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Relevant bibliographies by topics / Cosmic Rays, CALET, Interaction Point

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Academic literature on the topic 'Cosmic Rays, CALET, Interaction Point'

Author: Grafiati

Published: 14 March 2023

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Journal articles on the topic "Cosmic Rays, CALET, Interaction Point"

1

Tatischeff, Vincent, and Stefano Gabici. "Particle Acceleration by Supernova Shocks and Spallogenic Nucleosynthesis of Light Elements." Annual Review of Nuclear and Particle Science 68, no. 1 (2018): 377–404. http://dx.doi.org/10.1146/annurev-nucl-101917-021151.

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In this review, we first reassess the supernova remnant paradigm for the origin of Galactic cosmic rays in the light of recent cosmic-ray data acquired by the Voyager 1 spacecraft. We then describe the theory of light-element nucleosynthesis by nuclear interaction of cosmic rays with the interstellar medium and outline the problem of explaining the measured beryllium abundances in old halo stars of low metallicity with the standard model of the Galactic cosmic-ray origin. We then discuss the various cosmic-ray models proposed in the literature to account for the measured evolution of the light

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2

BARBIERI, JAMES, GEORGE CHAPLINE, and DAVID I. SANTIAGO. "QUANTUM CRITICALITY, EVENT HORIZONS AND COSMIC GAMMA RAY BURSTS." Modern Physics Letters A 18, no. 39 (2003): 2767–73. http://dx.doi.org/10.1142/s0217732303012489.

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The logical inconsistency of quantum mechanics and general relativity can be avoided if the relativity principle fails for length scales smaller than the quantum coherence length for the vacuum state. This has dramatic consequences for the phenomenology of compact astrophysical objects. If we assume that at the Planck scale elementary particles interact via a universal four-point interaction and baryon number conservation is violated, then nucleons approaching an event horizon surface can disintegrate into gamma rays and high energy leptons. Integrating the Altarelli–Parisi equations to find t

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3

Fiorillo, Damiano F. G., Mauricio Bustamante, and Victor B. Valera. "Near-future discovery of point sources of ultra-high-energy neutrinos." Journal of Cosmology and Astroparticle Physics 2023, no. 03 (2023): 026. http://dx.doi.org/10.1088/1475-7516/2023/03/026.

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Abstract Upcoming neutrino telescopes may discover ultra-high-energy (UHE) cosmic neutrinos, with energies beyond 100 PeV, in the next 10–20 years. Finding their sources would identify guaranteed sites of interaction of UHE cosmic rays, whose origin is unknown. We search for sources by looking for multiplets of UHE neutrinos arriving from similar directions. Our forecasts are state-of-the-art, geared at neutrino radio-detection in IceCube-Gen2. They account for detector energy and angular response, and for critical, but uncertain backgrounds. Sources at declination of -45° to 0° will be easies

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4

SALTZBERG, DAVID, Katsushi Arisaka, Ron Bain, et al. "INTRODUCTION TO THE SALSA, A SALTDOME SHOWER ARRAY AS A GZK NEUTRINO OBSERVATORY." International Journal of Modern Physics A 21, supp01 (2006): 252–53. http://dx.doi.org/10.1142/s0217751x06033726.

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The observed spectrum of ultra-high energy cosmic rays virtually guarantees the presence of ultra-high energy neutrinos due to their interaction with the cosmic microwave background. Every one of these neutrinos will point back to its source and, unlike cosmic rays, will arrive at the Earth unattenuated, from sources perhaps as distant as z =20. The neutrino telescopes currently under construction, should discover a handful of these events, probably too few for detailed study. In this talk I will describe how an array of VHF and UHF antennas embedded in a large salt dome, SalSA (Saltdome Showe

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5

de Naurois, Mathieu. "TeV observations of the Galactic center and starburst galaxies." Proceedings of the International Astronomical Union 9, S303 (2013): 29–42. http://dx.doi.org/10.1017/s1743921314000118.

