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Mott-Berezinsky formula, instantons, and integrability Ilya A. Gruzberg In collaboration with Adam Nahum (Oxford University) Euler Symposium, Saint Petersburg, Russia ...
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The physics of extra dimensions. LNGS 12 March 2001 *..and Berezinsky, Cassisi, Castellani, Degl'Innocenti, ... Stellar evolution and large extra dimensions ...
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Currently has the highest exposure above 10 EeV. HiRes ... Extragalactic component assuming uniform source density as in Berezinsky et al., hep-ph/0204357 ...
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Title: PowerPoint Presentation Author: GAZ Last modified by: GAZ Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3) Other titles
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Results from the HiRes Experiment Gordon Thomson University of Utah
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Belarus is a country with an ancient history, marvelous architecture, rich culture and, of course, distinctive traditions. It s Belarusian nature that makes the ...
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sources of UHECR are unknown: are they galactic or extragalactic (AGN, GRB, Hypernovae... The only information comes from observations of Faraday rotation ...
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The next 10 years in Particle Astrophysics Workshop summary Some personal observations Tribute to Alan
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What s new and what questions remain since our previous meeting? Workshop on Physics at the End of the Galactic Cosmic-ray Spectrum April 26-30, 2005
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d3 dc1 resceu ipmu ...
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Lorentz Invariant Violation and UHECR spectrum. Theoretical UHECR spectrum ... extragalactic. E(eV) GZK cutoff ? Hires VS. AGASA. If Hires, ...
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The Cosmological Energy Density of Neutrinos from Oscillation Measurements. Kev Abazajian ... Extended quintessence ('dark radiation') (Chen, Scherrer & Steigman 2001) ...
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Fly's Eye, Haverah Park, Akeno. mixed composition. Hires elongation rate ... acceleration energy is fixed by the geometry of the source and its magnetic field ...
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Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...
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... Proceedings of the 30th International Cosmic Ray ... 1 LORD Lunar Orbital Radio Detector 16 Detection of Ultrahigh-Energy Cosmic Rays and Neutrinos ...
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XXth Rencontres de Blois 'Challenges in Particle Astrophysics' ... inelasticity. Eikonal. Differential cross section. Amplitude ...
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(Some) Concepts of Condensed Matter Physics Anatoli Polkovnikov, Boston University AFOSR Fluctuations around mean field solution destroy long range order in 1D at all ...
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Anisotropy. Large scale patterns (dipole, quadrupole, galactic plane, ... galactic anisotropy (and it is hard to imagine how they accelerate to such high ...
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Leeds, July 23, 2004. in honor of Alan Watson ... pre-pre-production DAQ and main board. monitoring temperatures during austral winter ...
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Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
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Title: Neutrino Oscillations and the Sudbury Neutrino Observatory Author: wark Last modified by: Preferred Customer Created Date: 4/23/2001 9:02:18 AM
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UHE photons and neutrinos at the Pierre Auger Observatory Enrique Zas Departamento de F sica de Part culas & Instituto Galego de F sica de Altas Enerx as,
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To a good approximation atoms do not move and form a periodic lattice. ... We can have two electrons per each (lattice) momentum state due to spin degeneracy. ...
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Results of AGASA Experiment __Energy spectrum & Chemical composition __ Kenji SHINOZAKI Max-Planck-Institut f r Physik (Werner-Heisenberg-Institut)
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... Z=26 LB 1043.5 erg/s (G/3)2 b-1 Much dimmer sources are allowed as UHECR sources Survival from photodisintegration (tAg~ng sAg (r/G)
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Ultra High Energy Cosmic Rays Origin and Propagation of UHECRs
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Listening for Neutrinos The ACORNE Project
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... shock is formed when a faster shell catches up with a slower one. ... Acceleration time Wind ... Stecker (2000) - Only 10% of the cosmic rays observed above 10 ...
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Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
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The redshifted 21 cm background and particle decays. Evgenii O. ... baryon density fluctuations. density-velocity cross spectrum. velocity fluctuations ...
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AUGER experiment combining ground array with fluorescence such. will resolve most of this issues in 1-2 years from now. Statistics ... relict background n and g ...
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A question concerning consistency and suggestions for the resolution ... N(l, Eth) dl is the number of cosmic ray events which are originated from ...
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Sandip Pakvasa University of Hawaii Honolulu Pseudo-Dirac Neutrinos and Neutrinoless Double Beta Decay
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Neighbors: young and slim. Initial NS mass spectrum is unknown ... Young close-by NSs are slim 1.4Msun. Mass constraint can be useful for ...
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INAF-Istituto di Radioastronomia, Bologna, Italy. Rossella Cassano ... formalism (E-PS) CR in Galaxy Clusters. CR Confinment in Galaxy Clusters ...
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1912 Hess (Austrian) balloons to 5km, his sparks increase; ... a Tiger Woods tee shot, a Pete Sampras tennis serve, Or a speeding bullet. ...
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Constraining UHECR source spectrum from observations in GZK regime ... Convolve result with experimental exposure and take into account energy resolution. ...
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Hobbies: Reading, watching movies, psychology, biology, writing ... sport hall for playing games and ... contribution to different branches of ...
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Awaiting definitive air fluorescence yields (Sept 07? ... (Millenium Run, Springel et al 2004) Clustering of UHECR (if from galaxies) ...
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Telescope Array experiment
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Several experiments are aiming to detect the 'guaranteed' cosmogenic neutrino flux ... measuring cosmogenic neutrinos from heavy primaries is always less than ...
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as a classical field of Cooper pairs with center of mass at x. More ... The mesoscopic Cooper pairs contribution to the entropy density is less ...
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Predictions for the Detection of Neutralino Dark Matter
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The Highest Energy Particles
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The LHCf experiment at LHC
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QLG gives but possibly affected by dissipation and disorder ... QPS events dissipation via Josephson effect. voltage related to the rate of phase slips ...
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Institute of Physics, National Chiao-Tung University, Taiwan ... altitude of 4.8 km, and used a a gold leaf electroscope to measure the radiation. ...
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Kiel, Haverah Park, Fly's Eye, Akeno, Baksan, Tien-Shan, Ooty, Gulmarg, Plateu ... (quintessence) Wetterich 1988, Peebles & Vilenkin 1999 ...
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Optical X- ray. what is a galaxy cluster made of ? Coma Cluster. Galaxy cluster mass: ... Radio-X ray correlation observed for. Radio Halos suggest that a large ...
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Egret blazars. Blazars are AGN with jet. illuminating observer. Two-component spectra ... GeV g (Egret) TeV. ICHEP 2002, Amsterdam, July 31, 2002. Thomas K. Gaisser ...
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[Blandford 76; Lovelace 76] [Waxman 95, Vietri 95, Milgrom & Usov 95] ... Linda Smith (University College London), WIYN//NSF, NASA/ESA. Robert Gendler. M82 M81 ...
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C. W.Kim et al., S. Pakvasa ... Maximal mixing. CKM mixing. mD ~ mu ... P. F. Harrison. D. H. Perkins. W. G. Scott. Utbm = U23(p/4)U12 - maximal 2-3 mixing ...
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Enhanced flux possible thanks to halo density profile and substructure (as predicted by CDM) ... profile needed for DM substructure; some fine-tuning to get ...
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New Cosmic Rays at the Highest Energies
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