MétaCan
Menu
Back to cohort
Record W4396592559 · doi:10.1103/physrevd.109.102001

Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory

2024· article· en· W4396592559 on OpenAlexaff
Adila Abdul Halim, P. Abreu, M. Aglietta, I. Allekotte, Kévin Almeida Cheminant, A. Almela, Roberto Aloisio, Jaime Álvarez-Muñiz, Juan Ammerman Yebra, Gioacchino Alex Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, L. Apollonio, C. Aramo, P. R. Araújo Ferreira, E. Arnone, J. C. Arteaga Velázquez, P. Assis, G. Ávila, Emanuele Avocone, Alena Bakalová, Felicia Barbato, Adriel Bartz Mocellin, Jose A. Bellido, Corinne Bérat, M. E. Bertaina, Gopal Bhatta, Marta Bianciotto, Peter L. Biermann, V. Binet, Kathrin Bismark, Teresa Bister, Jonathan Biteau, J. Blazek, C. Bleve, J. Blümer, M. Boháčová, Denise Boncioli, C. Bonifazi, L. Bonneau Arbeletche, Nataliia Borodai, J. Brack, P. G. Brichetto Orchera, F. L. Briechle, A. Bueno, S. Buitink, Mario Buscemi, Max Büsken, Anthony Bwembya, K. S. Caballero‐Mora, S. Cabana-Freire, Lorenzo Caccianiga, F. Campuzano, R. Caruso, A. Castellina, F. Catalani, G. Cataldi, Lorenzo Cazon, M. Cerda, A. Cermenati, J. A. Chinellato, J. Chudoba, L. Chytka, R. W. Clay, A. C. Cobos Cerutti, R. Colalillo, M. R. Coluccia, R. Conceição, Antonio Condorelli, Giovanni Consolati, M. Conte, Fabio Convenga, D. Correia dos Santos, Pedro J. Costa, C. E. Covault, M. Cristinziani, Carlo Salvattore Cruz Sanchez, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de Almeida, Joaquín de Jesús, S. J. de Jong, I. De Mitri, J. de Oliveira, Danelise de Oliveira Franco, V. de Souza, Beatriz de Errico, Emanuele De Vito, A. Del Popolo, O. Deligny, N. Denner, L. Deval, A. di Matteo, M. Dobre, C. Dobrigkeit, J. C. D’Olivo, Luis Miguel Domingues Mendes, Q. Dorosti, J. C. dos Anjos, R. C. dos Anjos, Jan Ebr, Fiona H. Ellwanger, M. Emam, R. Engel, Italo Epicoco, M. Erdmann, A. Etchegoyen, Carmelo Evoli, H. Falcke, G. Farrar, A. C. Fauth, N. Fazzini, F. Feldbusch, Francesco Fenu, Alexandra Fernandes, Brian Fick, J. M. Figueira, A. Filipčič, T. Fitoussi, Benjamin Flaggs, Antonio Franco, Toshihiro Fujii, A. Fuster, C. Galea, C. Galelli, B. Garćıa, Chloé Gaudu, H. Gemmeke, F. Gesualdi, A. Gherghel‐Lascu, P. L. Ghia, U. Giaccari, Jonas Glombitza, Fabian Gobbi, F. Gollan, G. Golup, M. Gómez Berisso, D. Góra, J. P. Gongora, J. M. González, Nicolás Martín González, A. Gorgi, M. Gottowik, T. D. Grubb, F. Guarino, G. P. Guedes, Eleonora Guido, Lukas Gülzow, S. R. Hahn, P. Hamal, M. R. Hampel, P. Hansen, D. Harari, V. M. Harvey, A. Haungs, T. Hebbeker, C. Hojvat, J.R. Hörandel, Pavel Horváth, Miroslav Hrabovský, T. Huege, A. Insolia, Paula Gina Isar, P. Janecek, Vlastimil Jílek, J. A. Johnsen, J. Jurysek, K.‐H. Kampert, B. Keilhauer, Abha Khakurdikar, Varada Varma Kizakke Covilakam, H. O. Klages, M. Kleifges, F. Knapp, J. Köhler, N. Kunka, Bruno L. Lago, N. Langner, M. A. Leigui de Oliveira, Yago Lema-Capeans, A. Letessier‐Selvon, Isabelle Lhenry-Yvon, L. Lopes, L. Lu, Quentin Luce, Jon Paul Lundquist, A. Machado Payeras, M. Majercakova, Dušan Mandát, Bradley C. Manning, P. Mantsch, F. M. Mariani, A. G. Mariazzi, Ioana Codrina Mariş, G. Marsella, D. Martello, Sara Martinelli, Miguel A. Martins, H.-J. Mathes, J. Matthews, G. Matthiae, Eric William Mayotte, Sonja Mayotte, P. O. Mazur, G. Medina-Tanco, J. Meinert, Diego Melo, A. Menshikov, Carmen Merx, S. Michal, M. I. Micheletti, L. Miramonti, Silvia Mollerach, F. Montanet, Leonel Morejón, C. Morello, K. Mulrey, R. Mussa, W. M. Namasaka, S. Negi, L. Nellen, K. Nguyen, G. Nicora, Marcus Niechciol, D. Nitz, Dalibor Nosek, V. Novotny, L. Nožka, A. Nucita, Luis A. Núñez, C. Oliveira, M. Palatka, J. Pallotta, Subhasis Panja, G. Parente, T. Paulsen, J. Pawlowsky, M. Pech, J. Pȩkala, Rodrigo Pelayo, Luiz Augusto Pereira, E. E. Pereira Martins, J. Perez Armand, C. Pérez Bertolli, L. Perrone, S. Petrera, C. Petrucci, T. Pierog, M. Pimenta, M. Platino, B. Pont, Mart Pothast, Mohsen Pourmohammad Shahvar, P. Privitera, M. Prouza, S. Querchfeld, J. Rautenberg, D. Ravignani, João Vítor Reginatto Akim, M. Reininghaus, J. Řídký, Felix Riehn, Markus Risse, V. Rizi, W. Rodrigues de Carvalho, E. Rodrı́guez, J. Rodriguez Rojo, M. J. Roncoroni, S. Rossoni, M. Roth, E. Roulet, A. C. Rovero, P. Ruehl, A. Sǎftoiu, M. Saharan, F. Salamida, H. Salazar, G. Salina, Jose Sanabria Gomez, F. Sánchez, Eva Santos, E. Santos, F. Sarazin, R. Sarmento, Ricardo Sato, Pierpaolo Savina, C. M. Schäfer, V. Scherini, H. Schieler, Martin Schimassek, M. Schimp, D. Schmidt, O. Scholten, H. Schoorlemmer, P. Schovánek, Frank Schröder, J. Schulte, T. Schulz, Sergio J Sciutto, M. Scornavacche, Adrian Sedoski, A. Segreto, S. Sehgal, S. U. Shivashankara, G. Sigl, G. Silli, O. Sima, Katarína Simkova, F. Simon, Raluca Smău, Radomir Šmída, P. Sommers, J. F. Soriano, R. Squartini, Maximilian Stadelmaier, S. Stanič, Jarosław Stasielak, P. Stassi, S. Strähnz, M. Straub, T. Suomijärvi, A. D. Supanitsky, Zuzana Svozilikova, Zbigniew Szadkowski, Fedor Tairli, A. Tapia, C. Taricco, Charles Timmermans, O. Tkachenko, P. Tobiska, Carlos J. Todero Peixoto, B. Tomé, Z. Torrès, Andres Travaini, P. Trávnı́ček, C. Trimarelli, Matias Jorge Tueros, M. Unger, Lukáš Vaclavek, Martin Vacula, J. F. Valdés Galicia, L. Valore, Enrique Varela, A. Vásquez-Ramírez, D. Veberič, Cynthia Ventura, I. D. Vergara Quispe, V. Verzi, J. Vícha, J. Vink, S. Vorobiov, C. Watanabe, A. Weindl, L. Wiencke, H. Wilczyński, D. Wittkowski, Brian Wundheiler, Bin Yue, Alexey Yushkov, Orazio Zapparrata, E. Zas, D. Zavrtanik, M. Zavrtanik

