'Neutrino oscillation' diaporamas de présentation

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab. Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology Southern Methodist-U HEP seminar, Dallas, September, 27, 2010. MiniBooNE, a neutrino oscillation experiment at Fermilab. Outline

1.19k views • 111 slides

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab. Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology Southern Methodist-U HEP seminar, Dallas, September, 27, 2010. MiniBooNE, a neutrino oscillation experiment at Fermilab. Outline

1.3k views • 111 slides

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab. Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology U-Glasgow HEP seminar, Glasgow, Scotland, Mar. 21, 2011. MiniBooNE, a neutrino oscillation experiment at Fermilab. Outline

1.05k views • 87 slides

MiniBooNE, a neutrino oscillation experiment at Fermilab

MiniBooNE, a neutrino oscillation experiment at Fermilab. Outline Introduction 2. Neutrino beam 3. Events in the detector 4. Cross section model 5. Neutrino oscillation result 6. Anti-neutrino oscillation result 7. Outlook .

875 views • 66 slides

Neutrino o scillation physics II

652 views • 51 slides

Future Atmospheric Neutrino Experiments

Future Atmospheric Neutrino Experiments. Naba K Mondal Tata Institute of Fundamental Research Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.

599 views • 47 slides

NUINT11, Dehradun March 9, 2011

Neutrino-Nucleus Reactions at MeV Region based on New Shell-Model Hamiltonians Toshio Suzuki Nihon University. NUINT11, Dehradun March 9, 2011. Neutrino energy: < 100 MeV Shell model: Our work is based on Recent advances in shell model calculations, owing to

549 views • 42 slides

Neutrino Masses and Mixings

584 views • 41 slides

Neutrinos: At the Heart of the Matter?

524 views • 40 slides

Type II Seesaw Portal and PAMELA/Fermi LAT Signals

Type II Seesaw Portal and PAMELA/Fermi LAT Signals. Toshifumi Yamada Sokendai, KEK In collaboration with Ilia Gogoladze, Qaisar Shafi (Univ. of Delaware) and Nobuchika Okada (Univ. of Alabama) 12/11/2009, HEAP2009@KEK.

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500 views • 38 slides

M.Nakahata Kamioka observatory, ICRR, IPMU, Univ. of Tokyo

Kamiokande and Super- Kamiokande Results on Neutrino Astrophysics. M.Nakahata Kamioka observatory, ICRR, IPMU, Univ. of Tokyo. Professor Yoji Totsuka (1942-2008). Kamiokande spokesman: 1987 April ---- end. Super-Kamiokande spokesman: beginning ---- 2002.

630 views • 38 slides

Shinya Kanemura (Osaka Univ.)

A Study on muon (electron) to tau conversion in Deep Inelastic Scattering. Yoshitaka Kuno (Osaka), Toshihiko Ota (TU Munich) Masahiro Kuze, Tomoyasu Takai (Tokyo Inst. Tech.). Shinya Kanemura (Osaka Univ.).

524 views • 37 slides

Hallsie Reno Trento, May 2005

Neutrino-nucleon interactions: what can we learn from electromagnetic interactions and quark-hadron duality?. Hallsie Reno Trento, May 2005. Advertisement for neutrino physics in context of this workshop. (Ultra)-high energy neutrinos:. Neutrino induced air showers

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Marco G. Giammarchi Istituto Nazionale di Fisica Nucleare

498 views • 33 slides

Bruno Pontecorvo

Bruno Pontecorvo. Pontecorvo Prize is very special for us: All the important works done by Super- Kamiokande point back to Bruno Pontecorvo 1957 First idea of a Neutrino Osicllation 1978 First idea to use atmospheric neutrinos to study neutrino oscillations (w/ Bilenky )

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Comparing Super-K to Hyper-K: Attenuation Length

Comparing Super-K to Hyper-K: Attenuation Length. Karl Ahrendsen Buena Vista University Dr. Chris Walter and Dr. Kate Scholberg. Outline. Super K -> Hyper K and why My Project: Examining the attenuation length. Super K( amiokaNDE ). Kamiokande -> Not big enough

280 views • 14 slides

Neutrino Mass and Spontaneous Parity Nonconservation

Neutrino Mass and Spontaneous Parity Nonconservation Rabindra N. Mohapatra ( Department of Physics, City College of New York) Goran Senjanovic ( Department of Physics and Astronomy, University of Maryland) Published on 10 December 1979 Presented by Stephen Bello, September 3 2013.

197 views • 13 slides

ECFA conclusions (I)

ECFA conclusions (I). ECFA Review Panel for future large infrastructures for neutrino oscillation experiments mandate and term of reference agreed chair and members ratified ECFA Review Panel for Detector R&D mandate and term of reference agreed start to search chair and members

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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:

218 views • 1 slides