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AbstractThe vicinity of the Galactic center harbors many potential accelerators of cosmic rays (CR) that could shine in very-high-energy (VHE) γ-rays, such as pulsar wind nebulae, supernova remnants, binary systems and the central black hole Sgr A*, and is characterized by high gas density, large magnetic fields and a high rate of starburst activity similar to that observed in the core of starburst galaxies. In addition to these astrophysical sources, annihilation of putative WIMPs concentrated in the gravitational well could lead to significant high-energy emission at the Galactic center. The

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6

Barlykov, N., V. Dudin, T. Enik, et al. "MiniSPD Stand for Testing Si-Detectors." Nonlinear Phenomena in Complex Systems 25, no. 3 (2022): 254–65. http://dx.doi.org/10.33581/1561-4085-2022-25-3-254-265.

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SPD (Spin Physics Detector) collaboration proposes to install a universal setup in the second interaction point of the NICA collider under construction (JINR, Dubna) to study the spin structure of the proton and deuteron. It plans to carry out research of spin-related phenomena with polarized proton and deuteron beams at a collision energy up to 27 GeV and a luminosity up to 1032 cm−2 s−1. MiniSPD stand is manufactured as a setup for testing SPD detector prototypes with cosmic muons at LHEP. It allows to carry out checkout of the Data Acquisition System (DAQ), the Detector Control System (DCS)

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7

Gusev, А. I., and O. I. Guseva. "NEMESIS APPROXIMATED TO SUN." Globus 7, no. 2(59) (2021): 4–11. http://dx.doi.org/10.52013/2658-5197-59-2-1.

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Photographs of double Sun lead in paper that it took off with Prohodnaja Griva of Gornyy Altay (near c. Belokurikha). Evidences of approaching second Sun – Nemesis to our Shine. Influence of Nemesis on the cosmic events in Sun system are very impression that its testify about interaction of two stars and influence second Sun on the planets of Sun system. Powerful emissions of plasma in view concentration rays with side of our Sun and separation blue spectrums clots with Nemesis that it point on the essential helium component. Myself Nemesis can to be carry to class B – white-blue giants. Anoma

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8

Fehérkuti, Anna, Gábor I. Veres, Ralf Ulrich, and Tanguy Pierog. "Feasibility Studies of Charge Exchange Measurements in pp Collisions at the LHC." Entropy 24, no. 9 (2022): 1188. http://dx.doi.org/10.3390/e24091188.

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(1) Pions produced in the development of extended atmospheric cosmic ray air showers subsequently decay to muons. The measured yield of those muons is generally underestimated by current phenomenological models and event generators optimized for cosmic ray physics. The importance of those disagreements motivates the feasibility studies for testing these models at the Large Hadron Collider (LHC) energies, at the highest center-of-mass energies achievable in a laboratory. The interaction of a nucleus and a virtual pion created in a charge exchange reaction at the LHC is a similar process to thos

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9

Chalov, S. V., H. J. Fahr, and Y. G. Malama. "Unexpected sites of efficient stochastic acceleration in the inner heliosheath." Annales Geophysicae 25, no. 3 (2007): 575–80. http://dx.doi.org/10.5194/angeo-25-575-2007.

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Abstract. Up until the recent past, it was generally believed that the solar wind termination shock (TS) is the favourite site to accelerate ions from the keV- to the MeV- energy levels by means of Fermi-1 processes. When Voyager 1 was crossing the TS at the end of 2004, the registrations of this spacecraft showed, however, that beyond the shock passage fluxes of anomalous cosmic rays kept increasing with time. This obviously called for an acceleration site further downstream of the shock in the heliosheath which had not been identified before. In this paper we thus investigate the process of

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10

Nam, J. W., C. C. Chen, C. H. Chen, et al. "Design and implementation of the TAROGE experiment." International Journal of Modern Physics D 25, no. 13 (2016): 1645013. http://dx.doi.org/10.1142/s0218271816450139.

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Taiwan astroparticle radiowave observatory for geo-synchrotron emissions (TAROGE) is an antenna array on the high mountains of Taiwan’s east coast for the detection of ultra-high energy cosmic rays (UHECRs) in an energy above [Formula: see text] eV. The antennas point toward the ocean to detect radiowave signals emitted by the UHECR-induced air-shower as a result of its interaction with the geomagnetic field. Looking down from the coastal mountain, the effective area is enhanced by collecting both direct-emission as well as the ocean-reflected signals. This instrument also provides the capabil

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