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1018eV Neutrinos associated with UHECR (>1019eV) sources PowerPoint PPT Presentation
1018eV Neutrinos associated with UHECR (>1019eV) sources - 1018eV Neutrinos associated with. UHECR ( 1019eV) sources. Zhuo Li (??) ... Neutrino energy. en2n(en) For 10PeV protons, the fraction of total energy loss ...
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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???? ??????? D3 PowerPoint PPT Presentation
???? ??????? D3 - d3 dc1 resceu ipmu ...
d3 dc1 resceu ipmu ...
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Results%20of%20AGASA%20Experiment%20__Energy%20spectrum%20 PowerPoint PPT Presentation
Results%20of%20AGASA%20Experiment%20__Energy%20spectrum%20 - Results of AGASA Experiment __Energy spectrum & Chemical composition __ Kenji SHINOZAKI Max-Planck-Institut f r Physik (Werner-Heisenberg-Institut)
Results of AGASA Experiment __Energy spectrum & Chemical composition __ Kenji SHINOZAKI Max-Planck-Institut f r Physik (Werner-Heisenberg-Institut)
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Pierre%20Auger%20Observatory%20for%20UHE%20Cosmic%20Rays PowerPoint PPT Presentation
Pierre%20Auger%20Observatory%20for%20UHE%20Cosmic%20Rays - Pierre Auger Observatory. for UHE Cosmic Rays. Gianni Navarra (INFN ... light source flown on balloon. FD Calibration. Absolute: End to End Calibration ...
Pierre Auger Observatory. for UHE Cosmic Rays. Gianni Navarra (INFN ... light source flown on balloon. FD Calibration. Absolute: End to End Calibration ...
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The Aperture and Precision of the Auger Observatory PowerPoint PPT Presentation
The Aperture and Precision of the Auger Observatory - ... eye give angular resolution comparable to 'stereo' reconstruction ... Note the significant aperture at 1018eV, and the stereo aperture at the higher energies ...
... 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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The%20Status%20of%20the%20Pierre%20Auger%20Observatory PowerPoint PPT Presentation
The%20Status%20of%20the%20Pierre%20Auger%20Observatory - The Status of the Pierre Auger Observatory. Bruce Dawson ... Millard county. Utah, USA. Southern hemisphere: Malarg e. Provincia de Mendoza. Argentina ...
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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Presentazione%20di%20PowerPoint PowerPoint PPT Presentation
Presentazione%20di%20PowerPoint - Extreme Universe Space Observatory DETECTING NEUTRINOS WITH EUSO Sergio Bottai INFN Firenze on behalf of the EUSO Collaboration Paris neutrino2004
Extreme Universe Space Observatory DETECTING NEUTRINOS WITH EUSO Sergio Bottai INFN Firenze on behalf of the EUSO Collaboration Paris neutrino2004
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Examples of Science PowerPoint PPT Presentation
Examples of Science - For Sources with tgp 1: Strongest know z evolution (QSO, SFR): collect n's beyond GZK ... tgp for known sources. ep. e'g. n. p e e- eg. Antares. Nemo ...
For Sources with tgp 1: Strongest know z evolution (QSO, SFR): collect n's beyond GZK ... tgp for known sources. ep. e'g. n. p e e- eg. Antares. Nemo ...
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Preliminary Profile Reconstruction of EA Hybrid Showers PowerPoint PPT Presentation
Preliminary Profile Reconstruction of EA Hybrid Showers - ... to combine signal from all pixels seeing shower during a given ... for every 100ns time bin include signal from pixels with centres within c of spot centre. ...
... to combine signal from all pixels seeing shower during a given ... for every 100ns time bin include signal from pixels with centres within c of spot centre. ...
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AUGER Experiment Status and Performances PowerPoint PPT Presentation
AUGER Experiment Status and Performances - key com.apple.print.ticket.creator /key string com.apple.printingmanager /string ... key com.apple.print.ticket.creator /key string com.apple.print.pm. ...
key com.apple.print.ticket.creator /key string com.apple.printingmanager /string ... key com.apple.print.ticket.creator /key string com.apple.print.pm. ...
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The Pierre Auger Project PowerPoint PPT Presentation
The Pierre Auger Project - Summer School on Particle and Nuclear Astrophysics ... Radiosonde. Balloon-borne radiosondes are planned to monitor the atmosphere's density and ...
Summer School on Particle and Nuclear Astrophysics ... Radiosonde. Balloon-borne radiosondes are planned to monitor the atmosphere's density and ...
