Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory
To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the p...
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2013
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Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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001 | PAPER-12998 | ||
003 | AR-BaUEN | ||
005 | 20240513184448.0 | ||
008 | 190411s2013 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-84874723778 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
100 | 1 | |a Multitudinario:508 | |
245 | 1 | 0 | |a Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory |
260 | |c 2013 | ||
270 | 1 | 0 | |m Abreu, P.; LIP, Instituto Superior Técnico, Technical University of LisbonPortugal |
500 | |a Este trabajo contiene más de 100 autores, por lo que solo se registrarán: el primer autor que aparece en el mismo (independientemente de su filiación institucional) y a continuación, únicamente los autores que tengan como filiación institucional esta casa de estudios, es decir Exactas-UBA | ||
506 | |2 openaire |e Política editorial | ||
504 | |a Engel, R., Heck, D., Pierog, T., Extensive air showers and hadronic interactions at high energy (2011) Ann. Rev. Nucl. Part. Sci., 61, p. 467. , 10.1146/annurev.nucl.012809.104544 0163-8998 | ||
504 | |a Gaisser, T.K., (1990) Cosmic Rays and Particle Physics | ||
504 | |a Linsley, J., (1983) Spectra, Anisotropies and Composition of Cosmic Rays above 1000 GeV, 12, p. 135 | ||
504 | |a Linsley, J., (1985) Proton-air and Proton-proton Cross Sections from Air Shower Data, 6, p. 1 | ||
504 | |a Abraham, J., Measurement of the Depth of Maximum of Extensive Air Showers above 1018 eV (2010) Phys. Rev. Lett., 104, p. 091101. , 10.1103/PhysRevLett.104.091101, Pierre Auger collaboration | ||
504 | |a Facal San Luis, P., (2011) The Distribution of Shower Maxima of UHECR Air Showers, 2, p. 225. , Pierre Auger collaboration | ||
504 | |a Abreu, P., The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction Models, , Pierre Auger collaboration | ||
504 | |a Matthews, J., A Heitler model of extensive air showers (2005) Astropart. Phys., 22, p. 387. , 10.1016/j.astropartphys.2004.09.003 0927-6505 | ||
504 | |a Linsley, J., (1977) Structure of Large Air Showers at Depth 834 g/cm2, 12, p. 89 | ||
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504 | |a Pierog, T., Alekseeva, M., Bergmann, T., Chernatkin, V., Engel, R., First results of fast one-dimensional hybrid simulation of EAS using CONEX (2006) Nucl. Phys. Proc. Suppl., 151, p. 159. , 10.1016/j.nuclphysBPS.2005.07.029 0920-5632 | ||
504 | |a Bird, D., Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high-energies (1993) Phys. Rev. Lett., 71, p. 3401. , 10.1103/PhysRevLett.71.3401 0031-9007, HIRES collaboration | ||
504 | |a Abbasi, R., A Study of the composition of ultrahigh energy cosmic rays using the High Resolution Fly's Eye (2005) Astrophys. J., 622 (2), p. 910. , 10.1086/427931 0004-637X 910. High Resolution Fly's Eye collaboration | ||
504 | |a Abbasi, R., Indications of Proton-Dominated Cosmic Ray Composition above 1.6 EeV (2010) Phys. Rev. Lett., 104, p. 161101. , 10.1103/PhysRevLett.104.161101, HiRes collaboration | ||
504 | |a Knurenko, S., Sabourov, A., (2011) Spectrum and Mass Composition of Cosmic Rays in the Energy Range 1015 - 1018 EV Derived from the Yakutsk Array Data, 1, p. 189 | ||
504 | |a Jui, C.C., Cosmic Ray in the Northern Hemisphere: Results from the Telescope Array Experiment (2011) Proc. APS DPF Meeting, Providence, RI, U.S.A., J. Phys. Conf. Ser., 404, p. 012037. , 10.1088/1742-6596/404/1/012037 1742-6596 | ||
