التفاصيل البيبلوغرافية
| العنوان: |
Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory |
| المؤلفون: |
Aab, Alexander, Abreu, Pedro, Aglietta, Marco, Al Samarai, Imen, Albuquerque, Ivone, Allekotte, Ingomar, Almela, Alejandro, Alvarez Castillo, Jesus, Alvarez-Muñiz, Jaime, Anastasi, Gioacchino Alex, Anchordoqui, Luis, Andrada, Belén, Andringa, Sofia, Aramo, Carla, Arqueros, Fernando, Arsene, Nicusor, Asorey, Hernán Gonzalo, Assis, Pedro, Aublin, Julien, Avila, Gualberto, Badescu, Alina Mihaela, Balaceanu, Alexandru, Barbato, Felicia, Barreira Luz, Ricardo Jorge, Beatty, Jim, Becker, Karl-Heinz, Bellido, Jose A, Berat, Corinne, Bertaina, Mario Edoardo, Bertou, Xavier, Biermann, Peter, Biteau, Jonathan, Blaess, Simon G, Blanco, Alberto, Blazek, Jiri, Bleve, Carla, Boháčová, Martina, Boncioli, Denise, Bonifazi, Carla, Borodai, Nataliia, Botti, Ana Martina, Brack, Jeffrey, Brancus, Iliana, Bretz, Thomas, Bridgeman, Ariel, Briechle, Florian Lukas, Buchholz, Peter, Bueno, Antonio, Buitink, Stijn, Buscemi, Mario, Caballero-Mora, Karen S, Caccianiga, Lorenzo, Cancio, Ángel, Canfora, Fabrizia, Caramete, Laurentiu, Caruso, Rossella, Castellina, Antonella, Catalani, Fernando, Cataldi, Gabriella, Cazon, Lorenzo, Chavez, Alan G, Chinellato, Jose Augusto, Chudoba, Jiri, Clay, Roger W, Cobos, Agustín, Colalillo, Roberta, Coleman, Alan, Collica, Laura, Coluccia, Maria Rita, Conceição, Ruben, Consolati, Giovanni, Contreras, Fernando, Cooper, Mathew J, Coutu, Stephane, Covault, Corbin, Cronin, James, d'Amico, Stefano, Daniel, Bruno, Dasso, Sergio, Daumiller, Kai, Dawson, Bruce R, de Almeida, Rogerio M, de Jong, Sijbrand J, de Mauro, Giuseppe, de Mello Neto, Joao, de Mitri, Ivan, de Oliveira, Jaime, de Souza, Vitor, Debatin, Joachim, Deligny, Olivier, Díaz Castro, Mary Lucia, Diogo, Francisco, Dobrigkeit, Carola, d'Olivo, Juan Carlos, Dorosti, Qader, dos Anjos, Rita, Dova, Maria Teresa, Dundovic, Andrej, Ebr, Jan, Engel, Ralph, Erdmann, Martin, Erfani, Mona, Escobar, Carlos O, Espadanal, João, Etchegoyen, Alberto, Falcke, Heino, Farmer, John, Farrar, Glennys, Fauth, Anderson, Fazzini, Norberto, Fenu, Francesco, Fick, Brian, Figueira, Juan Manuel, Filipčič, Andrej, Fratu, Octavian, Freire, Martín Miguel, Fujii, Toshihiro, Fuster, Alan, Gaior, Romain, García, Beatriz, Garcia-Pinto, Diego, Gaté, Florian, Gemmeke, Hartmut, Gherghel-Lascu, Alexandru, Ghia, Piera Luisa, Giaccari, Ugo, Giammarchi, Marco, Giller, Maria, Głas, Dariusz, Glaser, Christian, Golup, Geraldina, Gómez Berisso, Mariano, Gómez Vitale, Primo F, González, Nicolás, Gorgi, Alessio, Gorham, Peter, Grillo, Aurelio, Grubb, Trent D, Guarino, Fausto, Guedes, Germano, Halliday, Robert, Hampel, Matías Rolf, Hansen, Patricia, Harari, Diego, Harrison, Thomas A, Harton, John, Haungs, Andreas, Hebbeker, Thomas, Heck, Dieter, Heimann, Philipp, Herve, Alexander E, Hill, Gary C, Hojvat, Carlos, Holt, Ewa, Homola, Piotr, Hörandel, Jörg, Horvath, Pavel, Hrabovský, Miroslav, Huege, Tim, Hulsman, Johannes, Insolia, Antonio, Isar, Paula Gina, Jandt, Ingolf, Johnsen, Jeffrey A, Josebachuili, Mariela, Jurysek, Jakub, Kääpä, Alex, Kambeitz, Olga, Kampert, Karl-Heinz, Keilhauer, Bianca, Kemmerich, Nikolas, Kemp, Ernesto, Kemp, Julian, Kieckhafer, Roger, Klages, Hans, Kleifges, Matthias, Kleinfeller, Jonny, Krause, Raphael, Krohm, Nicole, Kuempel, Daniel, Kukec Mezek, Gasper, Kunka, Norbert, Kuotb