara , W. H. Lee , J. Lee , H. León Vargas , J. T. Linnemann , G. Luis-Raya , J. Lundeen , K. Malone , V. Marandon , O. Martinez , J. Martínez-Castro , J. A. Matthews , P. Miranda-Romagnoli , J. A. Morales-Soto , A. Nayerhoda , L. Nellen , M. U. Nisa , R. Noriega-Papaqui , L. Olivera-Nieto , N. Omodei , A. Peisker , Y. Pérez Araujo , E. G. Pérez-Pérez , C. D. Rho , D. Rosa-González , E. Ruiz-Velasco , H. Salazar , F. Salesa Greus , A. Sandoval , P. M. Saz Parkinson , J. Serna-Franco , A. J. Smith , R. W. Springer , O. Tibolla , K. Tollefson , I. Torres , R. Torres-Escobedo , R. Turner , F. Ureña-Mena , L. Villaseñor , X. Wang , I. J. Watson , F. Werner , E. Willox , J. Wood , A. Zepeda , H. Zhou

Radio-detection is becoming an established technique for the detection of air showers induced by cosmic particles. This is in particular true at the highest energies, where very large detection areas are required. A proper description of…

Instrumentation and Methods for Astrophysics · Physics 2022-10-04 Valentin Decoene , Olivier Martineau-Huynh , Matias Tueros

The Telescope Array (TA) experiment, located in the western desert of Utah,USA, is designed for observation of extensive air showers from extremely high energy cosmic rays. The experiment has a surface detector array surrounded by three…

Instrumentation and Methods for Astrophysics · Physics 2015-06-03 T. Abu-Zayyad , R. Aida , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , R. Cady , B. G. Cheon , J. Chiba , M. Chikawa , E. J. Cho , W. R. Cho , H. Fujii , T. Fujii , T. Fukuda , M. Fukushima , D. Gorbunov , W. Hanlon , K. Hayashi , Y. Hayashi , N. Hayashida , K. Hibino , K. Hiyama , K. Honda , T. Iguchi , D. Ikeda , K. Ikuta , N. Inoue , T. Ishii , R. Ishimori , D. Ivanov , S. Iwamoto , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , T. Kanbe , K. Kasahara , H. Kawai , S. Kawakami , S. Kawana , E. Kido , H. B. Kim , H. K. Kim , J. H. Kim , J. H. Kim , K. Kitamoto , K. Kobayashi , Y. Kobayashi , Y. Kondo , K. Kuramoto , V. Kuzmin , Y. J. Kwon , S. I. Lim , S. Machida , K. Martens , J. Martineau , T. Matsuda , T. Matsuura , T. Matsuyama , J. N. Matthews , I. Myers , M. Minamino , K. Miyata , H. Miyauchi , Y. Murano , T. Nakamura , S. W. Nam , T. Nonaka , S. Ogio , M. Ohnishi , H. Ohoka , K. Oki , D. Oku , T. Okuda , A. Oshima , S. Ozawa , I. H. Park , M. S. Pshirkov , D. Rodriguez , S. Y. Roh , G. Rubtsov , D. Ryu , H. Sagawa , N. Sakurai , A. L. Sampson , L. M. Scott , P. D. Shah , F. Shibata , T. Shibata , H. Shimodaira , B. K. Shin , J. I. Shin , T. Shirahama , J. D. Smith , P. Sokolsky , T. J. Sonley , R. W. Springer , B. T. Stokes , S. R. Stratton , T. A. Stroman , S. Suzuki , Y. Takahashi , M. Takeda , A. Taketa , M. Takita , Y. Tameda , H. Tanaka , K. Tanaka , M. Tanaka , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , Y. Tsunesada , K. Tsutsumi , Y. Tsuyuguchi , Y. Uchihori , S. Udo , H. Ukai , G. Vasiloff , Y. Wada , T. Wong , M. Wood , Y. Yamakawa , H. Yamaoka , K. Yamazaki , J. Yang , S. Yoshida , H. Yoshii , R. Zollinger , Z. Zundel

