Conveners
Theory and measurement of UHECR flux and composition
- James Matthews (Louisiana State University)
Theory and measurement of UHECR flux and composition
- Peter Grieder (University of Bern)
Description
Contributed talks 6 x 15+5 min
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Jonathan R. Ellis (CERN)14/02/2012, 14:00
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Prof. Yoshitaka Itow (Nagoya University)14/02/2012, 14:40
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Gaku Mitsuka (Nagoya University (JP))14/02/2012, 15:20talkThe Large Hadron Collider forward experiment measured very forward neutral particle spectra in LHC proton-proton collisions in early 2010. In this talk we will discuss the energy and transverse momentum spectra of neutral pion at the 7TeV proton-proton collision, and also present the inclusive photon energy spectra taken at the 900GeV collisions. The spectra in both collision energy are...Go to contribution page
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Prof. Paolo Lipari (Universita di Roma I)14/02/2012, 15:40talkThis contribution discusses possible methods to measure the proton-proton total cross section from observations of Ultra High Energy cosmic rays, and the theoretical uncertainties associated with these methods.Go to contribution page
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Dr Ralf Matthias Ulrich (KIT - Karlsruhe Institute of Technology (DE))14/02/2012, 16:30talkAuthorship: The Pierre Auger Collaboration. Using the tail of the distribution of the depth of shower maxima observed with the Pierre Auger Observatory, we derive an estimate of the proton-air cross section for particle production at center-of-mass energies of 57 TeV. Air showers observed with the fluorescence detector and at least one station of the surface array are analyzed in the...Go to contribution page
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Alexey Yushkov14/02/2012, 16:50talkVarious methods of estimation of the muonic part of the signal observed in the surface Cherenkov detectors have been developed within the Pierre Auger Collaboration in the recent years. Muon shower content, derived from data with these methods, is larger in comparison with predictions of QGJSET II and EPOS 1.99 interaction models. The zenith angle dependence of the muon deficit in simulations...Go to contribution page
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Prof. Glennys Farrar (New York University)14/02/2012, 17:10talkUltrahigh energy cosmic rays (UHECRs) are the highest energy particles in the Universe, recorded to have energies up to 100 million times greater than the LHC beams. Whether they are protons or nuclei and how they are accelerated are presently unknown. The particle cascades created when these UHECRs interact in the atmosphere are not well-described by simulations, but since the primary...Go to contribution page
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Prof. Anatoly Petrukhin (MEPhI)14/02/2012, 17:30talkNew technique of EAS investigations by means of the method of local muon density spectra (LMDS) is developed. Application of this method to investigations of inclined EAS allows exploration of CR energy interval from 10^15 to 10^19 eV by means of a relatively small detector with area ~100 m^2 due to very strong dependence of EAS muon density on zenith angle. During 2002-2007, long-term...Go to contribution page
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Dr Ralph Engel (Forschungszentrum Karlsruhe)14/02/2012, 17:50