Awad, Alaa, Lago, Bruno L, Lahurd, Danielle, Lang, Rodrigo Guedes, Lauscher, Markus, Legumina, Remigiusz, Leigui de Oliveira, Marcelo Augusto, Letessier-Selvon, Antoine, Lhenry-Yvon, Isabelle, Link, Katrin, Lo Presti, Domenico, Lopes, Luis, López, Rebeca, López Casado, Aida, Lorek, Ryan, Luce, Quentin, Lucero, Agustin, Malacari, Max, Mallamaci, Manuela, Mandat, Dusan, Mantsch, Paul, Mariazzi, Analisa, Mariş, Ioana, Marsella, Giovanni, Martello, Daniele, Martinez, Humberto, Martínez Bravo, Oscar, Masías Meza, Jimmy, Mathes, Hermann-Josef, Mathys, Sebastian, Matthews, James, Matthews, John, Matthiae, Giorgio, Mayotte, Eric, Mazur, Peter, Medina, Carlos, Medina-Tanco, Gustavo, Melo, Diego, Menshikov, Alexander, Merenda, Kevin-Druis, Michal, Stanislav, Micheletti, Maria Isabel, Middendorf, Lukas, Miramonti, Lino, Mitrica, Bogdan, Mockler, Daniela, Mollerach, Silvia, Montanet, François, Morello, Carlo, Mostafá, Miguel, Müller, Ana L, Müller, Gero, Muller, Marcio Aparecido, Müller, Sarah, Mussa, Roberto, Naranjo, Ivo, Nellen, Lukas, Nguyen, Phong H, Niculescu-Oglinzanu, Mihai, Niechciol, Marcus, Niemietz, Lukas, Niggemann, Tim, Nitz, Dave, Nosek, Dalibor, Novotny, Vladimir, Nožka, Libor, Núñez, Luis, Ochilo, Livingstone, Oikonomou, Foteini, Olinto, Angela, Palatka, Miroslav, Pallotta, Juan, Papenbreer, Philipp, Parente, Gonzalo, Parra, Alejandra, Paul, Thomas, Pech, Miroslav, Pedreira, Francisco, Pękala, Jan, Pelayo, Rodrigo, Peña-Rodriguez, Jesús, Pereira, Luiz Augusto, Perlin, Matías, Perrone, Lorenzo, Peters, Christine, Petrera, Sergio, Phuntsok, Jamyang, Piegaia, Ricardo, Pierog, Tanguy, Pimenta, Mário, Pirronello, Valerio, Platino, Manuel, Plum, Matthias, Porowski, Czeslaw, Prado, Raul Ribeiro, Privitera, Paolo, Prouza, Michael, Quel, Eduardo J, Querchfeld, Sven, Quinn, Sean, Ramos-Pollan, Raúl, Rautenberg, Julian, Ravignani, Diego, Ridky, Jan, Riehn, Felix, Risse, Markus, Ristori, Pablo, Rizi, Vincenzo, Rodrigues de Carvalho, Washington, Rodriguez Fernandez, Gonzalo, Rodriguez Rojo, Jorge Rubén, Rogozin, Dmytro, Roncoroni, Matías J, Roth, Markus, Roulet, Esteban, Rovero, Adrian, Ruehl, Philip, Saffi, Steven J, Saftoiu, Alexandra, Salamida, Francesco, Salazar, Humberto, Saleh, Ahmed, Salesa Greus, Francisco, Salina, Gaetano, Sánchez, Federico, Sanchez-Lucas, Patricia, Moura Santos, Edivaldo, Santos, Eva, Sarazin, Fred, Sarmento, Raul, Sarmiento-Cano, Christian, Sato, Ricardo, Schauer, Markus, Scherini, Viviana, Schieler, Harald, Schimp, Michael, Schmidt, David, Scholten, Olaf, Schovánek, Petr, Schröder, Frank G, Schröder, Sonja, Schulz, Alexander, Schumacher, Johannes, Sciutto, Sergio, Segreto, Alberto, Shadkam, Amir, Shellard, Ronald C, Sigl, Guenter, Silli, Gaia, Sima, Octavian, Śmiałkowski, Andrzej, Šmída, Radomir, Snow, Gregory, Sommers, Paul, Sonntag, Sebastian, Squartini, Ruben, Stanca, Denis, Stanič, Samo, Stasielak, Jaroslaw, Stassi, Patrick, Stolpovskiy, Mikhail, Strafella, Francesco, Streich, Alexander, Suarez, Federico, Suarez Durán, Mauricio, Sudholz, Tristan, Suomijärvi, Tiina, Supanitsky, a Daniel, Šupík, Jan, Swain, John, Szadkowski, Zbigniew, Taboada, Alvaro, Taborda, Oscar Alejandro, Theodoro, Vanessa Menezes, Timmermans, Charles, Todero Peixoto, Carlos J, Tomankova, Lenka, Tomé, Bernardo, Torralba Elipe, Guillermo, Travnicek, Petr, Trini, Marta, Ulrich, Ralf, Unger, Michael, Urban, Martin, Valdés