Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory

Aab A, Abreu P, Aglietta M, Ahn EJ, Al Samarai I, Albuquerque IFM, Allekotte I, Allison P, Almela A, Alvarez Castillo J, Alvarez-Muniz J, Batista RA, Ambrosio M, Anchordoqui L, Andrada B, Andringa S, Aramo C, Arqueros F, Arsene N, Asorey H, Assis PJS, Aublin J, Avila G, Awal N, Badescu AM, Baus C, Beatty JJ, Becker KH, Bellido JA, Berat C, Bertaina ME, Bertou X, Biermann PL, Billoir P, Blaess SG, Blanco A, Blazek J, Bleve C, Blumer H, Bohacova M, Boncioli D, Bonifazi C, Borodai N, Botti AM, Brack J, Brancus I, Bretz T, Bridgeman A, Briechle FL, Buchholz P, Bueno A, Buitink S, Buscemi M, Caballero-Mora KS, Caccianiga B, Caccianiga L, Cancio A, Candusso M, Caramete L, Caruso R, Castellina A, Cataldi G, Cazon L, Cester R, Chavez AG, Chiavassa A, Chinellato JA, Diaz JCC, Chudoba J, Clay RW, Colalillo R, Coleman A, Collica L, Coluccia MR, Conceicao R, Contreras F, Cooper MJ, Coutu S, Covault CE, Cronin J, Dallier R, D'Amico S, Daniel B, Dasso S, Daumiller K, Dawson BR, De Almeida RM, De Jong SJ, De Mauro G, Neto JRTDM, De Mitri I, De Oliveira J, De Souza V, Debatin J, Deligny O, Dhital N, Di Giulio C, Di Matteo A, Castro MLD, Diogo F, Dobrigkeit C, Docters W, D'Olivo JC, Dorofeev A, Dos Anjos RC, Dova MT, Dundovic A, Ebr J, Engel R, Erdmann M, Erfani M, Escobar CO, Espadanal J, Etchegoyen A, Falcke H, Fang K, Farrar G, Fauth AC, Fazzini N, Ferguson AP, Fick B, Figueira JM, Filevich A, Filipcic A, Fratu O, Freire MM, Fujii T, Fuster A, Gallo F, Garcia B, Garcia-Pinto D, Gate F, Gemmeke H, Gherghel-Lascu A, Ghia PL, Giaccari U, Giammarchi M, Giller M, Glas D, Glaser C, Glass H, Golup G, Gomez Berisso M, Gomez Vitale PF, Gonzalez N, Gookin B, Gordon J, Gorgi A, Gorham P, Gouffon P, Griffith N, Grillo AF, Grubb TD, Guarino F, Guedes GP, Hampel MR, Hansen P, Harari D, Harrison TA, Harton JL, Hasankiadeh Q, Haungs A, Hebbeker T, Heck D, Heimann P, Herve AE, Hill GC, Hojvat C, Hollon N, Holt E, Homola P, Hoerandel JR, Horvath P, Hrabovsky M, Huege T, Insolia A, Isar PG, Jandt I, Jansen S, Jarne C, Johnsen JA, Josebachuili M, Kaeaepae A, Kambeitz O, Kampert KH, Kasper P, Katkov I, Keilhauer B, Kemp E, Kieckhafer RM, Klages HO, Kleifges M, Kleinfeller J, Krause R, Krohm N, Kuempel D, Mezek GK, Kunka N, Awad AK, Lahurd D, Latronico L, Lauscher M, Lautridou P, Lebrun P, De Oliveira MAL, Letessier-Selvon A, Lhenry-Yvon I, Link K, Lopes L, Lopez R, Casado AL, Lucero A, Malacari M, Mallamaci M, Mandat D, Mantsch P, Mariazzi AG, Marin V, Maris IC, Marsella G, Martello D, Martinez H, Martinez Bravo O, Masias Meza JJ, Mathes HJ, Mathys S, Matthews J, Matthews JAJ, Matthiae G, Maurizio D, Mayotte E, Mazur PO, Medina C, Medina-Tanco G, Mello VBB, Melo D, Menshikov A, Messina S, Micheletti MI, Middendorf L, Minaya IA, Miramonti L, Mitrica B, Molina-Bueno L, Mollerach S, Montanet F, Morello C, Mostafa M, Moura CA, Mueller G, Muller MA, Mueller S, Naranjo I, Navas S, Necesal P, Nellen L, Nelles A, Neuser J, Nguyen PH, Niculescu-Oglinzanu M, Niechciol M, Niemietz L, Niggemann T, Nitz D, Nosek D, Novotny V, Nozka H, Nunez LA, Ochilo L, Oikonomou F, Olinto A, Selmi-Dei DP, Palatka M, Pallotta J, Papenbreer P, Parente G, Parra A, Paul T, Pech M, Pekala J, Pelayo R, Pena-Rodriguez J, Pepe IM, Pereira LAS, Perrone L, Petermann E, Peters C, Petrera S, Phuntsok J, Piegaia R, Pierog T, Pieroni P, Pimenta M, Pirronello V, Platino M, Plum M, Porowski C, Prado RR, Privitera P, Prouza M, Quel EJ, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Reinert D, Revenu B, Ridky J, Risse M, Ristori P, Rizi V, De Carvalho WR, Rojo JR, Rogozin D, Rosado J, Roth M, Roulet E, Rovero AC, Saffi SJ, Saftoiu A, Salazar H, Saleh A, Greus FS, Salina G, Gomez JDS, Sanchez F, Sanchez-Lucas P, Santos EM, Santos EM, Sarazin F, Sarkar B, Sarmento R, Sarmiento-Cano C, Sato R, Scarso C, Schauer M, Scherini V, Schieler H, Schmidt D, Scholten O, Schoorlemmer H, Schovanek P, Schroeder FG, Schulz A, Schulz J, Schumacher J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard C, Sigl G, Sima O, Smialkowski A, Smida R, Snow GR, Sommers P, Sonntag S, Sorokin J, Squartini R, Stanca D, Stanic S, Stapleton J, Stasielak J, Strafella F, Stutz A, Suarez F, Suarez Duran M, Sudholz T, Suomijaervi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Taborda OA, Tapia A, Tepe A, Theodoro VM, Timmermans C, Peixoto CJT, Tomankova L, Tome B, Tonachini A, Torralba Elipe G, Machado DT, Travnicek P, Trini M, Ulrich R, Unger M, Urban M, Valdes Galicia JF, Valino I, Valore L, Van Aar G, Van Bodegom P, Van Den Berg AM, Van Vliet A, Varela E, Vargas Cardenas B, Varner G, Vasquez R, Vazquez JR, Vazquez RA, Veberic D, Verzi V, Vicha J, Videla M, Villasenor L, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weindl A, Wiencke L, Wilczynski H, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yang L, Yapici T, Yelos D, Yushkov A, Zas E, Zavrtanik D, Zavrtanik M, Zepeda A, Zimmermann B, Ziolkowski M, Zong Z, Zuccarello F (2016)


