Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/102851
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Type: Journal article
Title: Testing hadronic interactions at ultrahigh energies with air showers measured by the Pierre Auger Observatory
Author: Aab, A.
Abreu, P.
Aglietta, M.
Ahn, E.J.
Al Samarai, I.
Albuquerque, I.F.M.
Allekotte, I.
Allen, J.D.
Allison, P.
Almela, A.
Alvarez Castillo, J.
Alvarez-Muñiz, J.
Ambrosio, M.
Anastasi, G.A.
Anchordoqui, L.
Andrada, B.
Andringa, S.
Aramo, C.
Arqueros, F.
Arsene, N.
et al.
Citation: Physical Review Letters, 2016; 117(19):192001-1-192001-9
Publisher: American Physical Society
Issue Date: 2016
ISSN: 0031-9007
1079-7114
Statement of
Responsibility: 
A. Aab ... J. A. Bellido ... S. G. Blaess ... R.W. Clay ... M. J. Cooper ... B. R. Dawson ... T. D. Grubb ... T. A. Harrison ... G. C. Hill ... M. Malacari ... P. H. Nguyen ... S. J. Saffi ... J. Sorokin ... T. Sudholz ... P. van Bodegom ... et al. (Pierre Auger Collaboration)
Abstract: 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 to events with primary energy 6-16 EeV (E_{CM}=110-170  TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.
Keywords: Pierre Auger Collaboration
Description: Published 31 October 2016
Rights: © 2016 American Physical Society
DOI: 10.1103/PhysRevLett.117.192001
Grant ID: ARC
Published version: http://dx.doi.org/10.1103/physrevlett.117.192001
Appears in Collections:Aurora harvest 3
IPAS publications

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