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsInstitute of Particle Physics
FundersColegiul Consultativ pentru Cercetare-Dezvoltare şi InovareInstitut Lagrange de ParisInstitut National de Physique Nucléaire et de Physique des ParticulesInstituto Nazionale di Fisica NucleareAgencia Nacional de Promoción Científica y TecnológicaFundação para a Ciência e a TecnologiaAustralian Research CouncilMinistero dell'Università e della RicercaHelmholtz Alliance for Astroparticle PhysicsMinisterium für Kultur und Wissenschaft des Landes Nordrhein-WestfalenDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekBundesministerium für Bildung, Wissenschaft und ForschungIstituto Nazionale di Fisica NucleareJavna Agencija za Raziskovalno Dejavnost RSVlaamse regeringJunta de AndalucíaHelmholtz-GemeinschaftStrongXunta de GaliciaMinisterio de Asuntos Económicos y Transformación Digital, Gobierno de EspañaMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenUniversité Paris-SaclayFinanciadora de Estudos e ProjetosUnitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si InovariiMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesIstituto Nazionale di AstrofisicaUniversidad Nacional Autónoma de MéxicoCentre National de la Recherche ScientifiqueU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroFonds De La Recherche Scientifique - FNRSConselho Nacional de Desenvolvimento Científico e TecnológicoNarodowe Centrum NaukiConseil Régional, Île-de-FranceDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaMinistry of Education and Science of the Russian FederationMinistero dell’Istruzione, dell’Università e della RicercaMinisterium für Wissenschaft, Forschung und Kunst Baden-WürttembergFonds Wetenschappelijk OnderzoekGrantová Agentura České RepublikyConsejo Nacional de Investigaciones Científicas y TécnicasMinisterstvo Školství, Mládeže a TělovýchovyMinisterio de Economía y CompetitividadBundesministerium für Bildung und ForschungMinistry of Education, Culture, Sports, Science and TechnologyMinistero degli Affari Esteri e della Cooperazione InternazionaleComisión Nacional de Investigación Científica y TecnológicaGrainger FoundationAgence Nationale de la RechercheMarie CurieEuropean CommissionFundação de Amparo à Pesquisa do Estado de São PauloUnited Nations Educational, Scientific and Cultural OrganizationConsellería de Cultura, Educación e Ordenación Universitaria, Xunta de GaliciaMinisterul Cercetării, Inovării şi DigitalizăriiCorporation for National and Community ServiceNational Science Foundation
KeywordsPierre Auger ObservatoryShowerAir showerHadronObservatoryPhysicsNuclear physicsParticle (ecology)AstrophysicsGeologyCosmic ray

