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Since 2006, EPOS hadronic interaction model is being used for very high energy cosmic ray analysis. Designed for minimum bias particle physics and used for having a precise description of SPS and RHIC heavy ion collisions, EPOS brought more…

High Energy Astrophysical Phenomena · Physics 2010-11-17 T. Pierog , Iu. Karpenko , S. Porteboeuf , K. Werner

The description of high-energy hadronic interactions plays an important role in the (astrophysical) interpretation of air shower data. The parameter space important for the development of air showers (energy and kinematical range) extends…

High Energy Astrophysical Phenomena · Physics 2015-06-30 J. R. Hoerandel

KASCADE-Grande, the extension of the multi-detector setup of KASCADE, was devoted to measure the properties of extensive air showers initiated by high-energy cosmic rays in the primary energy range of 1 PeV up to 1 EeV. The observations of…

In this article, I will review how observations performed with extensive air showers are being used to probe hadronic interactions at high energy. I will briefly overview the new studies exploring the connection between the dynamics of air…

High Energy Physics - Experiment · Physics 2019-09-09 Lorenzo Cazon

Extensive air showers are complex objects, resulting of billions of particle reactions initiated by single cosmic ray at ultra-high-energy. Their characteristics are sensitive both to the mass of the primary cosmic ray and to the details of…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Lorenzo Cazon

High-energy collisions at the High-Luminosity Large Hadron Collider (HL-LHC) will generate a substantial flux of particles along the beam collision axis that current LHC experiments cannot access. Multi-particle production in the…

High Energy Physics - Experiment · Physics 2024-07-08 Dennis Soldin

Studies of the nature of cosmic ray particles at the highest energies are based on the measurement of extensive air showers. Most cosmic ray properties can therefore only be obtained from the interpretation of air shower data and are thus…

High Energy Physics - Phenomenology · Physics 2011-03-31 Ralf Ulrich , Ralph Engel , Michael Unger

The hadron production in the simulation of extensive air showers is a long standing problem and the origin of large uncertainties in the reconstruction of the mass of the high energy primary cosmic rays. Hadronic interaction models re-tuned…

High Energy Astrophysical Phenomena · Physics 2025-08-12 Tanguy Pierog , Klaus Werner

Primary proton-air interactions at ultra-high energies leave a physically interpretable imprint on the correlated fluctuations of the depth of shower maximum and the muon content in extensive air showers. This imprint reflects the…

High Energy Astrophysical Phenomena · Physics 2026-02-26 Lorenzo Cazon , Ruben Conceição , Miguel Alexandre Martins , Felix Riehn

Observations of cosmic rays have been improving at all energies, with higher statistics and reduced systematics. Fundamental questions remain regarding the origins of cosmic rays both within the Galaxy and in extragalactic sources, and new…