504 | |a Walker, R., Watson, A., Measurement of the fluctuations in the depth of maximum of showers produced by primary particles of energy greater than 1.5× 1017 eV (1982) J. Phys., 8 (8), p. 1131. , 10.1088/0305-4616/8/8/016 0305-4616 G 016 | ||
504 | |a Garcia-Pinto, D., (2011) Measurements of the Longitudinal Development of Air Showers with the Pierre Auger Observatory, 2, p. 87. , Pierre Auger collaboration | ||
504 | |a Abreu, P., The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction Models, , Pierre Auger collaboration | ||
504 | |a http://www.auger.org/technical_info/ICRC2011/shower_development_data.txt; Unger, M., (2011) EAS Studies of Cosmic Rays above 1016 EV, 12, p. 225 | ||
504 | |a Cazon, L., Ulrich, R., The non-linearity between 〈ln A〉 and 〈Xmax〉 induced by the acceptance of fluorescence telescopes (2012) Astropart. Phys., 38, p. 41. , 10.1016/j.astropartphys.2012.09.001 0927-6505 | ||
504 | |a Pesce, R., (2011) Energy Calibration of Data Recorded with the Surface Detectors of the Pierre Auger Observatory: An Update, 2, p. 214. , Pierre Auger collaboration | ||
504 | |a Abreu, P., The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related Measurements, , Pierre Auger collaboration | ||
504 | |a Abreu, P., Measurement of the proton-air cross-section at s1/2=57 TeV with the Pierre Auger Observatory (2012) Phys. Rev. Lett., 109, p. 062002. , 10.1103/PhysRevLett.109.062002, Pierre Auger collaboration | ||
504 | |a Watson, A., Wilson, J., Fluctuation studies of large air showers - The composition of primary cosmic ray particles of energy E p ∼ 10 18 eV (1974) J. Phys., 7 (10), p. 1199. , 10.1088/0305-4470/7/10/013 0301-0015 A 013 | ||
504 | |a Walker, R., Watson, A., Measurement of the elongation rate of extensive air showers produced by primary cosmic rays of energy above 2× 10 17 eV (1981) J. Phys., 7 (9), p. 1297. , 10.1088/0305-4616/7/9/021 0305-4616 G 021 | ||
504 | |a Kampert, K.-H., Unger, M., Measurements of the Cosmic Ray Composition with Air Shower Experiments (2012) Astropart. Phys., 35, p. 660. , 10.1016/j.astropartphys.2012.02.004 0927-6505 | ||
504 | |a Taylor, A.M., Ahlers, M., Aharonian, F.A., The need for a local source of UHE CR nuclei (2011) Phys. Rev., 84, p. 105007. , 10.1103/PhysRevD.84.105007 0556-2821 D | ||
504 | |a Allard, D., Extragalactic propagation of ultrahigh energy cosmic-rays (2012) Astropart. Phys., 39-40, p. 33. , 10.1016/j.astropartphys.2011.10.011 0927-6505 | ||
504 | |a Allen, J., (2011) Interpretation of the Signals Produced by Showers from Cosmic Rays of 1019 EV Observed in the Surface Detectors of the Pierre Auger Observatory, 2, p. 83. , Pierre Auger collaboration | ||
504 | |a Abreu, P., The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction Models, , Pierre Auger collaboration | ||
504 | |a Rodriguez, G., (2011) Reconstruction of Inclined Showers at the Pierre Auger Observatory: Implications for the Muon Contenty, 2, p. 95. , Pierre Auger collaboration | ||
504 | |a Abreu, P., The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related Measurements, , Pierre Auger collaboration | ||
504 | |a Nelson, W., (1985) The Egs4 Code System, SLAC-265 | ||
504 | |a Fesefeldt, H., (1985) RWTH Aachen Report PITHA 85/2 | ||
520 | 3 | |a To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the parameterization to Pierre Auger Observatory data allows one to study the energy dependence of the mean ln A and of its variance under the assumption of selected hadronic interaction models. We discuss possible implications of these dependences in term of interaction models and astrophysical cosmic ray sources. © 2013 IOP Publishing Ltd and Sissa Medialab srl. |l eng | |
593 | |a Centro Atómico Bariloche, Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina | ||
