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We discuss the necessary steps for implementing an angularly ordered (AO) electroweak (EW) parton shower in Herwig 7 multi-purpose event generator. This includes calculating the helicity-dependent quasi-collinear EW branching functions that…

High Energy Physics - Phenomenology · Physics 2022-04-26 M. R. Masouminia , P. Richardson

The hybrid design of the Pierre Auger Observatory allows for the measurement of a number of properties of extensive air showers initiated by ultra-high energy cosmic rays. By comparing these measurements to predictions from air shower…

High Energy Astrophysical Phenomena · Physics 2019-05-22 R. R. Prado

The development of extensive air showers at extreme energies is studied using a simulation model much simpler and cruder, but also more transparent and flexible, than existing sophisticated codes. Evidence for its satisfactory performance…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Do Thi Hoai , Pham Ngoc Diep , Pierre Darriulat , Pham Tuan Anh , Pham Ngoc Dong , Nguyen Van Hiep , Pham Thi Tuyet Nhung , Nguyen Thi Thao

{Measurements of cosmic-ray composition based on air-shower measurements rely mostly on the determination of the position of the shower maximum ($X_\mathrm{max}$). One efficient technique is to image the development of the air shower using…

High Energy Astrophysical Phenomena · Physics 2025-06-03 V. B. Jhansi , S. Thoudam , S. Buitink , A. Corstranje , M. Desmet , J. R. Horandel , T. Heuge , K. Mulrey , O. Scholten

Short radio pulses can be measured from showers of both high-energy cosmic rays and neutrinos. While commonly several antenna stations are needed to reconstruct the energy of an air shower, we describe a novel method that relies on the…

Instrumentation and Methods for Astrophysics · Physics 2019-11-26 Christoph Welling , Christian Glaser , Anna Nelles

We present a new method for probing the hadronic interaction models at ultra-high 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…