High Energy Astrophysical Phenomena · Physics 2010-10-20 Paul Sommers

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it…

High Energy Physics - Experiment · Physics 2016-11-01 The Pierre Auger Collaboration , A. Aab , P. Abreu , M. Aglietta , E. J. Ahn , I. Al Samarai , I. F. M. Albuquerque , I. Allekotte , J. Allen , P. Allison , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , M. Ambrosio , G. A. Anastasi , L. Anchordoqui , B. Andrada , S. Andringa , C. Aramo , F. Arqueros , N. Arsene , H. Asorey , P. Assis , J. Aublin , G. Avila , A. M. Badescu , C. Baus , J. J. Beatty , K. H. Becker , J. A. Bellido , C. Berat , M. E. Bertaina , X. Bertou , P. L. Biermann , P. Billoir , J. Biteau , S. G. Blaess , A. Blanco , J. Blazek , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , N. Borodai , A. M. Botti , J. Brack , I. Brancus , T. Bretz , A. Bridgeman , F. L. Briechle , P. Buchholz , A. Bueno , S. Buitink , M. Buscemi , K. S. Caballero-Mora , B. Caccianiga , L. Caccianiga , A. Cancio , F. Canfora , L. Caramete , R. Caruso , A. Castellina , G. Cataldi , L. Cazon , R. Cester , A. G. Chavez , A. Chiavassa , J. A. Chinellato , J. Chudoba , R. W. Clay , R. Colalillo , A. Coleman , L. Collica , M. R. Coluccia , R. Conceição , F. Contreras , M. J. Cooper , S. Coutu , C. E. Covault , J. Cronin , R. Dallier , S. D'Amico , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , R. M. de Almeida , S. J. de Jong , G. De Mauro , J. R. T. de Mello Neto , I. De Mitri , J. de Oliveira , V. de Souza , J. Debatin , L. del Peral , O. Deligny , N. Dhital , C. Di Giulio , A. Di Matteo , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , J. C. D'Olivo , A. Dorofeev , R. C. dos Anjos , M. T. Dova , A. Dundovic , J. Ebr , R. Engel , M. Erdmann , M. Erfani , C. O. Escobar , J. Espadanal , A. Etchegoyen , H. Falcke , K. Fang , G. Farrar , A. C. Fauth , N. Fazzini , A. P. Ferguson , B. Fick , J. M. Figueira , A. Filevich , A. Filipčič , O. Fratu , M. M. Freire , T. Fujii , A. Fuster , F. Gallo , B. García , D. Garcia-Pinto , F. Gate , H. Gemmeke , A. Gherghel-Lascu , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , D. Głas , C. Glaser , H. Glass , G. Golup , M. Gómez Berisso , P. F. Gómez Vitale , N. González , B. Gookin , J. Gordon , A. Gorgi , P. Gorham , P. Gouffon , N. Griffith , A. F. Grillo , T. D. Grubb , F. Guarino , G. P. Guedes , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , J. L. Harton , Q. Hasankiadeh , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , A. E. Herve , G. C. Hill , C. Hojvat , N. Hollon , E. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , T. Huege , J. Hulsman , A. Insolia , P. G. Isar , I. Jandt , S. Jansen , C. Jarne , J. A. Johnsen , M. Josebachuili , A. Kääpä , O. Kambeitz , K. H. Kampert , P. Kasper , I. Katkov , B. Keilhauer , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Krause , N. Krohm , D. Kuempel , G. Kukec Mezek , N. Kunka , A. Kuotb Awad , D. LaHurd , L. Latronico , M. Lauscher , P. Lautridou , P. Lebrun , R. Legumina , M. A. Leigui de Oliveira , A. Letessier-Selvon , I. Lhenry-Yvon , K. Link , L. Lopes , R. López , A. López Casado , A. Lucero , M. Malacari , M. Mallamaci , D. Mandat , P. Mantsch , A. G. Mariazzi , V. Marin , I. C. Mariş , G. Marsella , D. Martello , H. Martinez , O. Martínez Bravo , J. J. Masías Meza , H. J. Mathes , S. Mathys , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , E. Mayotte , P. O. Mazur , C. Medina , G. Medina-Tanco , V. B. B. Mello , D. Melo , A. Menshikov , S. Messina , M. I. Micheletti , L. Middendorf , I. A. Minaya , L. Miramonti , B. Mitrica , D. Mockler , L. Molina-Bueno , S. Mollerach , F. Montanet , C. Morello , M. Mostafá , C. A. Moura , G. Müller , M. A. Muller , S. Müller , I. Naranjo , S. Navas , P. Necesal , L. Nellen , A. Nelles , J. Neuser , P. H. Nguyen , M. Niculescu-Oglinzanu , M. Niechciol , L. Niemietz , T. Niggemann , D. Nitz , D. Nosek , V. Novotny , H. Nožka , L. A. Núñez , L. Ochilo , F. Oikonomou , A. Olinto , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , P. Papenbreer , G. Parente , A. Parra , T. Paul , M. Pech , F. Pedreira , J. Pękala , R. Pelayo , J. Peña-Rodriguez , I. M. Pepe , L. A. S. Pereira , L. Perrone , E. Petermann , C. Peters , S. Petrera , J. Phuntsok , R. Piegaia , T. Pierog , P. Pieroni , M. Pimenta , V. Pirronello , M. Platino , M. Plum , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , E. J. Quel , S. Querchfeld , S. Quinn , J. Rautenberg , O. Ravel , D. Ravignani , B. Revenu , J. Ridky , M. Risse , P. Ristori , V. Rizi , W. Rodrigues de Carvalho , J. Rodriguez Rojo , M. D. Rodríguez-Frías , D. Rogozin , J. Rosado , M. Roth , E. Roulet , A. C. Rovero , S. J. Saffi , A. Saftoiu , H. Salazar , A. Saleh , F. Salesa Greus , G. Salina , J. D. Sanabria Gomez , F. Sánchez , P. Sanchez-Lucas , E. M. Santos , E. Santos , F. Sarazin , B. Sarkar , R. Sarmento , C. Sarmiento-Cano , R. Sato , C. Scarso , M. Schauer , V. Scherini , H. Schieler , D. Schmidt , O. Scholten , H. Schoorlemmer , P. Schovánek , F. G. Schröder , A. Schulz , J. Schulz , J. Schumacher , S. J. Sciutto , A. Segreto , M. Settimo , A. Shadkam , R. C. Shellard , G. Sigl , O. Sima , A. Śmiałkowski , R. Šmída , G. R. Snow , P. Sommers , S. Sonntag , J. Sorokin , R. Squartini , D. Stanca , S. Stanič , J. Stapleton , J. Stasielak , F. Strafella , A. Stutz , F. Suarez , M. Suarez Durán , T. Sudholz , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , O. A. Taborda , A. Tapia , A. Tepe , V. M. Theodoro , C. Timmermans , C. J. Todero Peixoto , L. Tomankova , B. Tomé , A. Tonachini , G. Torralba Elipe , D. Torres Machado , P. Travnicek , M. Trini , R. Ulrich , M. Unger , M. Urban , A. Valbuena-Delgado , J. F. Valdés Galicia , I. Valiño , L. Valore , G. van Aar , P. van Bodegom , A. M. van den Berg , A. van Vliet , E. Varela , B. Vargas Cárdenas , G. Varner , J. R. Vázquez , R. A. Vázquez , D. Veberič , V. Verzi , J. Vicha , M. Videla , L. Villaseñor , S. Vorobiov , H. Wahlberg , O. Wainberg , D. Walz , A. A. Watson , M. Weber , A. Weindl , L. Wiencke , H. Wilczyński , T. Winchen , D. Wittkowski , B. Wundheiler , S. Wykes , L. Yang , T. Yapici , D. Yelos , E. Zas , D. Zavrtanik , M. Zavrtanik , A. Zepeda , B. Zimmermann , M. Ziolkowski , Z. Zong , F. Zuccarello