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COSMIC RAY ORIGINS PowerPoint PPT Presentation
COSMIC RAY ORIGINS - COSMIC RAY ORIGINS
COSMIC RAY ORIGINS
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Gamma-ray Bursts and Particle Acceleration PowerPoint PPT Presentation
Gamma-ray Bursts and Particle Acceleration - 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 ...
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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Diffusion of UltraHigh Energy Particles in Expanding Universe PowerPoint PPT Presentation
Diffusion of UltraHigh Energy Particles in Expanding Universe - 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
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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Origin%20of%20Ultra%20High%20Energy%20Cosmic%20Rays PowerPoint PPT Presentation
Origin%20of%20Ultra%20High%20Energy%20Cosmic%20Rays - anisotropy expectations. for different AGN types. Takami, SI , in prep. ... characteristic spectra, anisotropy, composition. hard X-rays TeV gamma-rays. AGNs ...
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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Astrophysics of high energy cosmicrays PowerPoint PPT Presentation
Astrophysics of high energy cosmicrays - 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 ...
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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Tom Gaisser, PowerPoint PPT Presentation
Tom Gaisser, - The next 10 years in Particle Astrophysics Workshop summary Some personal observations Tribute to Alan
The next 10 years in Particle Astrophysics Workshop summary Some personal observations Tribute to Alan
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Astroparticle Physics with High Energy Neutrinos: from AMANDA to IceCube PowerPoint PPT Presentation
Astroparticle Physics with High Energy Neutrinos: from AMANDA to IceCube - Astroparticle Physics with High Energy Neutrinos: from AMANDA to IceCube
Astroparticle Physics with High Energy Neutrinos: from AMANDA to IceCube
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Systematics in the Pierre Auger Observatory PowerPoint PPT Presentation
Systematics in the Pierre Auger Observatory - Fluorescence - a technique with great rewards, but a lot of ... corrector lens. camera. 440 PMTs. 11 m2 mirror. UV-Filter 300-400 nm. No coma, good ... Camera ...
Fluorescence - a technique with great rewards, but a lot of ... corrector lens. camera. 440 PMTs. 11 m2 mirror. UV-Filter 300-400 nm. No coma, good ... Camera ...
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Neutrino astronomy and telescopes PowerPoint PPT Presentation
Neutrino astronomy and telescopes - Crab nebula Cen A Teresa Montaruli, Assistant Professor, Chamberlin Hall, room 5287, tmontaruli@icecube.wisc.edu Neutrino astronomy and telescopes
Crab nebula Cen A Teresa Montaruli, Assistant Professor, Chamberlin Hall, room 5287, tmontaruli@icecube.wisc.edu Neutrino astronomy and telescopes
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High Energy CosmicRays and High Energy Neutrino Astronomy PowerPoint PPT Presentation
High Energy CosmicRays and High Energy Neutrino Astronomy - XG cosmic accelerators? They exist 1020 eV cosmic-rays detected 1019 eV: Isotropic ... Jet content (kinetic/Poynting) Particle acceleration. Radiation mechanisms ...
XG cosmic accelerators? They exist 1020 eV cosmic-rays detected 1019 eV: Isotropic ... Jet content (kinetic/Poynting) Particle acceleration. Radiation mechanisms ...
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The Second International Workshop on Ultra-high-energy cosmic rays and their sources PowerPoint PPT Presentation
The Second International Workshop on Ultra-high-energy cosmic rays and their sources - 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 ...
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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Propagation of Ultrahigh Energy Cosmic Rays in Local Magnetic Fields PowerPoint PPT Presentation
Propagation of Ultrahigh Energy Cosmic Rays in Local Magnetic Fields - However, HiRes observation showed the distribution has no small scale anisotropy. ... panels, MFs, especially EGMF, makes the small-scale anisotropy be weaken. ...
However, HiRes observation showed the distribution has no small scale anisotropy. ... panels, MFs, especially EGMF, makes the small-scale anisotropy be weaken. ...
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Phenomenology of Cosmic Ray Air Showers PowerPoint PPT Presentation
Phenomenology of Cosmic Ray Air Showers - For SOFT processes the rates and properties are dominated by non-perturbative QCD effects ... Pierre Auger Observatory: - New arsenal of 'hybrid' data. ...
For SOFT processes the rates and properties are dominated by non-perturbative QCD effects ... Pierre Auger Observatory: - New arsenal of 'hybrid' data. ...
