Event calendar file
2-11 October 2008
San Carlos, Sonora, México
America/Hermosillo timezone
- bamr@nucleares.unam.mx
Support
Neutrino Physics
Place
Location: San Carlos, Sonora, México
Address: San Carlos Plaza Hotel,
Paseo Mar Bermejo Norte # 4.
Los Algodones, San Carlos Nuevo Guaymas,
Sonora, México 85506
Room: Room 2: Sirena
Date:
6 Oct 16:00 - 19:00
Timetable | Contribution List
Displaying 4
contributions
out of
4
Session:
Neutrino Physics
A variety of lepton flavour violating effects related to the recent discovery of neutrino oscillations and mixing is here systematically discussed in terms of an S3 flavour permutational symmetry. After a brief updated review of some relevant results on neutrino masses and mixings, that had been derived in the framework of a minimal S3-invariant extension of the Standard Model, we will give explic
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Presented by Prof. Alfonso MONDRAGON BALLESTEROS
on
7/10/2008
at
0:30
Session:
Neutrino Physics
Non-standard interactions (NSI) arise naturally in different models of physics beyond the Standard Model, and they can have an important influence in the solar neutrino analysis. In this talk, after a discussion of the solar neutrino data I will concentrate in present and future low-energy experiments and their sensitivity to NSI. The current status of NSI constraints will be introduced and it wil
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Presented by Dr. Omar MIRANDA
on
6/10/2008
at
23:00
Session:
Neutrino Physics
The MINERvA (Main INjector ExpeRiment for ν A) collaboration (http://minerva.fnal.gov//) in a neutrino scattering experiment which uses the NuMI beamline at Fermilab. It seeks to measure low energy neutrino interactions both to support neutrino oscillation experiments and to study the strong dynamics of the nucleon and nucleus that affect these interactions. It is currently in its final prototypi
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Presented by Dr. Julian FELIX
on
7/10/2008
at
0:00
Session:
Neutrino Physics
The gauge-singlet fermions, or right-handed neutrinos, are commonly introduced to explain the neutrino masses. If their Majorana mass terms are relatively small, new degrees of freedom appear in the low-energy effective theory as sterile neutrinos. The dark side of the neutrino sector may hold the key to explaining dark matter in the universe and the pulsar kicks, and it may play a role in other
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Presented by Dr. Alexander KUSENKO
