Relevant bibliographies by topics / Ultra High Energy Cosmic Rays phenomenology

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
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Academic literature on the topic 'Ultra High Energy Cosmic Rays phenomenology'

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Published: 9 March 2023
Last updated: 10 March 2023

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Journal articles on the topic "Ultra High Energy Cosmic Rays phenomenology"

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Piórkowska-Kurpas, Aleksandra, and Marek Biesiada. "Testing Quantum Gravity in the Multi-Messenger Astronomy Era." Universe 8, no. 6 (June 8, 2022): 321. http://dx.doi.org/10.3390/universe8060321.

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Quantum gravity (QG) remains elusive despite almost century-long efforts to combine general relativity and quantum mechanics. All the approaches triggered and powered by purely theoretical considerations eventually failed with a prevailing feeling of a complete lack of guidance from the experimental side. Currently, however, this circumstance is beginning to change considerably. We have entered the era of multi-messenger astronomy. The electromagnetic window to the universe—so far the only one—has been tremendously enlarged in the energy range beyond gamma rays up to ultra-high-energy photons and has been complemented by other messengers: high-energy cosmic rays, cosmic neutrinos, and gravitational waves (GWs). This has created a unique environment in which to observationally constrain various phenomenological QG effects. In this paper, we focus on the LIV phenomenology manifested as energy-dependent time-of-flight delays and strong lensing time delays. We review results regarding time-of-flight delays obtained with GRBs. We also recall the idea of energy-dependent lensing time delays, which allow one to constrain LIV models independently of the intrinsic time delay. Lastly, we show how strongly a gravitationally lensed GW signal would place interesting constraints on the LIV.
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Torri, Marco Danilo Claudio. "Quantum Gravity Phenomenology Induced in the Propagation of UHECR, a Kinematical Solution in Finsler and Generalized Finsler Spacetime." Galaxies 9, no. 4 (November 14, 2021): 103. http://dx.doi.org/10.3390/galaxies9040103.

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It is well-known that the universe is opaque to the propagation of Ultra-High-Energy Cosmic Rays (UHECRs) since these particles dissipate energy during their propagation interacting with the background fields present in the universe, mainly with the Cosmic Microwave Background (CMB) in the so-called GZK cut-off phenomenon. Some experimental evidence seems to hint at the possibility of a dilation of the GZK predicted opacity sphere. It is well-known that kinematical perturbations caused by supposed quantum gravity (QG) effects can modify the foreseen GZK opacity horizon. The introduction of Lorentz Invariance Violation can indeed reduce, and in some cases making negligible, the CMB-UHECRs interaction probability. In this work, we explore the effects induced by modified kinematics in the UHECR lightest component phenomenology from the QG perspective. We explore the possibility of a geometrical description of the massive fermions interaction with the supposed quantum structure of spacetime in order to introduce a Lorentz covariance modification. The kinematics are amended, modifying the dispersion relations of free particles in the context of a covariance-preserving framework. This spacetime description requires a more general geometry than the usual Riemannian one, indicating, for instance, the Finsler construction and the related generalized Finsler spacetime as ideal candidates. Finally we investigate the correlation between the magnitude of Lorentz covariance modification and the attenuation length of the photopion production process related to the GZK cut-off, demonstrating that the predicted opacity horizon can be dilated even in the context of a theory that does not require any privileged reference frame.
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Attallah, R. "Ultra high energy cosmic rays." Journal of Physics: Conference Series 1766, no. 1 (January 1, 2021): 012004. http://dx.doi.org/10.1088/1742-6596/1766/1/012004.

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Kim, Hang Bae. "Ultra-high energy cosmic rays." Journal of the Korean Physical Society 78, no. 10 (March 8, 2021): 912–17. http://dx.doi.org/10.1007/s40042-021-00119-w.

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KIM, Hang Bae. "Ultra-High-Energy Cosmic Rays." Physics and High Technology 27, no. 7/8 (August 31, 2018): 26–30. http://dx.doi.org/10.3938/phit.27.033.

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Watson, A. A. "Ultra-high Energy Cosmic Rays." Acta Physica Polonica B 50, no. 12 (2019): 2035. http://dx.doi.org/10.5506/aphyspolb.50.2035.

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Mollerach, Silvia. "Ultra-High energy cosmic rays." Journal of Physics: Conference Series 2156, no. 1 (December 1, 2021): 012007. http://dx.doi.org/10.1088/1742-6596/2156/1/012007.