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AGASA PowerPoint PPT Presentation
AGASA - Detector response(box, housing) 5% Energy Estimator S(600) ... AGASA fast simulation (based on empirical formula and toy simulation) Based on CORSIKA M.C. ...
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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The case for High energy neutrino astronomy PowerPoint PPT Presentation
The case for High energy neutrino astronomy - [Blandford 76; Lovelace 76] [Waxman 95, Vietri 95, Milgrom & Usov 95] ... Linda Smith (University College London), WIYN//NSF, NASA/ESA. Robert Gendler. M82 M81 ...
[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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Recent%20Results%20for%20Small-Scale%20Anisotropy%20with%20HiRes%20Stereo%20Data PowerPoint PPT Presentation
Recent%20Results%20for%20Small-Scale%20Anisotropy%20with%20HiRes%20Stereo%20Data - ... Results for Small-Scale Anisotropy with HiRes Stereo Data. Chad ... A cosmic ray induces a shower in the atmosphere which can be ... scale anisotropy searches ...
... Results for Small-Scale Anisotropy with HiRes Stereo Data. Chad ... A cosmic ray induces a shower in the atmosphere which can be ... scale anisotropy searches ...
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Photons and Neutrinos Originating from Accelerated Protons in GRBs PowerPoint PPT Presentation
Photons and Neutrinos Originating from Accelerated Protons in GRBs - Future observations of gamma-rays and neutrinos from mesons will justify the ... Fermi Acceleration. v. u. Shock Front. Shocked Region. Magnetic Field. Particle ...
Future observations of gamma-rays and neutrinos from mesons will justify the ... Fermi Acceleration. v. u. Shock Front. Shocked Region. Magnetic Field. Particle ...
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Diffusion of UltraHigh Energy Particles in Expanding Universe PowerPoint PPT Presentation
Diffusion of UltraHigh Energy Particles in Expanding Universe - sources of UHECR are unknown: are they galactic or extragalactic (AGN, GRB, Hypernovae... The only information comes from observations of Faraday rotation ...
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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New Views on the Universe PowerPoint PPT Presentation
New Views on the Universe - Sagittarius A* (2003. 2 Tel.) - 11 sigma. HESS Galactic Center! ... Constellation-X, GLAST, ACTs(Hess, Cangaroo3, Magic, Veritas) ...
Sagittarius A* (2003. 2 Tel.) - 11 sigma. HESS Galactic Center! ... Constellation-X, GLAST, ACTs(Hess, Cangaroo3, Magic, Veritas) ...
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gray Burst Physics PowerPoint PPT Presentation
gray Burst Physics - [Taylor et al. 04] Dynamics 101b. 2qj. G(R) 1/qj. Rj 'Ignorant' jet/observer ... SWIFT Afterglows. II. Challenges. Collisionless shock physics (ee, eB ...
[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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Scientific Case for All Sky Coverage with the Northern Auger PowerPoint PPT Presentation
Scientific Case for All Sky Coverage with the Northern Auger - Trapped in Galactic Halo (like Cold Dark Matter) ... ANITA 30 days. IceCube (? ) 3 yrs. AGASA. Compiled by Stephane Coutu. Strong DIS. No DIS ...
Trapped in Galactic Halo (like Cold Dark Matter) ... ANITA 30 days. IceCube (? ) 3 yrs. AGASA. Compiled by Stephane Coutu. Strong DIS. No DIS ...
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Tom Gaisser, PowerPoint PPT Presentation
Tom Gaisser, - Leeds, July 23, 2004. in honor of Alan Watson ... pre-pre-production DAQ and main board. monitoring temperatures during austral winter ...
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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Recherche de photons dultra haute nergie dans les donnes de lobservatoire Pierre Auger PowerPoint PPT Presentation
Recherche de photons dultra haute nergie dans les donnes de lobservatoire Pierre Auger - Recherche de photons dultra haute nergie dans les donnes de lobservatoire Pierre Auger
Recherche de photons dultra haute nergie dans les donnes de lobservatoire Pierre Auger
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Photons and Neutrinos Originating from Accelerated Protons in GRBs PowerPoint PPT Presentation
Photons and Neutrinos Originating from Accelerated Protons in GRBs - Pion-decay time and cooling time- More detailed simulation ... Synchrotron radiation from electron, positron, muon, pion, and proton. Photon scattering (Inv. ...
Pion-decay time and cooling time- More detailed simulation ... Synchrotron radiation from electron, positron, muon, pion, and proton. Photon scattering (Inv. ...
