Neutrino Flavor Goniometry by High Energy Astrophysical Beams - INSPIRE

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Neutrino Flavor Goniometry by High Energy Astrophysical Beams

Sandip Pakvasa
(
- Hawaii U.
)

Mar, 2008

22 pages

Part of Proceedings, 4th International Symposium on Cosmology and particle astrophysics (CosPA 2007) : Taipei, Taiwan, November 13-15, 2007

Published in:

Mod.Phys.Lett.A 23 (2008) 1313-1324

Contribution to:

- CosPA 2007

e-Print:

0803.1701 [hep-ph]

DOI:

10.1142/S0217732308027680

Report number:

UH-511-1124-2008

View in:

ADS Abstract Service

reference search41 citations

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Abstract: (arXiv)

It is shown how high energy neutrino beams from very distant sources can be utilized to learn about many properties of neutrinos such as lifetimes, mass hierarchy, mixing, minuscule pseudo-Dirac mass splittings/ in addition, the production mechanism of neutrinos in astrophysical sources can also be elucidated.

talk: Taipei 2007/11/13
neutrino: beam
neutrino: cosmic radiation
cosmic radiation: particle source
neutrino: flavor
neutrino: oscillation
neutrino: mixing angle
mass: hierarchy
neutrino: mass difference
Cherenkov counter: water

References(83)

Figures(0)

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CHOOZ

Collaboration

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