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Rencontres de Moriond EW 2008

1–8 mars 2008
La Thuile
Fuseau horaire Europe/Paris

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Session

Neutrinos, Astroparticles (I)

06am
6 mars 2008, 08:30
La Thuile

La Thuile

Rencontres de Moriond Planibel Hotel - La Thuile Aosta Valley 11016 La Thuile (Aosta), Italy Phone : 39 (0)1 65 88 45 41 Fax : 39 (0)1 65 88 45 35

Documents de présentation

Aucun document.

  1. 99. MiniBoone results
    Chris Polly (Indiana Univ. USA)
    06/03/2008 08:30
  2. 100. Anomally mediated neutrino-photon inteactions
    Richard Hill (Fermilab USA)
    06/03/2008 08:55
  3. 44. New interactions and neutrinos
    Prof. Ann Nelson (University of Washington)
    06/03/2008 09:15
    A "Chameleon" is a force whose apparent range and strength can depend on the size and density of the source. I discuss how a U(1) gauge force can be chameleonic due to screening from a light charged scalar. Such screening can weaken astrophysical constraints on new gauge bosons, allow a B-L interaction to be strong enough to affect short baseline neutrino oscillations, and change the...
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  4. 48. MiniBooNE, LSND, and sterile neutrinos
    Dr Thomas Schwetz-Mangold (CERN)
    06/03/2008 09:35
    I review the interpretation of the LSND signal in terms of sterile neutrino oscillations in the light of MiniBooNE results, considering 1, 2, or 3 sterile neutrinos with eV scale masses. Since no satisfactory fit to the global data is obtained in these cases, I speculate on a non-standard energy dependence of sterile neutrino oscillations, which can significantly improve the fit.
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  5. 101. Neutrino cross sections
    M. Teppei Katori (Indiana University)
    06/03/2008 10:10
  6. 102. Low energy effects of neutrino masses
    Dr Thomas Hambye Hambye (Service de Physique Theorique, Universite Libre de Bruxelles)
    06/03/2008 10:35
  7. 40. First Measurement of the Be-7 Solar Neutrino Flux by Borexino
    Dr Ferenc Dalnoki-Veress (Princeton University)
    06/03/2008 10:55
    Borexino is a large volume, real-time, liquid scintillator detector located at the Gran Sasso National Laboratory in Italy. The principal objective of the detector is to measure mono energetic (862 keV) Be-7 neutrinos from the sun present with a count rate of several tens of events per day. Measurement at this level requires an extremely low internal background due to natural radioactivity...
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  8. 103. XENON
    Roberto Santorelli (Zurich Univ. Switzerland)
    06/03/2008 11:15
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