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Telescope Array experiment PowerPoint PPT Presentation
Telescope Array experiment - Telescope Array experiment
Telescope Array experiment
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Modeling the Radiation from the Supernova Remnant of SN1006 PowerPoint PPT Presentation
Modeling the Radiation from the Supernova Remnant of SN1006 - Modeling the Radiation from the Supernova Remnant of SN1006
Modeling the Radiation from the Supernova Remnant of SN1006
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Particle Acceleration PowerPoint PPT Presentation
Particle Acceleration - Well established facts for the Shock Acceleration theory: ... ECR ~ Egas ~ EB ~ ECMBR ~ 10-12 erg/cm3. dynamically important in the ISM of galaxies ...
Well established facts for the Shock Acceleration theory: ... ECR ~ Egas ~ EB ~ ECMBR ~ 10-12 erg/cm3. dynamically important in the ISM of galaxies ...
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The Highest Energy Particles PowerPoint PPT Presentation
The Highest Energy Particles - The Highest Energy Particles
The Highest Energy Particles
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The importance of knowing the primary mass and how little we really know PowerPoint PPT Presentation
The importance of knowing the primary mass and how little we really know - The importance of knowing the primary mass and how little we ... 'Fere libenter homines id, quod volunt, credunt!' 'Men wish to believe only what they prefer' ...
The importance of knowing the primary mass and how little we ... 'Fere libenter homines id, quod volunt, credunt!' 'Men wish to believe only what they prefer' ...
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Limites suprieures au flux de photons UHE avec lobservatoire Pierre Auger PowerPoint PPT Presentation
Limites suprieures au flux de photons UHE avec lobservatoire Pierre Auger - Pr dictions et limites actuelles pour les fractions de photons ... Baisse de la section efficace ?/air. Effet LPM pour les ? E 1019. Conversion de ? ...
Pr dictions et limites actuelles pour les fractions de photons ... Baisse de la section efficace ?/air. Effet LPM pour les ? E 1019. Conversion de ? ...
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New Cosmic Rays at the Highest Energies PowerPoint PPT Presentation
New Cosmic Rays at the Highest Energies - New Cosmic Rays at the Highest Energies
New Cosmic Rays at the Highest Energies
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Prospects in the EUSO project PowerPoint PPT Presentation
Prospects in the EUSO project - No clue of GZK cut @ 5 1019 ? JPM- LAPP-Les Houches ... The GKZ cut-off ... interest because of the 'GZK cut-off' (Greisen, 1966; Zatsepin and Kuz'min, 1966) ...
No clue of GZK cut @ 5 1019 ? JPM- LAPP-Les Houches ... The GKZ cut-off ... interest because of the 'GZK cut-off' (Greisen, 1966; Zatsepin and Kuz'min, 1966) ...
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Corinne B PowerPoint PPT Presentation
Corinne B - Title: Diapositive 1 Author: Corinne Berat Last modified by: Corinne Berat Created Date: 9/17/2002 7:39:20 PM Document presentation format: Affichage l' cran
Title: Diapositive 1 Author: Corinne Berat Last modified by: Corinne Berat Created Date: 9/17/2002 7:39:20 PM Document presentation format: Affichage l' cran
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P'Auger, a major step: PowerPoint PPT Presentation
P'Auger, a major step: - surface array (water Cerenkov tanks) fluorescence detector ... (with flamenco dancers), Nov. 2000. Official ribbon cutting, Nov. 2000. Open house for the public ...
surface array (water Cerenkov tanks) fluorescence detector ... (with flamenco dancers), Nov. 2000. Official ribbon cutting, Nov. 2000. Open house for the public ...
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HiRes Mapping the High Energy Universe PowerPoint PPT Presentation
HiRes Mapping the High Energy Universe - Gamma-ray Astronomy photons from MeV to TeV ... rays, BL Lacertae, and EGRET detections: A new way to identify EGRET sources? ...
Gamma-ray Astronomy photons from MeV to TeV ... rays, BL Lacertae, and EGRET detections: A new way to identify EGRET sources? ...
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Recent Results in Cosmic Ray Studies and Future Projects PowerPoint PPT Presentation
Recent Results in Cosmic Ray Studies and Future Projects - Recent Results in Cosmic Ray Studies and Future Projects
Recent Results in Cosmic Ray Studies and Future Projects
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Mthodes exprimentales pour ltude du rayonnement cosmique PowerPoint PPT Presentation
Mthodes exprimentales pour ltude du rayonnement cosmique - 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) ...
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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