Aspen, April 19, 2007Tom Gaisser1 10 17 eV decade Breakout summary.

Slides:



Advertisements
Similar presentations
Alessia Tricomi University and INFN Catania on behalf of the LHCf Collaboration The LHCf experiment at LHC ISVHECRI08 - XV International Symposium on Very.
Advertisements

AGASA Results Max-Planck-Institut für Physik, München, Germany Masahiro Teshima for AGASA collaboration at 3 rd Int. Workshop on UHECR, Univ. Leeds.
A.A. Ivanov for the Yakutsk array group The scientific goals of the Yakutsk array under modernization.
Towards the trans-GZK area ray (from AGASA, AUGER, HIRES TO JEM -EUSO) J. N. Capdevielle, APC, University Paris Diderot
Application for Pierre Auger Observatory.
Results from the Telescope Array experiment H. Tokuno Tokyo Tech The Telescope Array Collaboration 1.
GZK Horizons and the Recent Pierre Auger Result on the Anisotropy of Highest-energy Cosmic Ray Sources Chia-Chun Lu Institute of Physics, National Chiao-Tung.
XXI st European Cosmic Ray Symposium Kosice 2008 ^ Tadeusz Wibig University of Łódź A. Sołtan Institute for Nuclear Studies Heavy Cosmic Ray Nuclei from.
IAS, Princeton September 16, 2003 Thomas K. Gaisser Anatomy of the Cosmic-ray Energy Spectrum from the knee to the ankle.
The Pierre Auger Observatory Nicolás G. Busca Fermilab-University of Chicago FNAL User’s Meeting, May 2006.
AGASA update M. Teshima ICRR, U of CfCP mini workshop Oct
The Telescope Array Low Energy Extension (TALE)‏ Pierre Sokolsky University of Utah.
Tom Gaisser, Leeds, July 23, 2004 in honor of Alan Watson The next 10 years in Particle Astrophysics Workshop summary Some personal observations Tribute.
AGASA Masahiro Teshima Max-Planck-Institut für Physik, München, Germany for AGASA collaboration.
Aspen, April 16, 2007Tom Gaisser1 What’s new and what questions remain since our previous meeting? Workshop on Physics at the End of the Galactic Cosmic-ray.
TAUP 2005: Zaragoza Observations of Ultra-high Energy Cosmic Rays Alan Watson University of Leeds Spokesperson for Pierre Auger Observatory
Ultra high energy cosmic rays: highlights of recent results J. Matthews Pierre Auger Observatory Louisiana State University 19 August August.
Aspen, April 26, 2005 Tom Gaisser The cosmic-ray spectrum From the knee to the ankle.
1 Roma Meeting: June 2007 Recent results from the Pierre Auger Observatory (and comparisons with AGASA and HiRes) Alan Watson University of Leeds
Welcome to Aspen Agenda Logistics Working groups Publication of proceeding.
Accelerators in the KEK, Tsukuba Mar. 14, Towards unravelling the structural distribution of ultra-high-energy cosmic ray sources Hajime.
Status of Cosmic Rays Physics at the Knee Andrea Chiavassa Università and INFN Torino NOW 2006 Otranto 9-16 September 2006.
Konstantin Belov. GZK-40, Moscow. Konstantin Belov High Resolution Fly’s Eye (HiRes) Collaboration GZK-40. INR, Moscow. May 17, measurements by fluorescence.
Summary Where we are. Physics questions to be answered. Why Auger is a good investment for Fermilab and the US. Fermilab Auger Group proposal.
The 23-European Symposium and the 32 Russian cosmic ray conference 3-7 July Moscow 1 Possible composition of the primary particles at ultrahigh energies.
Auger at eV Bruce Dawson University of Adelaide, Australia.
LBL November 3, 2003 selection & comments 14 June 2004 Thomas K. Gaisser Anatomy of the Cosmic-ray Energy Spectrum from the knee to the ankle.
Mar 9, 2005 GZK Neutrinos Theory and Observation D. Seckel, Univ. of Delaware.
Telescope Array Experiment: Status and Prospects Pierre Sokolsky University of Utah.
Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration, CTEQ- Fermilab School Lima, Peru, August 2012 Ultrahigh Cosmic Rays: The highest energy.
Status and first results of the KASCADE-Grande experiment
A.Z. Gazizov LNGS, Italy Based on works with V. Berezinsky and R. Aloisio Quarks-08.
Fitting the HiRes Data Douglas Bergman Rutgers University 28 April 2005.
April 23, 2009PS638 Tom Gaisser 1 Neutrinos from AGN & GRB Expectations for a km 3 detector.
Energy Spectrum C. O. Escobar Pierre Auger Director’s Review December /15/2011Fermilab Director's Review1.
1 NATURE OF KNEES AND ANKLE V.S. Berezinsky INFN, Laboratori Nazionali del Gran Sasso.
AGASA Results Masahiro Teshima for AGASA collaboration
KEK, Feb 27, 2006Tom Gaisser1 Cosmic-ray physics with IceCube IceTop the surface component of IceCube.
Low-Energy Interaction Models in CORSIKA Dieter Heck, Ralph Engel Forschungszentrum Karlsruhe, Germany Giuseppe Battistoni, Alberto Fassò, Alfredo Ferrari,
The muon component in extensive air showers and its relation to hadronic multiparticle production Christine Meurer Johannes Blümer Ralph Engel Andreas.
Laboratory Particle- Astrophysics P. Sokolsky High Energy Astrophysics Institute, Univ. of Utah.
Newly Born Pulsars as Sources of High and Ultrahigh Energy Cosmic Rays Ke Fang University of Chicago ISCRA - Jul 9, KF, Kotera, Olinto 2012, ApJ,
Future Plans and Summary Gordon Thomson Rutgers University.
“The Cosmic Ray composition in the knee region and the hadronic interaction models” G. Navarra INFN and University, Torino, Italy For the EAS-TOP Collaboration.
QCD at Cosmic Energies Erice, Aug 30, 2004 Thomas K. Gaisser Hadronic interactions in modeling atmospheric cascades The atmospheric cascade equation Heavy.
June 1, 2005Tom Gaisser CORSIKA summer school Cosmic-ray cascades in the atmosphere 1)Air shower phenomenology 2)Inclusive fluxes in the atmosphere.
School of Cosmic-ray Astrophysics, Erice, July 4, 2004 Thomas K. Gaisser Role of particle interactions in high-energy astrophysics Uncorrelated fluxes.
Heraeus Feb Tom Gaisser1 Particle Astrophysics Some questions to consider during this meeting.
Propagation and Composition of Ultra High Energy Cosmic Rays
Cosmic Rays from to eV. Open Problem and Experimental Results. (KASCADE-Grande view) Very High Energy Phenomena in the Universe XLIV th Rencontres.
Current Physics Results Gordon Thomson Rutgers University.
Juan Carlos Arteaga-Velázquez for the KASCADE-Grande Collaboration Institute of Physics and Mathematics Universidad Michoacana, Mexico 132nd ICRCJ.C.Arteaga.
South Pole Astro April 4, 2011 Tom Gaisser1 125 m Cosmic-ray physics with IceCube IceTop is the surface component of IceCube as a three-dimensional cosmic-ray.
Astrophysics of the Highest Energy Cosmic Rays Paul Sommers Cracow, Poland January 10, 2004.
NEVOD-DECOR experiment: results and future A.A.Petrukhin for Russian-Italian Collaboration Contents MSU, May 16, New method of EAS investigations.
On the Prospect of Tau Neutrino Astronomy in GeV Energies and Beyond G.-L. Lin National Chiao-Tung U. Taiwan Moriond 2005.
High Energy Cosmic Rays The Primary Particle Types Paul Sommers for Alan Watson Epiphany Conference, Cracow January 10, 2004.
Jim Matthews Louisiana State University Results from the Pierre Auger Observatory ECRS, Moscow, 4 July
Ultra High Energy Cosmic Rays: The disappointing model Askhat Gazizov LNGS, INFN, Italy in collaboration with Roberto Aloisio and Veniamin Berezinsky April.
Andrea Chiavassa Universita` degli Studi di Torino
IceCube: Neutrino telescope & cosmic-ray detector
Signatures of Protons in UHECR Transition from Galactic to
Frank Deppisch, Ralph Engel, Paolo Lipari, James Pinfold
observations of the muon bundles with IceCube
Latest Results from the KASCADE-Grande experiment
Search Sources of Ultrahigh Energy Particles in our Galaxy. V. A
Composition of Cosmic Rays at Ultra High Energies
The Aperture and Precision of the Auger Observatory
Studies and results at Pierre Auger Observatory
Presentation transcript:

