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1018eV Neutrinos associated with. UHECR ( 1019eV) sources. Zhuo Li (??) ... Neutrino energy. en2n(en) For 10PeV protons, the fraction of total energy loss ...
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... eye give angular resolution comparable to 'stereo' reconstruction ... Note the significant aperture at 1018eV, and the stereo aperture at the higher energies ...
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Neutrinos @ HiRes HR2 HR1 Kai Martens High Energy Astrophysics Institute Department of Physics, University of Utah
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The Second International Workshop on Ultra-high-energy cosmic rays and ... Cosmology, Particle Physics. A new actor on the scene of CR from space? neutrino ...
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To catch the sign of proton acceleration. GLAST will be Launched May in this year. ... Proton acceleration efficiency. We need 6-8 1043 ergs/Mpc3/yr to explain UHECRs ...
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anisotropy expectations. for different AGN types. Takami, SI , in prep. ... characteristic spectra, anisotropy, composition. hard X-rays TeV gamma-rays. AGNs ...
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Not via multi-step accelerations, (in situ, Fermi 1, 2 , shock ... Rather by single-step sweeping via corotating magnetic fields, ... Post-cursors (offset by ...
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FE II had only partial azimuth coverage. HiRes prototype/MIA ... FOV 3-17 in elevation, 322 in azimuth. HiRes 2 has 42 operational mirrors in two rings. ...
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out of Galaxy (but: hint of index ... Colliding Galaxies. Rapidly spinning giant black holes. Highly magnetized, ... from nearby galaxies would appear ...
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The Galactic Center is one of the most interesting galactic target ... 3rd method - Exposure-based study. Residual modulation. 1 E 3 EeV ...
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The Status of the Pierre Auger Observatory. Bruce Dawson ... Millard county. Utah, USA. Southern hemisphere: Malarg e. Provincia de Mendoza. Argentina ...
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Stereo detection over the ankle region provides better resolution than monocular ... The tower can operate in monocular mode, but limited to Xmax resolution of ~50 g ...
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Ultra High Energy Neutrino Astronomy
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Title: Slide 1 Author: pinfold Last modified by: Richard Soluk Created Date: 6/6/2003 9:51:51 PM Document presentation format: On-screen Show Company
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The Highest Energy Particles
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Modeling the Radiation from the Supernova Remnant of SN1006
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For Sources with tgp 1: Strongest know z evolution (QSO, SFR) ... tgp for known sources. ep. e'g. n. p e e- eg. Antares (0.1 Gton) Nemo (1 Gton) Anita ...
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... P ' ' n*x KQn ' ?M LF M PNG ...
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Louisiana State University, Baton Rouge, LA, USA ... 1051 ergs in the blast wave. SN rate 2/century 2X1049ergs/yr. Blast wave must convert ~1% of its energy into ...
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Cosmic Rays are subatomic particles and radiation of extra-terrestrial origin. First discovered in 1912 by German scientist Victor Hess, measuring radiation ...
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cs/Lc = characteristic signal frequency. E = shower energy. 07.10.2004 ... (literature value: (1450 10)m/s). Confirms precision of time and position measurements. ...
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Measured shower parameters. J.N. Matthews XXth ECRS Lisboa. Sept 2006 ... Analyze 'golden events' above 8 EeV to increase statistical reach ' ...
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[Taylor et al. 04] Dynamics 101b. 2qj. G(R) 1/qj. Rj 'Ignorant' jet/observer ... SWIFT Afterglows. II. Challenges. Collisionless shock physics (ee, eB ...
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Experimental cosmic ray physics in the 1017 1019 eV region
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New Cosmic Rays at the Highest Energies
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t lescope les 4 actuels en st r oscopie. 20 GeV esp r s en ' mono ' avec le tr s grand ... Sensibilit s des t lescopes d'imagerie actuels. Ecole de Gif 2006 ...
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... of supermassive relic of Big Bang 1024 eV = 1015 GeV ... Bulge. Halo. Ring bar. Galactic center. Sun. 1 pc = 3.3 ly. Theorical hypothesis. Propagation ...
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VHE PARTICLE ASTROPHYSICS Science, Projects, Roadmap,
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Actuellement, avec les ? d' nergie 100 GeV, on atteint une r solution de 4 6 minutes d'arc ( comparer quelques secondes d'arc en astronomie X) ...
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Detector response(box, housing) 5% Energy Estimator S(600) ... AGASA fast simulation (based on empirical formula and toy simulation) Based on CORSIKA M.C. ...
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