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Abstract An overview of the status of the knowledge in the field of ultra-high energy cosmic rays is presented. The latest results on the spectrum, arrival direction distribution and composition measurements are summarized and some implications for the understanding of the cosmic ray origin and their propagation are discussed.
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Protheroe, R. J., and R. W. Clay. "Ultra High Energy Cosmic Rays." Publications of the Astronomical Society of Australia 21, no. 1 (2004): 1–22. http://dx.doi.org/10.1071/as03047.

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AbstractCosmic rays with energies above 1018 eV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are either currently under construction or the subject of well-developed proposals. This paper aims to discuss some of the physics of such particles in terms of current knowledge and information from particle astrophysics at other energies.
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Wibig, Tadeusz, and Arnold W. Wolfendale. "Ultra high energy cosmic rays." Journal of Physics G: Nuclear and Particle Physics 34, no. 9 (July 31, 2007): 1891–900. http://dx.doi.org/10.1088/0954-3899/34/9/003.

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SOKOLSKY, PIERRE. "ULTRA-HIGH ENERGY COSMIC RAYS." Modern Physics Letters A 19, no. 13n16 (May 30, 2004): 959–66. http://dx.doi.org/10.1142/s0217732304014240.

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We describe the current status of the High Resolution Fly's Eye detector. Recent results indicate that the UHE cosmic ray spectrum exhibits significant structure near 1019 eV. A few events are seen beyond 1020 eV in contradiction to the AGASA ground array claim of no cut-off. The composition of the cosmic rays is found to change from a predominantly heavy to a predominantly light mixture between and 1017 and 1018 eV. No evidence for anisotropy, on either small scales or large scales is found, in contradiction to AGASA. Systematic errors and absolute energy scale issues are now being carefully considered to see how to partially resolve this discrepancy. A new experiment(FLASH) at the Stanford Linear Accelerator Center (SLAC) to measure the Nitrogen fluorescence efficiency more precisely is described.
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Dissertations / Theses on the topic "Ultra High Energy Cosmic Rays phenomenology"

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TORRI, MARCO DANILO CLAUDIO. "LORENTZ INVARIANCE VIOLATION EFFECTS ON ULTRA HIGH ENERGY COSMIC RAYS PROPAGATION: A GEOMETRICAL APPROACH." Doctoral thesis, Università degli Studi di Milano, 2019. http://hdl.handle.net/2434/625711.

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Cosmic rays are highly energetic extraterrestrial particles, mainly originated outside the Solar system, with energy that spans many decades. Since they include the most energetic particles, accessible nowadays, it is very interesting to study this kind of radiation, that constitute a significant source of informations about astrophysical objects. Moreover these highly energetic particles propagate for cosmological distances, so they can furnish a deeper understanding of the physical mechanisms of the universe. Hence it results very important to obtain a deeper understanding of the so called GZK “puzzle”. Universe results opaque to the propagation of the highest energetic particles, because of their interaction with the Cosmic Microwave Background Radiation (CMBR). Therefore the sources of these Ultra High Energy Cosmic Rays (UHECR) must be collocated inside a foreseen opacity sphere (GZK effect). But some recent experimental observations seem to indicate the possibility that certain UHECR correlate with candidate sources collocated farther than expected. One of the most interesting possible explanations of this GZK suppression “puzzle” consists in introducing a particle kinematics modification, assuming this effect as a relic of the supposed quantum structure of space-time. In this respect, physics is amended by the introduction of small perturbations to the Lorentz symmetry, the so called Lorentz Invariance Violation (LIV) scenario. In this work, to preserve the idea of space-time homogeneity and isotropy, a possible way to introduce a LIV theory, without a preferred class of inertial observers, is explored. The Lorentz symmetry is therefore only modified, as in Doubly Special Relativity theories. Thus the idea of space-time isotropy results restored respect to the new amended Lorentz transformations, here introduced. Hence it results possible to solve the GZK “puzzle” without the necessity of the introduction of a privileged class of inertial observers. The geometry of space-time is constructed starting from the momentum space modified structure, determined by the amended particle kinematics. The resultant geometry is of Finsler type, with an acquired energy dependance. The Lorentz group is then modified, in order to preserve space-time isotropy. The particle Standard Model results modified, but it still preserve the symmetry structure of the ordinary one, as shown proving the validity of the Coleman-Mandula theorem, with the substitution of the ordinary Lorentz group with the modified one. Finally the model is employed to compute phenomenological predictions on the behavior of UHECR and even of high energy neutrinos.
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Blanco-Pillado, José Juan. "Topological defects and ultra-high energy cosmic rays /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2001.