Abstract

fetched live from OpenAlex

We test the predictions of hadronic interaction models regarding the depth of maximum of air-shower profiles, <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>X</a:mi><a:mi>max</a:mi></a:msub></a:math>, and ground-particle signals in water-Cherenkov detectors at 1000 m from the shower core, <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>S</c:mi><c:mo stretchy="false">(</c:mo><c:mn>1000</c:mn><c:mo stretchy="false">)</c:mo></c:math>, using the data from the fluorescence and surface detectors of the Pierre Auger Observatory. The test consists of fitting the measured two-dimensional (<g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:mi>S</g:mi><g:mo stretchy="false">(</g:mo><g:mn>1000</g:mn><g:mo stretchy="false">)</g:mo></g:math>, <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:msub><k:mi>X</k:mi><k:mi>max</k:mi></k:msub></k:math>) distributions using templates for simulated air showers produced with hadronic interaction models pos-, et--04, 2.3d and leaving the scales of predicted <m:math xmlns:m="http://www.w3.org/1998/Math/MathML" display="inline"><m:msub><m:mi>X</m:mi><m:mi>max</m:mi></m:msub></m:math> and the signals from hadronic component at ground as free-fit parameters. The method relies on the assumption that the mass composition remains the same at all zenith angles, while the longitudinal shower development and attenuation of ground signal depend on the mass composition in a correlated way. The analysis was applied to 2239 events detected by both the fluorescence and surface detectors of the Pierre Auger Observatory with energies between <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"><o:msup><o:mn>10</o:mn><o:mn>18.5</o:mn></o:msup><o:mtext> </o:mtext><o:mtext> </o:mtext><o:mi>eV</o:mi></o:math> to <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"><q:msup><q:mn>10</q:mn><q:mn>19.0</q:mn></q:msup><q:mtext> </q:mtext><q:mtext> </q:mtext><q:mi>eV</q:mi></q:math> and zenith angles below 60°. We found, that within the assumptions of the method, the best description of the data is achieved if the predictions of the hadronic interaction models are shifted to deeper <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"><s:msub><s:mi>X</s:mi><s:mi>max</s:mi></s:msub></s:math> values and larger hadronic signals at all zenith angles. Given the magnitude of the shifts and the data sample size, the statistical significance of the improvement of data description using the modifications considered in the paper is larger than <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"><u:mn>5</u:mn><u:mi>σ</u:mi></u:math> even for any linear combination of experimental systematic uncertainties. Published by the American Physical Society 2024

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.630
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.061
GPT teacher head0.392
Teacher spread0.331 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations26
Published2024
Admission routes1
Has abstractyes

Explore more

Same venuePhysical review. D/Physical review. D.Same topicAstrophysics and Cosmic PhenomenaFrench-language works237,207