Results from NA61/SHINE

2013/01/01 by M. Unger · 19 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #COSMIC cancer database #Cosmic ray #Heavy ion #Interpretation (philosophy) #Ion #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Philosophy #Physics #astro-ph.HE #nucl-ex

paper · pdf · doi:10.1051/epjconf/20125201009

published in EPJ Web of Conferences 52, 01009 (EDP Sciences) · 7 pages, Talk given at the International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2012), Berlin, Germany, to appear in EPJ web of Conf

openalex publication_date 2013/01/01 · arxiv created 2013/05/22 · arxiv updated 2019/08/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

In this paper we summarize recent results from NA61/SHINE relevant for heavy ion physics, neutrino oscillations and the interpretation of air showers induced by ultra-high energy cosmic rays.

Citations

• Hadron Production at Fixed Target Energies and Extensive Air Showers
• How to Improve UrQMD Model to Describe NA61/SHINE Experimental Data
• Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam
• Microscopic models for ultrarelativistic heavy ion collisions
• QGSJET-II: towards reliable description of very high energy hadronic interactions