'Proton decay' diaporamas de présentation

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discovering neutrinos: from the earth...the sun... our sister galaxy...

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Takaaki Kajita (ICRR, U.of Tokyo)

III International Pontecorvo Neutrino Physics School Alushta, Ukraine, Sep. 2007. Atmospheric neutrinos -status and prospect-. Production of atmospheric neutrinos Some early history (Discovery of atmospheric neutrinos, Atmospheric neutrino anomaly) Discovery of neutrino oscillations

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Supersymmetry I

Supersymmetry I. Hitoshi Murayama Taiwan Spring School March 29, 2002. Why Beyond the Standard Model. Standard Model is sooooo successful. But none of us are satisfied with the SM. Why? Because it leaves so many great questions unanswered ? Drive to go beyond the Standard Model.

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Projet d'extension du Laboratoire souterrain de Modane

Projet d'extension du Laboratoire souterrain de Modane. F. Piquemal Laboratoire Souterrain de Modane (CNRS/IN2P3 ). Conseil scientifique IN2P3, 5 mai 2011. Deep Underground Laboratories. Soudan. Boulby. SNOLab. YangYang. DUSEL Homestake. Modane. Canfranc. Gran Sasso. WIPP. Kamioka.

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Fermion Masses and Unification

Fermion Masses and Unification. Steve King University of Southampton. Lecture 2. Unification. Most popular Groups are:. Quarks, Leptons. Quarks, Leptons, right-handed neutrino. Quarks, Leptons, exotics, SM singlet,. GUTs. Simple Group.

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E.M.Drobyshevski

Dark Electric Matter Objects: History of Discovery, Modes of Interaction with Matter, Some Inferences and Prospects. E.M.Drobyshevski Ioffe Physico-Technical Institute Russian Academy of Sciences 194021 St.Petersburg, Russia E-mail: emdrob@mail.ioffe.ru. The Talk Outline

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Neutrino Oscillations, Proton Decay and Grand Unified Theories

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International Underground science: Status and Prospects

International Underground science: Status and Prospects. Fabrice Piquemal Laboratoire Souterrain de Modane (CNRS/IN2P3 and CEA/IRFU) and CENBG (CNRS/IN2P3 and Bordeaux I university). IoP meeting April,29-31 UCL.

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Challenges for EURISOL and the EURISOL Design Study

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Mikhail Kirsanov , For the CMS collaboration

Search for Pair Production of 1 st Generation Scalar Leptoquarks Using Events Containing 2 Electrons and 2 Jets Produced in pp Collisions at ?s=7 TeV. Mikhail Kirsanov , For the CMS collaboration

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Novel LAr TPC developments for neutrino and astrophysics

Novel LAr TPC developments for neutrino and astrophysics. A. Badertscher, L. Kaufmann, L. Knecht, M. Laffranchi, A. Marchionni , G. Natterer, P. Otiougova, F. Resnati, A. Rubbia, T. Viant ETH Zurich CHIPP Workshop on Detector R&D, June 2008. A precision detector for proton decay searches

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Anomalous U(1) GUT

Anomalous U(1) GUT. Introduction Anomalous U(1) GUT Horizontal symmetry Summary and Discussion. Toshifumi YAMASHITA (Kyoto University). 2004/12/7 @UC Irvine. SUSY?. Introduction. Higgs?. hierarchal Yukawa?. SUSY-GUT. fascinating extension of SM gauge coupling unification (GCU).

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Rare Decays in Theories with LGS

Rare Decays in Theories with LGS. Cosimo Bambi Wayne State University. Search for B and L Number Violations , Berkeley, 22 September 2007. Based on the paper: C. Bambi, A.D. Dolgov and K. Freese, NPB 763, 91 (2007) [arXiv:hep-ph/0606321]. Outline. Gravitational Decays

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A super-dense ice detector for SN neutrinos and proton decay at the South Pole

A super-dense ice detector for SN neutrinos and proton decay at the South Pole. Marek Kowalski, Bonn University. MICA - Mega Ton Ice Cherenkov Array. IceCube ? DeepCore ? PINGU ? MICA So far, MICA is an idea and not yet a well defined project. Today I highlight two novel aspects:

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Proton decay studies in Liquid Argon TPC

Proton decay studies in Liquid Argon TPC. Dorota Stefan Epiphany Conference on Neutrinos and Dark Matter 5 - 8 January 2006, Cracow, Poland. References. L. E. Ibanez, CERN-TH.5237/88 Hitoshi Murayama and Aaron Pierce, Phys. Rev. D.65.055009(2002)

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Sadia Khalil & Sheldon Stone Syracuse University 03/30/2007

Sadia Khalil & Sheldon Stone Syracuse University 03/30/2007. Motivation. This decay is an analogue of proton decay, as in SUSY one can think of a decay such as . Instead of u-coupling one can check for c-coupling and take the inverse decay as

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40 Ca( 40 Ca,2 a ) 72 Kr: microball + GS

Studies of N=Z Nuclei from Ni to Sn. 40 Ca( 40 Ca,2 a ) 72 Kr: microball + GS. Physics Goal Understanding influence of shell effects ( 68 Se, S.Fischer et al., Phys. Rev. Lett. 84 (2000) 4064) Understanding of pair correlations, specifically T=0,1, n-p pairing.

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