Publication Status: Published

Publication Type: Journal article

Publication year: 2016

Journal

Publisher: AMER PHYSICAL SOC

Book Volume: 93

Article Number: ARTN 072006

Journal Issue: 7

DOI: 10.1103/PhysRevD.93.072006

Abstract

The azimuthal asymmetry in the risetime of signals in Auger surface detector stations is a source of information on shower development. The azimuthal asymmetry is due to a combination of the longitudinal evolution of the shower and geometrical effects related to the angles of incidence of the particles into the detectors. The magnitude of the effect depends upon the zenith angle and state of development of the shower and thus provides a novel observable, (sec theta)(max), sensitive to the mass composition of cosmic rays above 3 x 10(18) eV. By comparing measurements with predictions from shower simulations, we find for both of our adopted models of hadronic physics (QGSJETII-04 and EPOS-LHC) an indication that the mean cosmic-ray mass increases slowly with energy, as has been inferred from other studies. However, the mass estimates are dependent on the shower model and on the range of distance from the shower core selected. Thus the method has uncovered further deficiencies in our understanding of shower modeling that must be resolved before the mass composition can be inferred from (sec theta)(max).

How to cite

APA:

Aab, A., Abreu, P., Aglietta, M., Ahn, E.J., Al Samarai, I., Albuquerque, I.F.M.,... Zuccarello, F. (2016). Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory. Physical Review D, 93(7). https://dx.doi.org/10.1103/PhysRevD.93.072006

MLA:

Aab, A., et al. "Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory." Physical Review D 93.7 (2016).

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