'Neutrino astronomy' diaporamas de présentation

Neutrino astronomy with AMANDA and IceCube

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Aktuelle Ergebnisse und Zukunft der Neutrinoastronomie

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Future methods::Radio

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Emilio Migneco

Emilio Migneco. Erice ISCRA School 2004. Introduction to High energy neutrino astronomy. Topics. 1) Introduction to high energy neutrino astronomy Motivations for HE neutrino astronomy HE neutrino sources Neutrino telescopes operation principles Backgrounds

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Neutrino Mass

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Neutrino astronomy

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Chapter 15: The Sun: A Nuclear Powerhouse

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Showering Neutrino Astronomies at Horizons

Showering Neutrino Astronomies at Horizons. Update article. Why Neutrino may see where and what gamma and UHECR are no allowed to. accelerated protons interact:. => the energy fluences in ?-rays and neutrinos are comparable due to isospin symmetry.

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Neutrino Astronomy at the South Pole

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Neutrino Astronomy at the South Pole

Neutrino Astronomy at the South Pole. David Boersma UW Madison Lake Louise Winter Institute Chicago, 23 February 2006. IceCube Collaboration. Alabama University, USA University of Alaska, Anchorage, USA Bartol Research Institute, Delaware, USA Pennsylvania State University, USA

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Calorimetry (GeV-EeV) in AMANDA and IceCube Neutrino Telescopes

457 views • 27 slides

Probing for Leptonic Signatures from Gamma-Ray Bursts with Antarctic Neutrino Telescopes

Probing for Leptonic Signatures from Gamma-Ray Bursts with Antarctic Neutrino Telescopes. M ICHAEL S TAMATIKOS U NIVERSITY OF W ISCONSIN, M ADISON D EPARTMENT OF P HYSICS michael.stamatikos@icecube.wisc.edu

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Title

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Some Lessons Learned from Deep Oceanographic Neutrino Telescopes

Pacific Ocean Neutrino Explorer (P-ONE) General Meeting 22 July 2019 University of Alberta. Some Lessons Learned from Deep Oceanographic Neutrino Telescopes. John G. Learned University of Hawaii.

191 views • 19 slides

Neutrino emission

Neutrino emission. <E>=0.27 MeV. E=0.39,0.86 MeV. <E>=6.74 MeV. ppIII loss: 28%. ppII loss: 4%. ppI loss: ~2%. note: <E>/Q= 0.27/26.73 = 1%. Total loss: 2.3%. 2 neutrino energies from 7Be electron capture ?. 7 Be + e - ? 7 Li + n e. E n. E n. Continuous fluxes in /cm 2 /s/MeV

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Lorenzo Perrone (University & INFN of Lecce) for the MACRO Collaboration

TAUP 2001 Topics in Astroparticle and underground physics. Laboratori Nazionali del Gran Sasso, Italy September 8-12, 2001. Neutrino astronomy with MACRO. Lorenzo Perrone (University & INFN of Lecce) for the MACRO Collaboration. Summary of contents. Frame Hypotheses.

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The M aier- L eibnitz- L aboratory for Nuclear and Particle Physics of LMU Munich and TU Munich

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Welcome to the 2nd edition of TeV Particle Astrophysics Madison WI, 28-31 Aug 2006

Welcome to the 2nd edition of TeV Particle Astrophysics Madison WI, 28-31 Aug 2006. LOC: Albrecht Karle Francis Halzen Teresa Montaruli. Welcome to the 2nd edition of TeV Particle Astrophysics Madison WI, 28-31 Aug 2006. 1st edition was held at Fermilab, Batavia, IL, on July 13-15, 2005

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Experimental Astroparticle Physics

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July 30 th , Friday

July 30 th , Friday. Morning Session: Particle Astrophysics Organizers: L. Cominsky and F. Halzen Chair: Lynn Cominsky 8:40 Francis Halzen (Wisconsin): Particle astrophysics with cosmic hadrons, photons and neutrinos

125 views • 1 slides