High Energy Astrophysical Phenomena · Physics 2017-10-20 The Pierre Auger Collaboration , A. Aab , P. Abreu , M. Aglietta , I. Al Samarai , I. F. M. Albuquerque , I. Allekotte , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , 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 , A. Balaceanu , F. Barbato , R. J. Barreira Luz , J. J. Beatty , K. H. Becker , J. A. Bellido , C. Berat , M. E. Bertaina , X. Bertou , P. L. Biermann , J. Biteau , S. G. Blaess , A. Blanco , J. Blazek , C. Bleve , 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 , L. Caccianiga , A. Cancio , F. Canfora , L. Caramete , R. Caruso , A. Castellina , F. Catalani , G. Cataldi , L. Cazon , A. G. Chavez , J. A. Chinellato , J. Chudoba , R. W. Clay , A. Cobos , R. Colalillo , A. Coleman , L. Collica , M. R. Coluccia , R. Conceição , G. Consolati , F. Contreras , M. J. Cooper , S. Coutu , C. E. Covault , J. Cronin , 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 , O. Deligny , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , J. C. D'Olivo , Q. Dorosti , 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 , J. Farmer , G. Farrar , A. C. Fauth , N. Fazzini , F. Fenu , B. Fick , J. M. Figueira , A. Filipčič , O. Fratu , M. M. Freire , T. Fujii , A. Fuster , R. Gaior , B. García , D. Garcia-Pinto , F. Gaté , H. Gemmeke , A. Gherghel-Lascu , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , D. Głas , C. Glaser , G. Golup , M. Gómez Berisso , P. F. Gómez Vitale , N. González , A. Gorgi , P. Gorham , A. F. Grillo , T. D. Grubb , F. Guarino , G. P. Guedes , R. Halliday , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , J. L. Harton , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , A. E. Herve , G. C. Hill , C. Hojvat , E. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , T. Huege , J. Hulsman , A. Insolia , P. G. Isar , I. Jandt , J. A. Johnsen , M. Josebachuili , J. Jurysek , A. Kääpä , O. Kambeitz , K. H. Kampert , B. Keilhauer , N. Kemmerich , E. Kemp , J. 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 , B. L. Lago , D. LaHurd , R. G. Lang , M. Lauscher , R. Legumina , M. A. Leigui de Oliveira , A. Letessier-Selvon , I. Lhenry-Yvon , K. Link , D. Lo Presti , L. Lopes , R. López , A. López Casado , R. Lorek , Q. Luce , A. Lucero , M. Malacari , M. Mallamaci , D. Mandat , P. Mantsch , A. G. Mariazzi , 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 , E. Mayotte , P. O. Mazur , C. Medina , G. Medina-Tanco , D. Melo , A. Menshikov , K. -D. Merenda , S. Michal , M. I. Micheletti , L. Middendorf , L. Miramonti , B. Mitrica , D. Mockler , S. Mollerach , F. Montanet , C. Morello , M. Mostafá , A. L. Müller , G. Müller , M. A. Muller , S. Müller , R. Mussa , I. Naranjo , L. Nellen , P. H. Nguyen , M. Niculescu-Oglinzanu , M. Niechciol , L. Niemietz , T. Niggemann , D. Nitz , D. Nosek , V. Novotny , L. Nožka , L. A. Núñez , L. Ochilo , F. Oikonomou , A. Olinto , M. Palatka , J. Pallotta , P. Papenbreer , G. Parente , A. Parra , T. Paul , M. Pech , F. Pedreira , J. Pękala , R. Pelayo , J. Peña-Rodriguez , L. A. S. Pereira , M. Perlin , L. Perrone , C. Peters , S. Petrera , J. Phuntsok , R. Piegaia , T. Pierog , M. Pimenta , V. Pirronello , M. Platino , M. Plum , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , E. J. Quel , S. Querchfeld , S. Quinn , R. Ramos-Pollan , J. Rautenberg , D. Ravignani , J. Ridky , F. Riehn , M. Risse , P. Ristori , V. Rizi , W. Rodrigues de Carvalho , G. Rodriguez Fernandez , J. Rodriguez Rojo , D. Rogozin , M. J. Roncoroni , M. Roth , E. Roulet , A. C. Rovero , P. Ruehl , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , A. Saleh , F. Salesa Greus , G. Salina , F. Sánchez , P. Sanchez-Lucas , E. M. Santos , E. Santos , F. Sarazin , R. Sarmento , C. Sarmiento-Cano , R. Sato , M. Schauer , V. Scherini , H. Schieler , M. Schimp , D. Schmidt , O. Scholten , P. Schovánek , F. G. Schröder , S. Schröder , A. Schulz , J. Schumacher , S. J. Sciutto , A. Segreto , A. Shadkam , R. C. Shellard , G. Sigl , G. Silli , O. Sima , A. Śmiałkowski , R. Šmída , G. R. Snow , P. Sommers , S. Sonntag , R. Squartini , D. Stanca , S. Stanič , J. Stasielak , P. Stassi , M. Stolpovskiy , F. Strafella , A. Streich , F. Suarez , M. Suarez Durán , T. Sudholz , T. Suomijärvi , A. D. Supanitsky , J. Šupík , J. Swain , Z. Szadkowski , A. Taboada , O. A. Taborda , V. M. Theodoro , C. Timmermans , C. J. Todero Peixoto , L. Tomankova , B. Tomé , G. Torralba Elipe , P. Travnicek , M. Trini , R. Ulrich , M. Unger , M. Urban , 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 , R. A. Vázquez , D. Veberič , C. Ventura , I. D. Vergara Quispe , V. Verzi , J. Vicha , L. Villaseñor , S. Vorobiov , H. Wahlberg , O. Wainberg , D. Walz , A. A. Watson , M. Weber , A. Weindl , L. Wiencke , H. Wilczyński , M. Wirtz , D. Wittkowski , B. Wundheiler , L. Yang , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , A. Zepeda , B. Zimmermann , M. Ziolkowski , Z. Zong , F. Zuccarello

In this publication the implementation of a new parton shower model based on the Catani-Seymour dipole factorisation, as first suggested by Z. Nagy and D. E. Soper, is discussed. First results obtained with the new algorithm are compared…

High Energy Physics - Phenomenology · Physics 2008-11-26 Steffen Schumann , Frank Krauss

At Auger energies only model predictions enable us to extract primary cosmic ray features. The simulation of the shower evolution depends sensitively on the first few interactions, necessarily related to the quality of our understanding of…

