Day
1
Monday 18 |
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Atmospheric neutrinos and neutrino telescopes | |||
Convener : C. Tao | |||
Latest results from SuperKamiokande | Y. Totsuka |
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PDF / PPT |
Atmospheric neutrino production | T. Montaruli |
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Neutrino Telescopes | J. Learned |
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High Energy Astrophysics Sources | J. Rachen | ||
Afternoon sessions | Convener : S. Tilav |
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Ultrahigh energy cosmic rays and string theory | M. Pluemacher | PDF / PS | |
High-energy neutrino conversion and the lepton asymmetry | C. Lunardini |
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PDF / PS |
Non-adiabatic oscillations of (supernova) neutrinos | M. Kachelriess | PDF / PS | |
Determination of the atmospheric neutrino oscillation parameters with ANTARES | R. Hubbard |
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PDF / PPT |
Supernova detection with AMANDA | A. Bouchta |
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Overview of the recent AMANDA results | C. de los Heros |
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PDF / PPT |
EUSO as neutrino telescope and related experiments | J-P. Mendiburu | PDF / PPT | |
Review of MACRO results | T. Montaruli |
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After dinner session | Convener : J. Bouchez |
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First public SNO results | K. Heeger |
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PDF / PPT |
Day
2
Tuesday 19 |
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Stellar neutrinos | |||
Convener : J. Bouchez |
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Solar neutrinos analysis and future | D. Vignaud |
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Solar Models | S. Turck-Chièze |
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Supernovae | P. Vogel |
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Afternoon sessions | Convener : M. Cribier |
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Sterile neutrino: a good Warm Dark Matter candidate? | S. Hansen |
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Reviving the Energy independent Suppression of the Solar Neutrino Flux | D.P. Roy |
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QED corrections to the Scattering of Solar Neutrinos electrons | M. Passera |
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Theoretical estimates of the neutrino interaction cross section | C. Volpe |
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Status of the Galactic and Solar detectors OMNIS and SIREN | I. Liubarsky |
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Comments and perspective for Solar Neutrinos | M. Cribier |
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Day
3
Wednesday 20 |
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Combined Analyses | |||
Convener : S. Katsanevas |
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Medium Baseline (Karmen, LSND, Boone) | A. Bazarko |
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PDF / PPT |
Direct Mass Measurements | C. Weinheimer |
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PDF / PS |
Implications of oscillation parameters for neutrinoless beta decay | S. Petcov |
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A global 3 flavors analysis | G. Fogli |
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Solar and Atmospheric Four-Neutrino Oscillations | M.C. Gonzalez-Garcia |
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PDF / PS |
Afternoon sessions | Convener : A.Y. Smirnov |
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BOONE | F. Garcia | ||
Non Standard Analysis of the Solar Neutrino Anomaly | A. Strumia |
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PDF / PS |
4 Neutrino Schemes in Future Experiments | C. Pena-Garay |
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PDF / PS |
A Combined Fit to the LSND and Atmospheric Anomalies | S. Skadhauge |
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PDF / PS |
4-Neutrino Mass Schemes and the Likelihood of (3+1)-Mass Spectra | T. Schwetz |
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Proceedings /
PDF / PS |
Neutrino Mass Spectrum and Beta Decay | Y. Farzan | ||
Day
4
Thursday 21 |
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Long Baselines | |||
Convener : J. Marteau | |||
K2K | K. Nakamura |
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PDF / PPT |
MINOS | D. Harris |
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The European Long Baseline Program | D. Autiero | PDF / PPT | |
Neutrino factories | A. Blondel | ||
Afternoon sessions | Convener : A. Rubbia | ||
Status ICARUS | A. Rubbia | ||
CP and T violation searches at neutrino factories | M. Campanelli | PDF / PPT | |
Parameter correlations in neutrino factory experiments | M. Freund |
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Neutrino Oscillations with Two $\Delta m^2$ Scales | I. Mocioiu |
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Very Long Baselines with Neutrino Narrow Band Beams | F. Pierre |
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PDF / PS |
DONUT | N. Saoulidou |
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Matter effects | S. Umasankar |
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Day
5
Friday 22 |
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Theoretical models, future and Cosmology | |||
Convener : J. Orloff |
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Models for Small Neutrino Masses, with and without Extra Dimensions | P. Ramond |
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Neutrino Masses: Model Building | M. Lola |
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PDF / PS |
Neutrino Mass Patterns : Bottom Up Approach | F. Feruglio |
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Neutrino Mass and Universe's Baryon Asymmetry | T. Yanagida |
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Outlook and Perspective on Neutrino Masses and Mixings | G. Altarelli | ||
Afternoon sessions | Convener : S. King |
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Introduction | S. King |
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RGE analysis of neutrino mass matrix | G-H. Wu | ||
Insights on neutrino masses from lepton flavour violation | I. Masina |
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Neutrinos and extra dimensions : a solution to fit the data | N. Cosme |
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Leptogenesis in left-right symmetric theories | W. Rodejohann |
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How Cosmology Constrains Neutrino Oscillations | D. Kirilova |
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Texture Models, Neutrino Observables and Leptogenesis | M. Hirsch |
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PDF / PS |
Baryogenesis via lepton number violation in Anti-GUT model | Y. Takanishi |
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PDF / PS |
PDF is very inefficient for vectorially encode scatter plots generated by PAW (e.g. 60+ Mb from a 5 Mb gzipped PostScript file). For printing, use the gzipped "PS" version containing the scalable vector drawings, and only use the bitmap PDF file for quickly viewing on the screen.
When available, we kept the PowerPoint (PPT) source for the benefit
of those that can use, read and edit this format.