'Gran sasso' diaporamas de présentation

Recent results from the OPERA experiment

Recent results from the OPERA experiment. Maximiliano Sioli (Bologna University and INFN) on behalf of the OPERA Collaboration SLAC Experimental Seminar - June 22, 2010. The OPERA Collaboration. Belgium IIHE Brussels Bulgaria Sofia Croatia IRB Zagreb

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CNGS Project: primary beam

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0 ?- Double Beta Decay Search: Status and Perspectives

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Superluminal Neutrinos?

Susan Cartwright Department of Physics and Astronomy. Introduction The OPERA result SN 1987A Interpretations. Superluminal Neutrinos?. Introduction. The speed of light, c , plays a fundamental role in relativity and Lorentz transformations

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Directional Dark Matter Search With Ultra Fine Grain Nuclear Emulsion

Directional Dark Matter Search With Ultra Fine Grain Nuclear Emulsion. Takashi Asada Flab, Nagoya University JSPS Research Fellow. Index. Dark Matter About d ark matter Dark matter search experiments Emulsio n R&D New production method Sensitivity control Readout R&D

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Recent progress of direct dark matter detection

Recent progress of direct dark matter detection. S. Moriyama Institute for Cosmic Ray Research, University of Tokyo Oct. 8 th , 2011 @ FPUA2011, Okayama, Japan. Principle of direct detection in Lab. Dark matter hit detectors in Lab. Why interaction expected?

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Lino Miramonti Milano University and INFN sez. Milano

European underground laboratories: An overview. Lino Miramonti Milano University and INFN sez. Milano. LRT 2004 - Topical Workshop in Low Radioactivity Techniques (Sudbury, Canada ) December 12-14, 2004. Boulby Mine. Frejus. Canfranc. Gran Sasso.

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Astroparticle Physics

Astroparticle Physics. The 2011 ASPERA Roadmap. Christian Spiering, DESY VLVNT-2011, Erlangen, October 14, 2011. ApPEC/ASPERA Roadmap process. Detailed Description Glossy Paper Actual Status &

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Status of the COBRA Experiment

Status of the COBRA Experiment. K. Zuber, TU Dresden. Contents. General introduction Low background issues Pixel activities Summary and Outlook. COBRA. Use large amount of CdZnTe Semiconductor Detectors. large array of CdZnTe detectors.

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The OPERA long baseline neutrino experiment : status and first results.

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Integration of the Experimental Facility in West Area & CNGS

Integration of the Experimental Facility in West Area & CNGS. With input & slides from D. Brethoux , V. Clerc , E. Gschwendtner , J. Osbourne. Outline. General layout: Information available & missing West Area Guided tour Integration first proposal Issues CNGS Guided tour

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Double Beta experiment using nuclear emulsions?

Double Beta experiment using nuclear emulsions?. Marcos Dracos IPHC/IN2P3, Strasbourg. Double Beta Decay. Nuclear matrix element. Phase space factor. -1. T 1/2 = F(Q bb ,Z) |M| 2 <m n > 2. 5. ?. Effective mass:

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Position sensitive CZT detectors for the COBRA neutrinoless double beta decay project

Position sensitive CZT detectors for the COBRA neutrinoless double beta decay project. Brian Fulton University of York. Neutrinoless double beta decay The COBRA project CZT detector development. NEUTRINOLESS DOUBLE BETA DECAY.

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Geoneutrinos in Borexino

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GERDA double beta decay experiment

GERDA double beta decay experiment. L. Pandola INFN, Gran Sasso National Laboratories for the GERDA Collaboration. Neutrino Satellite Meeting, Santa Fe, October 29 th 2005.

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SEARCH FOR NUCLEARITES USING TLS DETECTOR AT SEA LEVEL

SEARCH FOR NUCLEARITES USING TLS DETECTOR AT SEA LEVEL T.Wada [1], Y.Akitsu [1], K.Iwata [6], S.Lan [1], M.Nakagawa [4], T.Nakatsuka [2], K. Okei [1], O.Saavedra [7], N.Takahashi [5], S.Tsuji [3], J.Ryou [1], I.Yamamoto [4], Y. Yamashita [1]

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27 April 2012 EGU General Assembly 2012

Introducing VESPA-22: a ground-based microwave spectrometer for measuring middle atmospheric water vapour at polar latitudes. Pietro Paolo Bertagnolio , Giovanni Muscari, Irene Fiorucci and Massimo Mari. 27 April 2012 EGU General Assembly 2012.

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GERDA, the GERmanium Detector Array for the search of neutrinoless bb decay in 76 Ge

GERDA, the GERmanium Detector Array for the search of neutrinoless bb decay in 76 Ge. L. Pandola INFN, Gran Sasso National Laboratories for the GERDA Collaboration. PANIC Conference, Santa Fe, NM, October 24 th 2005. D L = 2 process. 0 ???: (A,Z) ? (A,Z+2) + 2e -. p.

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Congresso del Dipartimento di Fisica Highlights in Physics 2005

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CTF and low background facility at Gran Sasso

A. Ianni a , M. Laubenstein a and Y. Suvorov a a INFN, Gran Sasso Laboratory, Assergi (AQ), Italy. CTF: 4-ton liquid scintillator. Spectrum of prompt events in the scintillator of CTF. CTF and low background facility at Gran Sasso. 204 days of livetime. Whole 4-ton mass.

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