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Thesis (Ph.D.)--Tufts University, 2001.
Adviser: Alexander Vilenkin. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 108-114). Access restricted to members of the Tufts University community. Also available via the World Wide Web;
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Taylor, Andrew Martin. "The propagation of ultra high energy cosmic rays." Thesis, University of Oxford, 2007. http://ora.ox.ac.uk/objects/uuid:63572ebe-fb32-41b6-8b91-a7294db135a6.

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This thesis presents theoretical work on the propagation of ultra high energy cosmic rays, from their source to Earth. The different energy loss processes, resulting from cosmic ray interactions with the radiation fields, are addressed. The subsequent uncertainties in the energy loss rates and the effect produced on the arriving cosmic ray spectrum are highlighted. The question of the composition of ultra high energy cosmic rays remains unresolved, with the range of possibilities leading to quite different results in both the secondary fluxes of particles produced through cosmic ray energy loss interactions en route, and the arriving cosmic ray spectra at Earth. A large range of nuclear species are considered in this work, spanning the range of physically motivated nuclear types ejected from the cosmic ray source. The treatment of cosmic ray propagation is usually handled through Monte Carlo simulations due to the stochastic nature of some of the particle physics processes relevant. In this work, an analytic treatment for cosmic ray nuclei propagation is developed. The development of this method providing a deeper understanding of the main components relevant to cosmic ray nuclei propagation, and through its application, a clear insight into the contributing particle physics aspects of the Monte Carlo simulation. A flux of secondary neutrinos, produced as a consequence of cosmic ray energy loss through pion production during propagation, is also expected to be observed at Earth. This spectrum, however, is dependent on several loosely constrained factors such as the radiation field in the infrared region and cosmic ray composition. The range of possible neutrino fluxes obtainable with such uncertainties are discussed in this work. High energy cosmic ray interactions with the radiation fields present within the source may also occur, leading to cosmic ray energy loss before the cosmic ray has even managed to escape. The secondary spectra produced are investigated through the consideration of three candidate sources. A relationship between the degree of photo-disintegration in the source region and the neutrino flux produced through p γ interactions is found.
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Brobeck, Elina Stone Edward McKeown R. D. "Measurement of ultra-high energy cosmic rays with CHICOS /." Diss., Pasadena, Calif. : California Institute of Technology, 2009. http://resolver.caltech.edu/CaltechETD:etd-10192008-143041.

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Lundanes, Ingvild Olsen. "The propagation and energy losses of ultra high energy cosmic rays." Thesis, Norges teknisk-naturvitenskapelige universitet, Institutt for fysikk, 2011. http://urn.kb.se/resolve?urn=urn:nbn:no:ntnu:diva-12654.

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This project investigates the propagation of ultra-high energy cosmic raynuclei and protons. A simulation of the propagation subjecting the particlesto energy losses due to cosmological redshift as well as interactions with theextra-galactic background radiation seeks to find the initial conditions at thesource which give the best results on Earth compared to the observations ofthe Pierre Auger Observatory (PAO).The results agree with previous works of the same kind that a chemicalcomposition of medium-weight fits the observed air shower data best. Thestarting conditions which gave the best results for the air shower characteristics and RMS(Xmax) were dN/dE proportional to E^{-alpha} with alpha = 1.6 for an initial chemical composition of 25% nitrogen and 75% silicon. Other combinations of themedium-weight nuclei also yielded similar results.No starting conditions could accommodate both the observed dN/dE and theair shower data simultaneously. Other works indicate that this might beimproved by the implementation of extra-galactic magnetic fields, but it couldalso indicate that the error margins in the observed data are underestimated
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Barbot, Cyrille. "Super-heavy X-particle decay and ultra-high energy cosmic rays." [S.l. : s.n.], 2003. http://deposit.ddb.de/cgi-bin/dokserv?idn=969379846.

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Khanin, Alexander. "Bayesian methods for the analysis of ultra-high-energy cosmic rays." Thesis, Imperial College London, 2016. http://hdl.handle.net/10044/1/42034.