Calibrating the absolute energy scale of air showers initiated by ultra-high energy cosmic rays is an important experimental issue. Currently, the corresponding systematic uncertainty amounts to 14-21% using the fluorescence technique. Here…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 Piotr Homola , Markus Risse

The measurement of the flux of muons produced in cosmic ray air showers is essential for the study of primary cosmic rays. Such measurements are important in extensive air shower detectors to assess the energy spectrum and the chemical…

High Energy Astrophysical Phenomena · Physics 2024-09-16 KM3NeT Collaboration

Some recent experiments, performed at Berkeley, Cologne, Florence and Vienna led to the claim that something seems to travel with a speed larger than the speed c of light in vacuum. Various other experimental results seem to point in the…

Classical Physics · Physics 2010-02-01 Erasmo Recami

Jets are ubiquitous in the Universe and, as demonstrated in this volume, are seen from a large number of astrophysical objects. For a number of reasons, in particular their proximity and the abundant range of diagnostics to determine their…

Solar and Stellar Astrophysics · Physics 2021-05-05 T. P. Ray , J. Ferreira

It has been proposed recently that Galactic microquasars may be prodigious emitters of TeV neutrinos that can be detected by upcoming km^2 neutrino telescopes. In this paper we consider a sample of identified microquasars and microquasar…

Astrophysics · Physics 2009-11-07 C. Distefano , D. Guetta , E. Waxman , A. Levinson

Satellite formation is a natural by-product of planet formation. With the discovery of nu- merous extrasolar planets, it is likely that moons of extrasolar planets (exomoons) will soon be discovered. Some of the most promising techniques…

Earth and Planetary Astrophysics · Physics 2017-01-10 Amy C. Barr

The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calculated on the basis of a detailed threshold analysis and computation of the shower production rate. We show that diffuse neutrinos from…

High Energy Physics - Phenomenology · Physics 2011-05-23 A. L. Provorov , I. M. Zheleznykh

We provide the first investigation of the solar production of symmetrons, a well-motivated class of screened scalar fields with density dependent couplings to the Standard Model, and their subsequent absorption in underground direct…

High Energy Physics - Phenomenology · Physics 2026-04-13 Hannah Banks , Anne-Christine Davis , Luca Visinelli

A new variational technique determines the general condition of equilibrium of a rotating gravito-electromagnetic system and provides a modified dynamical equation of motion from where it emerges a so-far unforseen topological torsion…

Space Physics · Physics 2019-03-25 Mario J. Pinheiro

A report on the characteristics of ultra-high energy air showers simulated with the current version of the AIRES program is presented. The AIRES system includes a fast simulating program, originally designed on the basis of the well-known…

Astrophysics · Physics 2007-05-23 S. J. Sciutto

Muons with a high transverse momentum (p_T) are produced in cosmic ray air showers via semileptonic decay of heavy quarks and the decay of high p_T kaons and pions. These high p_T muons have a large lateral separation from the shower core…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Lisa Gerhardt , Spencer Klein

Cosmic rays have valuable information about universe surroundings us. Finding energy, mass and arrival direction of primary cosmic ray particle are the most important aspects of extensive air shower studies. In order to determine these…

Instrumentation and Methods for Astrophysics · Physics 2011-03-17 H. Hedayati Kh. , A. Anvari , M. Bahmanabadi , M. Khakian Ghomi , J. Samimi

Evidence for fine-tuning of physical parameters suitable for life can perhaps be explained by almost any combination of providence, coincidence or multiverse. A multiverse usually includes parts unobservable to us, but if the theory for it…

High Energy Physics - Theory · Physics 2007-05-23 Don N. Page

Orbiting detectors will be able to observe showers initiated by neutrinos penetrating the Earth and interacting close to their exit point. There is a correlation between the impact parameter of the incident neutrino and its energy. We study…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Domokos , S. Kovesi-Domokos