Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/60499
Type: Artigo de periódico
Title: Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory
Author: Abreu, P
Aglietta, M
Ahlers, M
Ahn, EJ
Albuquerque, IFM
Allekotte, I
Allen, J
Allison, P
Almela, A
Castillo, JA
Alvarez-Muniz, J
Batista, RA
Ambrosio, M
Aminaei, A
Anchordoqui, L
Andringa, S
Anticic, T
Aramo, C
Arqueros, F
Asorey, H
Assis, P
Aublin, J
Ave, M
Avenier, M
Avila, G
Badescu, AM
Barber, KB
Barbosa, AF
Bardenet, R
Baughman, B
Bauml, J
Baus, C
Beatty, JJ
Becker, KH
Belletoile, A
Bellido, JA
BenZvi, S
Berat, C
Bertou, X
Biermann, PL
Billoir, P
Blanco, F
Blanco, M
Bleve, C
Blumer, H
Bohacova, M
Boncioli, D
Bonifazi, C
Bonino, R
Borodai, N
Brack, J
Brancus, I
Brogueira, P
Brown, WC
Buchholz, P
Bueno, A
Buroker, L
Burton, RE
Buscemi, M
Caballero-Mora, KS
Caccianiga, B
Caccianiga, L
Caramete, L
Caruso, R
Castellina, A
Cataldi, G
Cazon, L
Cester, R
Cheng, SH
Chiavassa, A
Chinellato, JA
Chudoba, J
Cilmo, M
Clay, RW
Cocciolo, G
Colalillo, R
Collica, L
Coluccia, MR
Conceicao, R
Contreras, F
Cook, H
Cooper, MJ
Coppens, J
Coutu, S
Covault, CE
Criss, A
Cronin, J
Curutiu, A
Dallier, R
Daniel, B
Dasso, S
Daumiller, K
Dawson, BR
de Almeida, RM
De Domenico, M
de Jong, SJ
De La Vega, G
de Mello, WJM
de Mello, JRT
De Mitri, I
de Souza, V
de Vries, KD
del Peral, L
Deligny, O
Dembinski, H
Dhital, N
Di Giulio, C
Diaz, JC
Castro, MLD
Diep, PN
Diogo, F
Dobrigkeit, C
Docters, W
D'Olivo, JC
Dong, PN
Dorofeev, A
dos Anjos, JC
Dova, MT
D'Urso, D
Ebr, J
Engel, R
Erdmann, M
Escobar, CO
Espadanal, J
Etchegoyen, A
San Luis, PF
Falcke, H
Fang, K
Farrar, G
Fauth, AC
Fazzini, N
Ferguson, AP
Fick, B
Figueira, JM
Filevich, A
Filipcic, A
Fliescher, S
Fox, BD
Fracchiolla, CE
Fraenkel, ED
Fratu, O
Frohlich, U
Fuchs, B
Gaior, R
Gamarra, RF
Gambetta, S
Garcia, B
Roca, STG
Garcia-Gamez, D
Garcia-Pinto, D
Garilli, G
Bravo, AG
Gemmeke, H
Ghia, PL
Giller, M
Gitto, J
Glaser, C
Glass, H
Golup, G
Albarracin, FG
Berisso, MG
Vitale, PFG
Goncalves, P
Gonzalez, JG
Gookin, B
Gorgi, A
Gorham, P
Gouffon, P
Grebe, S
Griffith, N
Grillo, AF
Grubb, TD
Guardincerri, Y
Guarino, F
Guedes, GP
Hansen, P
Harari, D
Harrison, TA
Harton, JL
Haungs, A
Hebbeker, T
Heck, D
Herve, AE
Hill, GC
Hojvat, C
Hollon, N
Holmes, VC
Homola, P
Horandel, JR
Horvath, P
Hrabovsky, M
Huber, D
Huege, T
Insolia, A
Ionita, F
Jansen, S
Jarne, C
Jiraskova, S
Josebachuili, M
Kadija, K
Kampert, KH
Karhan, P
Kasper, P
Katkov, I
Kegl, B
Keilhauer, B
Keivani, A
Kelley, JL
Kemp, E
Kieckhafer, RM
Klages, HO
Kleifges, M
Kleinfeller, J
Knapp, J
Kotera, K
Krause, R
Krohm, N
Kromer, O
Kruppke-Hansen, D
Kuempel, D
Kulbartz, JK
Kunka, N
La Rosa, G
LaHurd, D
Latronico, L
Lauer, R
Lauscher, M
Lautridou, P
Le Coz, S
Leao, MSAB
Lebrun, D
Lebrun, P
de Oliveira, MAL
Letessier-Selvon, A
Lhenry-Yvon, I
Link, K
Lopez, R
Aguera, AL
Louedec, K
Bahilo, JL
Lu, L
Lucero, A
Ludwig, M
Lyberis, H
Maccarone, MC
Macolino, C
Malacari, M
Maldera, S
Maller, J
Mandat, D
Mantsch, P
Mariazzi, AG
Marin, J
Marin, V
Maris, IC
Falcon, HRM
Marsella, G
Martello, D
Martin, L
Martinez, H
Bravo, OM
Martraire, D
Meza, JJM
Mathes, HJ