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The origins of ultra-high-energy cosmic rays (UHECRs) are one of the open puzzles of astrophysics. A number of plausible candidates, such as active galactic nuclei (AGNs) have been discussed, but no clear consensus has been reached. One way to assess the different hypotheses is by analyzing the UHECR arrival directions. Recently, a small number of studies have begun applying Bayesian methodologies to this problem, forming the first steps in the development of a comprehensive Bayesian framework for the study of UHECRs. In this work, we have developed two Bayesian methods to study this question, and have applied them to UHECRs from the Pierre Auger Observatory (PAO). The first method was a Bayesian approach to studying the catalogue-independent clustering of UHECRs. Previously, this had been difficult as there is no well motivated clustered model that can be used in a Bayesian model comparison. We have resolved this difficulty by developing a multi-step approach that derives such a model from a sub-set of the data. This approach could have broad applications for anisotropy searches in other areas of astronomy. Our results were consistent with both isotropic and clustered models. The second was a Bayesian method that was aimed to find associations between UHECR arrival directions and source catalogues. It was an extension of a previous Bayesian study, but analyzed a greater data set, used a more refined UHECR model, and was generalized to be applicable to a greater variety of source catalogues. Our results were broadly consistent with previous work, with the purely isotropic UHECR models being disfavoured for reasonable parameter ranges. It will be of great interest to apply our methods to samples of greater size. The extended UHECR samples that will be available in the near future should be sufficient for our methods to determine the origins of the UHECRs.
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Morris, Chad Michael. "Detection Techniques of Radio Emission from Ultra High Energy Cosmic Rays." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1254506832.

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Rodrigues, Xavier. "Blazars as Sources of Neutrinos and Ultra-high-energy Cosmic Rays." Doctoral thesis, Humboldt-Universität zu Berlin, 2019. http://dx.doi.org/10.18452/20610.

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Der Ursprung ultra-hochenergetischer kosmischer Strahlung (UHECRs) ist immer noch unbekannt. Neutrinoteleskope wie IceCube messen einen Fluss hochenergetischer astrophysikalischer Neutrinos, dessen erwarteter Ursprung Wechselwirkungen kosmischer Strahlung (CR) ist. Jedoch scheinen die Ankunftsrichtungen der beobachteten Neutrinos nicht signifikant mit den Koordinaten bekannter, hochenergetischer astrophysikalischer Quellen zu korrelieren. Wir tragen zum Verständnis dieses Problems durch die Untersuchung von Blazaren, eine Klasse aktiver Galaxienkerne, bei. Motiviert durch Hinweise, dass ein Teil der UHECRs schwerer als Protonen ist, modellieren wir die Wechselwirkungen einer Population beschleunigter Kerne mit den umgebenden Photonfelder in Blazaren. Wir folgern, dass in Blazaren niedriger Luminosität beschleunigte CRs nicht effizient wechselwirken. In hellen Blazaren sind photo-hadronische Wechselwirkungen effizient, was zu starker Neutrinoproduktion und zur Entwicklung einer nuklearen Kaskade führt. Wir berechnen die Neutrinoemission der gesamten Verteilung von Blazaren, und folgern, dass eine Population niedriger Luminosität, die derzeit nicht beobachtet, aber theoretisch erwartet wird, den gesamten IceCube-Fluss bei den höchsten Energien erklären kann. Weiterhin modellieren wir den Blazar TXS 0506+056, aus dessen Richtung ein Neutrino während einer Phase erhöhter elektromagnetischer Aktivität detektiert wurde. Wir testen die Hypothese, dass ein Signal von 13+/-5 Neutrinos, die in IceCube aus der selben Richtung im Jahr 2014-15 gemessen wurden, von der selben Quelle stammt. Unser Modell kann höchstens 5 Ereignisse erklären. Schließlich untersuchen wir das erste beobachte Ereignis verschmelzender Neutronensterne, GW170817, als CR-Beschleuniger. Wir modellieren die Quelle und zeigen, dass Radio- und Röntgenmessungen strikte Beschränkungen der magnetischen Feldstärke nach sich ziehen. Wir zeigen, dass diese Quelle in der Lage ist, CRs zu emittieren.
The origin of ultra-high-energy cosmic rays (UHECRs) is still unclear. Neutrino telescopes like IceCube have observed a flux of high-energy cosmic neutrinos, expected to originate in cosmic ray (CR) interactions. However, their arrival directions do not statistically correlate with the positions of known high-energy astrophysical sources. In this thesis we explore blazars, a class of active galaxies, as potential UHECR accelerators. Motivated by evidence that a fraction of the UHECRs are heavier than protons, we model the interactions of CR nuclei with the photon fields present in blazars, in order to estimate the emitted neutrino and UHECR spectrum. We conclude that in dim blazars, accelerated CRs do not interact efficiently due to the low photon density, but instead escape the source unscathed. In bright blazars, photo-hadronic interactions are more efficient, leading to abundant production of neutrinos and lighter nuclei. We use this model to quantify the neutrino emission from the entire cosmological blazar population. We conclude that low-luminosity blazars currently unobserved but expected theoretically, can explain the entire IceCube flux at the highest energies. We then focus on blazar TXS 0506+056, from whose direction a neutrino was recently detected during an electromagnetic flaring state. We test the hypothesis that a signal of 13+/-5 neutrinos observed by IceCube from the same direction in 2014-15 may have originated in the same source. Given the constraints from multi-wavelength observations, this model can explain at most 5 neutrino events. Finally, we study the remnant of the first neutron star merger ever observed, object GW170817. We model the particle interactions in the source and show that multi-wavelength observations can provide a constraint on the magnetic field strength. We estimate that this source may be an efficient CR emitter, which shows the importance of future multi-messenger observations to better constrain this source type.
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Smith, Nigel James Telfer. "A search for ultra high energy gamma ray sources from the South Pole." Thesis, University of Leeds, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.291023.