Aspen, April 19, 2007Tom Gaisser eV decade Breakout summary

Allard, Olinto, Parizot, astro-ph/ Alternatives for transition to E.G.

Aspen, April 19, 2007Tom Gaisser3 Model dependence of composition in galactic-extragalactic transition Allard, Olinto, Parizot, astro-ph/ proton model mixed model Model extragalactic component Subtract from observed to get galactic component

Aspen, April 19, 2007Tom Gaisser4 Berezhko & Völk arXiv: v1 [astro-ph] Model galactic component Subtract from observed to get extragalactic Transition predicted: to eV

Aspen, April 19, 2007Tom Gaisser5 Depth of Maximum Early transition favored –HiRes prototype + CASA/MIA –HiRes (E > ) G. Archbold, P. Sokolsky, et al., Proc. 28 th ICRC, Tsukuba, 2003 HiRes new composition result: transition occurs before ankle 0.3 EeV

Aspen, April 19, 2007Tom Gaisser6 Composition from density of muons ρ µ (600) vs. E 0 (Akeno, AGASA) From heavy toward protons Calculations by Bruce Dawson with MoccaSibyll

Aspen, April 19, 2007Tom Gaisser7 KASCADE-Grande : first analyses muon density investigations KASCADE-Grande preliminary T. Pierog (EPOS) MIA

Cross section summary M Block Note: old data are rescaled

Aspen, April 19, 2007Tom Gaisser9 Interaction models QGSjet01 SIBYLL QGSjet02 EPOS Ralph Engel

Aspen, April 19, 2007Tom Gaisser10

Hard  0 production of EPOS readily detectable in LHCf

More  in EAS with EPOS Attribute to NN production in EPOS

Aspen, April 19, 2007Tom Gaisser13 Xmax more stable

Aspen, April 19, 2007Tom Gaisser14 Summary comments Two very different models of transition –10 17 to or to eV –Strong composition change signature –HiRes favors low-energy transition Model dependence a problem Good energy resolution important KASCADE-Grande, IceCube/IceTop, TALE, Amiga/HEAT at Auger

Feedback: Privacy Policy Feedback
Do Not Sell My Personal Information
About project: SlidePlayer Terms of Service

© 2025 SlidePlayer.com. Inc. All rights reserved.