Very high energy cosmic rays are typically studied by measuring extensive air showers formed by secondary particles produced in collisions with air nuclei. The indirect character of the measurement makes the physics interpretation of cosmic…

High Energy Physics - Phenomenology · Physics 2014-11-17 Ralph Engel

High-energy collisions at the High-Luminosity Large Hadron Collider (HL-LHC) will produce an enormous flux of particles along the beam collision axis that is not accessible by existing LHC experiments. Multi-particle production in the…

High Energy Physics - Experiment · Physics 2023-08-22 Dennis Soldin

We explore particle physics beyond accelerator energies, motivated by questions exposed in astroparticle physics observations: 1) Are there reasonable modifications to the standard extrapolations of LHC-tuned hadronic interaction models, so…

High Energy Physics - Phenomenology · Physics 2019-03-01 Glennys R. Farrar

Extensive air showers are generated through interactions of high-energy cosmic rays impinging the Earth's atmosphere. A new method is described to infer the attenuation of hadrons in air showers. The numbers of electrons and muons,…

High Energy Astrophysical Phenomena · Physics 2009-08-11 W. D. Apel

The interpretation of extensive air shower (EAS) measurements is strongly dependent on the hadronic interaction models used for simulating reference showers. We study the importance of low-energy hadronic interactions in simulated air…

Astrophysics · Physics 2008-11-26 Christine Meurer , J. Bluemer , R. Engel , A. Haungs , M. Roth , the HARP collaboration

The LHCf experiment is dedicated to the measurement of very forward particle production in the high energy hadron-hadron collisions at LHC, with the aim of improving the cosmic-ray air shower developments models. The detector has taken data…

High Energy Physics - Experiment · Physics 2013-10-15 O. Adriani

The properties of cosmic rays with energies above 10**6 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review we summarize the phenomenology of these giant air…

High Energy Physics - Phenomenology · Physics 2010-01-15 Luis Anchordoqui , Maria Teresa Dova , Analisa Mariazzi , Thomas McCauley , Thomas Paul , Stephen Reucroft , John Swain

Hard probes are a cornerstone in the ongoing program to determine the properties of hot and dense QCD matter as created in ultrarelativistic heavy ion collisions. LHC measurements have so far resulted in a wealth of high P_T data, opening…

High Energy Physics - Phenomenology · Physics 2015-06-11 Thorsten Renk

At high energy, cosmic rays can only be studied by measuring the extensive air showers they produce in the atmosphere of the Earth. Although the main features of air showers can be understood within a simple model of successive…

Astrophysics · Physics 2015-06-24 T. Pierog , R. Engel , D. Heck
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