593 | |a Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF, CONICET, Argentina | ||
593 | |a Departamento de Física, FCEyN, Universidad de Buenos Aires y CONICET, Argentina | ||
593 | |a IFLP, Universidad Nacional de la Plata, CONICET, La Plata, Argentina | ||
593 | |a Instituto de Astronomá́ y Física Del Espacio (CONICET-UBA), Buenos Aires, Argentina | ||
593 | |a Instituto de Física de Rosario (IFIR), CONICET/U.N.R., Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina | ||
593 | |a Instituto de Tecnologá́s en Detección y Astropartículas, Buenos Aires, Argentina | ||
593 | |a National Technological University, Faculty Mendoza (CONICET/CNEA), Mendoza, Argentina | ||
593 | |a Observatorio Pierre Auger, Malargüe, Argentina | ||
593 | |a Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina | ||
593 | |a Universidad Tecnológica Nacional, Facultad Regional Buenos Aires, Buenos Aires, Argentina | ||
593 | |a University of Adelaide, Adelaide, SA, Australia | ||
593 | |a Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, Brazil | ||
593 | |a Universidade de São Paulo, Instituto de Física, São Carlos, SP, Brazil | ||
593 | |a Universidade de São Paulo, Instituto de Física, São Paulo, SP, Brazil | ||
593 | |a Universidade Estadual de Campinas, IFGW, Campinas, SP, Brazil | ||
593 | |a Universidade Estadual de Feira de Santana, Brazil | ||
593 | |a Universidade Federal da Bahia, Salvador, BA, Brazil | ||
593 | |a Universidade Federal Do ABC, Santo André, SP, Brazil | ||
593 | |a Universidade Federal Do Rio de Janeiro, Instituto de Física, Rio de Janeiro, RJ, Brazil | ||
593 | |a Universidade Federal Fluminense, EEIMVR, Volta Redonda, RJ, Brazil | ||
593 | |a Rudjer Bošković Institute, 10000 Zagreb, Croatia | ||
593 | |a Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic | ||
593 | |a Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic | ||
593 | |a Palacky University, RCPTM, Olomouc, Czech Republic | ||
593 | |a Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France | ||
593 | |a Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, France | ||
593 | |a Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France | ||
593 | |a Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier Grenoble, CNRS-IN2P3, France | ||
593 | |a Station de Radioastronomie de Nanćay, Observatoire de Paris, CNRS/INSU, France | ||
593 | |a SUBATECH, École des Mines de Nantes, Université de Nantes, France | ||
593 | |a Bergische Universität Wuppertal, Wuppertal, Germany | ||
593 | |a Karlsruhe Institute of Technology - Campus North, Institut für Kernphysik, Karlsruhe, Germany | ||
593 | |a Karlsruhe Institute of Technology - Campus North, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany | ||
593 | |a Karlsruhe Institute of Technology - Campus South, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany | ||
593 | |a Max-Planck-Institut für Radioastronomie, Bonn, Germany | ||
593 | |a RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany | ||
593 | |a Universität Hamburg, Hamburg, Germany | ||
593 | |a Universität Siegen, Siegen, Germany | ||
593 | |a Dipartimento di Fisica dell'Universitá, INFN, Genova, Italy | ||
593 | |a Universitá dell'Aquila, INFN, L'Aquila, Italy | ||
593 | |a Universitá di Milano, Sezione INFN, Milan, Italy | ||
593 | |a Universitá di Napoli Federico II, Sezione INFN, Napoli, Italy | ||
593 | |a Universitá di Roma II Tor Vergata, Sezione INFN, Roma, Italy | ||
593 | |a Universitá di Catania, Sezione INFN, Catania, Italy | ||
593 | |a Universitá di Torino, Sezione INFN, Torino, Italy | ||
593 | |a Dipartimento di Matematica e Fisica E. de Giorgi, Universitá Del Salento, Sezione INFN, Lecce, Italy | ||