High Energy Physics - Phenomenology · Physics 2010-01-15 Luis Anchordoqui , Haim Goldberg , Jared MacLeod , Tom McCauley , Tom Paul , Steve Reucroft , John Swain

The experiment KASCADE observes simultaneously the electron-photon, muon, and hadron components of high-energy extensive air showers (EAS). The analysis of EAS observables for an estimate of energy and mass of the primary particle invokes…

Astrophysics · Physics 2009-09-25 T. Antoni

This review provides an introduction to the radio emission by particle cascades, an overview on the various experiments, and explains methods for the radio measurement of air-shower properties. Furthermore, potential applications of the…

Instrumentation and Methods for Astrophysics · Physics 2017-01-04 Frank G. Schröder

The radio detection of very inclined air showers offers a promising avenue for studying ultra-high-energy cosmic rays (UHECRs) and neutrinos. Accurate reconstruction methods are essential for investigating the properties of primary…

Instrumentation and Methods for Astrophysics · Physics 2025-07-24 Kewen Zhang , Duan Kaikai , Ramesh Koirala , Matías Tueros , Chao Zhang , Yi Zhang

The reconstruction of very inclined air showers is a new challenge for next-generation radio experiments such as the AugerPrime radio upgrade, BEACON, and GRAND, which focus on the detection of ultra-high-energy particles. To tackle this,…

High Energy Astrophysical Phenomena · Physics 2024-08-01 Marion Guelfand , Simon Chiche , Kumiko Kotera , Simon Prunet , Tanguy Pierog

Ultra-high energy cosmic rays impinge on the atmosphere and induce air shower cascades, in which huge numbers of particles are produced. By travelling through the Earth's atmosphere and magnetic field, these particles create a noticeable…

High Energy Physics - Experiment · Physics 2026-04-01 Beatriz de Errico , Charles Timmermans

In hadron induced air showers of highest energies (E> 1e18 eV), the lateral distribution functions of electrons and muons are a superposition of many separate electromagnetic sub-showers, initiated by meson decay at different altitudes and…

High Energy Physics - Phenomenology · Physics 2011-05-23 Hans-Joachim Drescher , Glennys R. Farrar

Dynamic metasurface antennas (DMAs) are a promising hybrid analog/digital beamforming technology to realize next-generation wireless systems with low cost, footprint, and power consumption. The research on DMA-empowered wireless systems is…

Signal Processing · Electrical Eng. & Systems 2025-06-12 François Yven , Jean Tapie , Jérôme Sol , Philipp del Hougne

Correctly identifying the nature and properties of outgoing particles from high energy collisions at the Large Hadron Collider is a crucial task for all aspects of data analysis. Classical calorimeter-based classification techniques rely on…

High Energy Physics - Experiment · Physics 2021-04-06 Luke de Oliveira , Benjamin Nachman , Michela Paganini

Detection of extensive air showers with radio antennas is an appealing technique in cosmic ray physics. However, because of the high level of measurement noise, current reconstruction methods still leave room for improvement. Furthermore,…

Instrumentation and Methods for Astrophysics · Physics 2025-07-16 Simon Strähnz , Tim Huege , Torsten Enßlin , Karen Terveer , Anna Nelles

The hadronic light-by-light contribution to the anomalous magnetic moment of the muon was recently analyzed in the framework of dispersion theory, providing a systematic formalism where all input quantities are expressed in terms of…

High Energy Physics - Phenomenology · Physics 2015-06-22 Gilberto Colangelo , Martin Hoferichter , Bastian Kubis , Massimiliano Procura , Peter Stoffer

We discuss the relation between remnant fragmentation in inelastic high-energy hadronic interactions and muon production in extensive cosmic ray air showers. Using a newly developed tool, a simple and flexible hadronic event generator, we…

High Energy Physics - Phenomenology · Physics 2008-11-26 H. J. Drescher

The merging of matrix elements and parton showers is an established calculational tool for the description of multi-jet final states at hadron colliders. These methods have recently been promoted to next-to-leading order accuracy in the…

High Energy Physics - Phenomenology · Physics 2013-11-15 Marek Schonherr , Stefan Hoeche , Frank Krauss , Frank Siegert
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