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Paper: 0705.0116

From: Campagne Jean-Eric <campagne@lal.in2p3.fr>



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arXiv:0705.0116

From: Campagne Jean-Eric <campagne@lal.in2p3.fr>

Date: Tue, 1 May 2007 14:45:11 GMT   (804kb)



Title: Large underground, liquid based detectors for astro-particle physics in

  Europe: scientific case and prospects

Authors: J. Aysto, A. Badertscher, L. Bezrukov, J. Bouchez, A. Bueno, J. Busto,

  J.-E. Campagne, Ch. Cavata, A. de Bellefon, J. Dumarchez, J. Ebert, T.

  Enqvist, A. Ereditato, F. von Feilitzsch, P. Fileviez Perez, M. Goger-Neff,

  S. Gninenko, W. Gruber, C. Hagner, M. Hess, K. A. Hochmuth, J. Kisiel, L.

  Knecht, I. Kreslo, V. A. Kudryavtsev, P. Kuusiniemi, T. Lachenmaier, M.

  Laffranchi, B. Lefievre, P. K. Lightfoot, M. Lindner, J. Maalampi, M.

  Maltoni, A. Marchionni, T. Marrodan Undagoitia, A. Meregaglia, M. Messina, M.

  Mezzetto, A. Mirizzi, L. Mosca, U. Moser, A. Muller, G. Natterer, L.

  Oberauer, P. Otiougova, T. Patzak, J. Peltoniemi, W. Potzel, C. Pistillo, G.

  G. Raffelt, E. Rondio, M. Roos, B. Rossi, A. Rubbia, N. Savvinov, T. Schwetz,

  J. Sobczyk, N. J. C. Spooner, D. Stefan, A. Tonazzo, W. Trzaska, J. Ulbricht,

  C. Volpe, J. Winter, M. Wurm, A. Zalewska, R. Zimmermann

Categories: hep-ph

\\

  This document reports on a series of experimental and theoretical studies

conducted to assess the astro-particle physics potential of three future

large-scale particle detectors proposed in Europe as next generation

underground observatories. The proposed apparatus employ three different and,

to some extent, complementary detection techniques: GLACIER (liquid Argon TPC),

LENA (liquid scintillator) and MEMPHYS (\WC), based on the use of large mass of

liquids as active detection media. The results of these studies are presented

along with a critical discussion of the performance attainable by the three

proposed approaches coupled to existing or planned underground laboratories, in

relation to open and outstanding physics issues such as the search for matter

instability, the detection of astrophysical- and geo-neutrinos and to the

possible use of these detectors in future high-intensity neutrino beams.

\\