'Tau neutrino' diaporamas de présentation

Alain Blondel

Neutrino Physics. Alain Blondel. 1. What are neutrinos and how do we know ? 2. Standard Model neutrino properties 3. Neutrino transitions and neutrino mass 4. neutrino oscillations and CP violation 5. on-going and future neutrino experiments on oscillations

737 views • 72 slides

DONUT - Observation of n t Interactions

DONUT - Observation of n t Interactions. Reinhard Schwienhorst University of Minnesota. The DONUT collaboration :

579 views • 42 slides

What Are Neutrinos Anyway and What Is All This Fuss About?

411 views • 31 slides

CNGS: First Year of Operation

CNGS: First Year of Operation. E. Gschwendtner AB/ATB on behalf of the CNGS team. Flavor states:. Mass states:. ~. Introduction. Neutrino Parameter Status: July 2008 Review of Particle Physics.

442 views • 26 slides

A HiRes Limit On Cosmogenic Neutrino Flux

A HiRes Limit On Cosmogenic Neutrino Flux. Weiran Deng High Energy Astrophysics Institute University of Utah APS-DPF 2006+JPS2006, Hawaii. AGASA. HR2. HR1. Auger. UHE Cosmic Ray Spectrum and GZK. Fits interpret spectrum in terms of extragalactic protons that traveled from

164 views • 16 slides

The History of Standard Model

The History of Standard Model. 1. The Nobel Prize winner. 1979 Nobel Prize-- GLASHOW, SALAM and WEINBERG. the theory of the unified weak and electromagnetic interaction. 1984 Nobel Prize-- RUBBIA and VAN DER MEER.

540 views • 13 slides

Neutrinos

284 views • 5 slides

1998: Discovery that Neutrinos H ave S mall Mass

What is a Neutrino?. Detection of Neutrinos and the Super Kamiokande detector. Neutrino Oscillation and Mass. T . A neutrino is a subatomic particle with no charge. There are three flavors:

221 views • 1 slides