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Books on the topic "Ultra High Energy Cosmic Rays phenomenology"

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Laboratory, Fermi National Accelerator, ed. Cosmic strings and ultra-high energy cosmic rays. Batavia, IL: Fermi National Accelerator Laboratory, 1990.

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Laboratory, Fermi National Accelerator, ed. Cosmic strings and ultra-high energy cosmic rays. Batavia, IL: Fermi National Accelerator Laboratory, 1990.

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Lemoine, Martin, and Günter Sigl, eds. Physics and Astrophysics of Ultra-High-Energy Cosmic Rays. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/3-540-45615-5.

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Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. Hauppauge, N.Y: Nova Science Publishers, 2009.

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Uryson, Anna. Ultra high energy cosmic rays: A new tool for astrophysics research. New York: Nova Science Publishers, 2010.

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Mottram, Matthew Joseph. A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-30032-5.

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service), SpringerLink (Online, ed. A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.

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International Symposium on the Recent Progress of Ultra-high Energy Cosmic Ray Observation (2010 Nagoya-shi, Japan). International Symposium on the Recent Progress of Ultra-high Energy Cosmic Ray Observation, Aichi, Japan, 10-12 December 2010. Edited by Sagawa Hiroyuki. Melville, N.Y: American Institute of Physics, 2011.

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Ultra-High Energy Particle Astrophysics. Nova Science Publishers, 2003.

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(Editor), M. Lemoine, and G. Sigl (Editor), eds. Physics and Astrophysics of Ultra High Energy Cosmic Rays. Springer, 2002.

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Book chapters on the topic "Ultra High Energy Cosmic Rays phenomenology"

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Billoir, Pierre. "Phenomenology of Ultra-High-Energy Atmospheric Showers." In Physics and Astrophysics of Ultra-High-Energy Cosmic Rays, 27–44. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/3-540-45615-5_2.

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Spurio, Maurizio. "Ultra High Energy Cosmic Rays." In Astronomy and Astrophysics Library, 203–41. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-08051-2_7.

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Yodh, Gaurang B. "Ultra High Energy Astronomy." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics, 183–210. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_13.

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Kampert, Karl-Heinz, and Alan A. Watson. "Development of Ultra High-Energy Cosmic Ray Research." In From Ultra Rays to Astroparticles, 103–41. Dordrecht: Springer Netherlands, 2012. http://dx.doi.org/10.1007/978-94-007-5422-5_5.

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Khlopov, Maxim Yu, and Sergei G. Rubin. "Astronomy of Ultra High Energy Cosmic Rays." In Cosmological Pattern of Microphysics in the Inflationary Universe, 145–69. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2650-8_7.

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Berezinsky, Venya. "Course 5: Ultra High Energy Cosmic Rays." In Accretion discs, jets and high energy phenomena in astrophysics, 233–49. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-39932-2_5.

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Jones, T. W. "Acceleration of Ultra High Energy Cosmic Rays: Cosmic Zevatrons?" In The Early Universe and the Cosmic Microwave Background: Theory and Observations, 451–70. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-007-1058-0_20.