Matthews, J
Matthews, JAJ
Matthiae, G
Maurel, D
Maurizio, D
Mayotte, E
Mazur, PO
Medina-Tanco, G
Melissas, M
Melo, D
Menichetti, E
Menshikov, A
Messina, S
Meyhandan, R
Micanovic, S
Micheletti, MI
Middendorf, L
Minaya, IA
Miramonti, L
Mitrica, B
Molina-Bueno, L
Mollerach, S
Monasor, M
Ragaigne, DM
Montanet, F
Morales, B
Morello, C
Moreno, JC
Mostafa, M
Moura, CA
Muller, MA
Muller, G
Munchmeyer, M
Mussa, R
Navarra, G
Navarro, JL
Navas, S
Necesal, P
Nellen, L
Nelles, A
Neuser, J
Nhung, PT
Niechciol, M
Niemietz, L
Nierstenhoefer, N
Niggemann, T
Nitz, D
Nosek, D
Nozka, L
Oehlschlager, J
Olinto, A
Oliveira, M
Ortiz, M
Pacheco, N
Selmi-Dei, DP
Palatka, M
Pallotta, J
Palmieri, N
Parente, G
Parra, A
Pastor, S
Paul, T
Pech, M
Pekala, J
Pelayo, R
Pepe, IM
Perrone, L
Pesce, R
Petermann, E
Petrera, S
Petrolini, A
Petrov, Y
Pfendner, C
Piegaia, R
Pierog, T
Pieroni, P
Pimenta, M
Pirronello, V
Platino, M
Plum, M
Ponce, VH
Pontz, M
Porcelli, A
Privitera, P
Prouza, M
Quel, EJ
Querchfeld, S
Rautenberg, J
Ravel, O
Ravignani, D
Revenu, B
Ridky, J
Riggi, S
Risse, M
Ristori, P
Rivera, H
Rizi, V
Roberts, J
de Carvalho, WR
Cabo, IR
Fernandez, GR
Martino, JR
Rojo, JR
Rodriguez-Frias, MD
Ros, G
Rosado, J
Rossler, T
Roth, M
Rouille-d'Orfeuil, B
Roulet, E
Rovero, AC
Ruhle, C
Saffi, SJ
Saftoiu, A
Salamida, F
Salazar, H
Greus, FS
Salina, G
Sanchez, F
Santo, CE
Santos, E
Santos, EM
Sarazin, F
Sarkar, B
Sato, R
Scharf, N
Scherini, V
Schieler, H
Schiffer, P
Schmidt, A
Scholten, O
Schoorlemmer, H
Schovancova, J
Schovanek, P
Schroder, F
Schulz, J
Schuster, D
Sciutto, SJ
Scuderi, M
Segreto, A
Settimo, M
Shadkam, A
Shellard, RC
Sidelnik, I
Sigl, G
Sima, O
Smialkowski, A
Smida, R
Snow, GR
Sommers, P
Sorokin, J
Spinka, H
Squartini, R
Srivastava, YN
Stanic, S
Stapleton, J
Stasielak, J
Stephan, M
Straub, M
Stutz, A
Suarez, F
Suomijarvi, T
Supanitsky, AD
Susa, T
Sutherland, MS
Swain, J
Szadkowski, Z
Szuba, M
Tapia, A
Tartare, M
Tascau, O
Tcaciuc, R
Thao, NT
Thomas, D
Tiffenberg, J
Timmermans, C
Tkaczyk, W
Peixoto, CJT
Toma, G
Tomankova, L
Tome, B
Tonachini, A
Elipe, GT
Machado, DT
Travnicek, P
Tridapalli, DB
Trovato, E
Tueros, M
Ulrich, R
Unger, M
Urban, M
Galicia, JFV
Valino, I
Valore, L
van Aar, G
van den Berg, AM
van Velzen, S
van Vliet, A
Varela, E
Cardenas, BV
Varner, G
Vazquez, JR
Vazquez, RA
Veberic, D
Verzi, V
Vicha, J
Videla, M
Villasenor, L
Wahlberg, H
Wahrlich, P
Wainberg, O
Walz, D
Watson, AA
Weber, M
Weidenhaupt, K
Weindl, A
Werner, F
Westerhoff, S
Whelan, BJ
Widom, A
Wieczorek, G
Wiencke, L
Wilczynska, B
Wilczynski, H
Will, M
Williams, C
Winchen, T
Wommer, M
Wundheiler, B
Yamamoto, T
Yapici, T
Younk, P
Yuan, G
Yushkov, A
Garcia, BZ
Zas, E
Zavrtanik, D
Zavrtanik, M
Zaw, I
Zepeda, A
Zhou, J
Zhu, Y
Silva, MZ
Ziolkowski, M
Abstract: 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.
Subject: ultra high energy cosmic rays
cosmic ray experiments
Country: Inglaterra
Editor: Iop Publishing Ltd
Rights: fechado
Identifier DOI: 10.1088/1475-7516/2013/02/026
Date Issue: 2013
Appears in Collections:Unicamp - Artigos e Outros Documentos

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