593 | |a Istituto di Astrošica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy | ||
593 | |a Istituto di Fisica Dello Spazio Interplanetario (INAF), Universitá di Torino, Sezione INFN, Torino, Italy | ||
593 | |a INFN, Laboratori Nazionali Del Gran Sasso, Assergi (L'Aquila), Italy | ||
593 | |a Benemérita Universidad Autónoma de Puebla, Puebla, Mexico | ||
593 | |a Centro de Investigación y de Estudios Avanzados Del IPN (CINVESTAV), Mexico | ||
593 | |a Universidad Michoacana de San Nicolas de Hidalgo, Morelia, Michoacan, Mexico | ||
593 | |a Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico | ||
593 | |a IMAPP, Radboud University Nijmegen, Netherlands | ||
593 | |a Kernfysisch Versneller Instituut, University of Groningen, Groningen, Netherlands | ||
593 | |a Nikhef, Science Park, Amsterdam, Netherlands | ||
593 | |a ASTRON, Dwingeloo, Netherlands | ||
593 | |a Institute of Nuclear Physics PAN, Krakow, Poland | ||
593 | |a University of Lódź, Lódź, Poland | ||
593 | |a LIP, Instituto Superior Técnico, Technical University of Lisbon, Portugal | ||
593 | |a 'Horia Hulubei' National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania | ||
593 | |a University of Bucharest, Physics Department, Romania | ||
593 | |a University Politehnica of Bucharest, Romania | ||
593 | |a J. Stefan Institute, Ljubljana, Slovenia | ||
593 | |a Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia | ||
593 | |a Institut de Física Corpuscular, CSIC, Universitat de Valéncia, Valencia, Spain | ||
593 | |a Universidad Complutense de Madrid, Madrid, Spain | ||
593 | |a Universidad de Alcalá, Alcalá de Henares (Madrid), Spain | ||
593 | |a Universidad de Granada, C.A.F.P.E., Granada, Spain | ||
593 | |a Universidad de Santiago de Compostela, Spain | ||
593 | |a School of Physics and Astronomy, University of Leeds, United Kingdom | ||
593 | |a Argonne National Laboratory, Argonne, IL, United States | ||
593 | |a Case Western Reserve University, Cleveland, OH, United States | ||
593 | |a Colorado School of Mines, Golden, CO, United States | ||
593 | |a Colorado State University, Fort Collins, CO, United States | ||
593 | |a Colorado State University, Pueblo, CO, United States | ||
593 | |a Fermilab, Batavia, IL, United States | ||
593 | |a Los Alamos National Laboratory, Los Alamos, NM, United States | ||
593 | |a Louisiana State University, Baton Rouge, LA, United States | ||
593 | |a Michigan Technological University, Houghton, MI, United States | ||
593 | |a New York University, New York, NY, United States | ||
593 | |a Northeastern University, Boston, MA, United States | ||
593 | |a Ohio State University, Columbus, OH, United States | ||
593 | |a Pennsylvania State University, University Park, PA, United States | ||
593 | |a University of Chicago, Enrico Fermi Institute, Chicago, IL, United States | ||
593 | |a University of Hawaii, Honolulu, HI, United States | ||
593 | |a University of Nebraska, Lincoln, NE, United States | ||
593 | |a University of New Mexico, Albuquerque, NM, United States | ||
593 | |a University of Wisconsin, Madison, WI, United States | ||
593 | |a University of Wisconsin, Milwaukee, WI, United States | ||
593 | |a Institute for Nuclear Science and Technology (INST), Hanoi, Viet Nam | ||
593 | |a Konan University, Japan | ||
593 | |a Universidad Autonoma, Spain | ||
593 | |a University of Maryland, United States | ||
593 | |a NYU Abu Dhabi, United Arab Emirates | ||
690 | 1 | 0 | |a COSMIC RAY EXPERIMENTS |
690 | 1 | 0 | |a ULTRA HIGH ENERGY COSMIC RAYS |
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856 | 4 | 0 | |u https://doi.org/10.1088/1475-7516/2013/02/026 |x doi |y DOI |
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