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Berezinsky, Veniamin. "On origin of ultra high energy cosmic rays." In The Multi-Messenger Approach to High-Energy Gamma-Ray Sources, 453–63. Dordrecht: Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-6118-9_70.

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Auriemma, G. "The Mass Spectrum of Ultra High Energy Cosmic Rays." In Physical Processes in Hot Cosmic Plasmas, 315–23. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0545-0_18.

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Tanco, Gustavo Medina. "Ultra-high Energy Cosmic Rays: From GeV to ZeV." In Astrophysics and Space Science Proceedings, 165–96. Dordrecht: Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-5575-1_5.

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Conference papers on the topic "Ultra High Energy Cosmic Rays phenomenology"

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Mariazzi, A., and M. Tueros. "Phenomenology of the Invisible Energy: Revisiting the Heitler–Matthews Cascade Model." In Proceedings of 2016 International Conference on Ultra-High Energy Cosmic Rays (UHECR2016). Journal of the Physical Society of Japan, 2018. http://dx.doi.org/10.7566/jpscp.19.011044.

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WESTERHOFF, STEFAN. "ULTRA–HIGH-ENERGY COSMIC RAYS." In Proceedings of the XXII International Symposium. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812704023_0034.

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BLASI, PASQUALE. "ULTRA HIGH ENERGY COSMIC RAYS." In Proceedings of the International Conference. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702999_0004.

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Werner, K. "Ultra-High Energy Cosmic Rays." In IX HADRON PHYSICS AND VII RELATIVISTIC ASPECTS OF NUCLEAR PHYSICS: A Joint Meeting on QCD and QCP. AIP, 2004. http://dx.doi.org/10.1063/1.1843607.

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Stanev, Todor. "Ultra High Energy Cosmic Rays." In INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 8th Conference CIPANP2003. AIP, 2004. http://dx.doi.org/10.1063/1.1664257.

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Zepeda, A. "Ultra High Energy Cosmic Rays." In INSTRUMENTATION IN ELEMENTARY PARTICLE PHYSICS. AIP, 2003. http://dx.doi.org/10.1063/1.1604079.

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Lemoine, Martin. "On ultra-high energy cosmic rays." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0052.

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Lemoine, Martin. "On Ultra-High Rigidity Cosmic Rays." In Proceedings of 2016 International Conference on Ultra-High Energy Cosmic Rays (UHECR2016). Journal of the Physical Society of Japan, 2018. http://dx.doi.org/10.7566/jpscp.19.011004.

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Tkachev, Igor I. "Ultra high energy cosmic rays and inflation." In COSMO--98. ASCE, 1999. http://dx.doi.org/10.1063/1.59435.

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Kalli, Sihem, Martin Lemoine, Kumiko Kotera, N. Mebarki, and J. Mimouni. "Ultra High Energy Cosmic Rays Anisotropies Signatures." In THE THIRD ALGERIAN WORKSHOP ON ASTRONOMY AND ASTROPHYSICS. AIP, 2010. http://dx.doi.org/10.1063/1.3518323.

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Reports on the topic "Ultra High Energy Cosmic Rays phenomenology"

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Fowler, T., S. Colgate, and H. Li. On the Origin of Ultra High Energy Cosmic Rays. Office of Scientific and Technical Information (OSTI), July 2009. http://dx.doi.org/10.2172/963520.

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Fowler, T., S. Colgate, H. Li, R. Bulmer, and J. Pino. On the Origin of Ultra High Energy Cosmic Rays II. Office of Scientific and Technical Information (OSTI), March 2011. http://dx.doi.org/10.2172/1021558.

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Chen, Pisin. Plasma Wake Field Acceleration for Ultra High-Energy Cosmic Rays. Office of Scientific and Technical Information (OSTI), July 2002. http://dx.doi.org/10.2172/799975.

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4

Collica, Laura. Mass composition studies of Ultra High Energy cosmic rays through the measurement of the Muon Production Depths at the Pierre Auger Observatory. Office of Scientific and Technical Information (OSTI), January 2014. http://dx.doi.org/10.2172/1249492.

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5

Soleiman, M. H. M., S. S. Abdel-Aziz, and A. Abdelfattah Omar. Identification of nuclear mass range of primary event from the observation of shower in ultra-high energetic cosmic rays at energy ~ 106 GeV. MTPR Journal, September 2019. http://dx.doi.org/10.19138/mtpr/(19)45-49.

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