Galicia, Jose F, Valiño, Ines, Valore, Laura, van Aar, Guus, van Bodegom, Patrick, van den Berg, Ad M, van Vliet, Arjen, Varela, Enrique, Vargas Cárdenas, Bernardo, Varner, Gary, Vázquez, Ricardo, Veberič, Darko, Ventura, Cynthia, Vergara Quispe, Indira D, Verzi, Valerio, Vicha, Jakub, Villaseñor, Luis, Vorobiov, Serguei, Wahlberg, Hernan, Wainberg, Oscar, Walz, David, Watson, Alan, Weber, Marc, Weindl, Andreas, Wiencke, Lawrence, Wilczyński, Henryk, Wirtz, Marcus, Wittkowski, David, Wundheiler, Brian, Yang, Lili, Yushkov, Alexey, Zas, Enrique, Zavrtanik, Danilo, Zavrtanik, Marko, Zepeda, Arnulfo, Zimmermann, Benedikt, Ziolkowski, Michael, Zong, Zizhao, Zuccarello, Francesca |
| المساهمون: |
Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes 2016-2019 (UGA 2016-2019 ), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom Paris (IMT)-Institut Mines-Télécom Paris (IMT), Pierre Auger, ANR-11-IDEX-0004,SUPER,Sorbonne Universités à Paris pour l'Enseignement et la Recherche(2011) |
| المصدر: |
ISSN: 1550-7998. |
| بيانات النشر: |
HAL CCSD
American Physical Society |
| سنة النشر: |
2017 |
| المجموعة: |
Université de Nantes: HAL-UNIV-NANTES |
| مصطلحات موضوعية: |
96.50.S-, 96.50.sb, 96.50.sd, 98.70.Sa, showers: atmosphere, interaction: model, mass spectrum, observatory, Auger, fluorescence, energy dependence, electromagnetic, calibration, statistical, muon, Cherenkov counter, water, air, UHE, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
| الوصف: |
International audience ; We present a new method for probing the hadronic interaction models at ultrahigh energy and extracting details about mass composition. This is done using the time profiles of the signals recorded with the water-Cherenkov detectors of the Pierre Auger Observatory. The profiles arise from a mix of the muon and electromagnetic components of air showers. Using the risetimes of the recorded signals, we define a new parameter, which we use to compare our observations with predictions from simulations. We find, first, inconsistencies between our data and predictions over a greater energy range and with substantially more events than in previous studies. Second, by calibrating the new parameter with fluorescence measurements from observations made at the Auger Observatory, we can infer the depth of shower maximum Xmax for a sample of over 81,000 events extending from 0.3 to over 100 EeV. Above 30 EeV, the sample is nearly 14 times larger than what is currently available from fluorescence measurements and extending the covered energy range by half a decade. The energy dependence of ⟨Xmax⟩ is compared to simulations and interpreted in terms of the mean of the logarithmic mass. We find good agreement with previous work and extend the measurement of the mean depth of shower maximum to greater energies than before, reducing significantly the statistical uncertainty associated with the inferences about mass composition. |
| نوع الوثيقة: |
article in journal/newspaper |
| اللغة: |
English |
| العلاقة: |
info:eu-repo/semantics/altIdentifier/arxiv/1710.07249; hal-01669441; https://hal.science/hal-01669441Test; ARXIV: 1710.07249; INSPIRE: 1631620 |
| DOI: |
10.1103/PhysRevD.96.122003 |
| الإتاحة: |
https://doi.org/10.1103/PhysRevD.96.122003Test
https://hal.science/hal-01669441Test |
| رقم الانضمام: |
edsbas.9F5BC039 |
| قاعدة البيانات: |
BASE |
