Large underground, liquid based detectors for astro-particle physics in Europe:: scientific case and prospects

被引：116

作者：

Autiero, D. ^{[1
]}

Aysto, J. ^{[2
]}

Badertscher, A. ^{[3
]}

Bezrukov, L.

Bouchez, J. ^{[4
,5
,6
]}

Bueno, A. ^{[7
,8
]}

Busto, J. ^{[9
,10
]}

Campagne, J-E ^{[11
]}

Cavata, C. H. ^{[5
]}

Chaussard, L. ^{[1
]}

de Bellefon, A. ^{[12
]}

Declais, Y. ^{[1
]}

Dumarchez, J. ^{[13
,14
,15
]}

Ebert, J. ^{[16
]}

Enqvist, T. ^{[17
]}

Ereditato, A. ^{[18
]}

von Feilitzsch, F. ^{[19
]}

Perez, P. Fileviez ^{[20
]}

Goeger-Neff, M. ^{[21
]}

Gninenko, S. ^{[4
]}

Gruber, W. ^{[3
]}

Hagner, C. ^{[16
]}

Hess, M. ^{[18
]}

Hochmuth, K. A. ^{[21
]}

Kisiel, J. ^{[22
]}

Knecht, L. ^{[3
]}

Kreslo, I. ^{[18
]}

Kudryavtsev, V. A. ^{[23
]}

Kuusiniemi, P. ^{[17
]}

Lachenmaier, T. ^{[19
]}

Laffranchi, M. ^{[3
]}

Lefievre, B. ^{[12
]}

Lightfoot, P. K. ^{[23
]}

Lindner, M. ^{[24
]}

Maalampi, J. ^{[2
]}

Maltoni, M. ^{[25
,26
]}

Marchionni, A. ^{[3
]}

Undagoitia, T. Marrodan ^{[19
]}

Marteau, J. ^{[1
]}

Meregaglia, A. ^{[3
]}

Messina, M. ^{[18
]}

Mezzetto, M. ^{[27
]}

Mirizzi, A. ^{[21
,28
,29
]}

Mosca, L. ^{[5
]}

Moser, U. ^{[18
]}

Mueller, A. ^{[3
]}

Natterer, G. ^{[3
]}

Oberauer, L. ^{[19
]}

Otiougova, P. ^{[3
]}

Patzak, T. ^{[12
]}

机构：

[1] Univ Lyon 1, IPNL, CNRS IN2P3, F-69622 Villeurbanne, France

[2] Univ Jyvaskyla, Dept Phys, SF-40351 Jyvaskyla, Finland

[3] ETHZ, Inst Teilchenphys, Zurich, Switzerland

[4] Russian Acad Sci, Inst Nucl Res, Moscow, Russia

[5] CEA Saclay, F-91191 Gif Sur Yvette, France

[6] APC Paris, Paris, France

[7] Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain

[8] Univ Granada, CAFPE, E-18071 Granada, Spain

[9] IN2P3 CNRS, CPPM, Marseille, France

[10] Univ Aix Marseille 2, F-13284 Marseille 07, France

[11] Univ Paris Sud, LAL, IN2P3 CNRS, Orsay, France

[12] Univ Paris 07, CEA, Observ Paris, APC,CNRS, Paris, France

[13] IN2P3 CNRS, LPNHE, Paris, France

[14] Univ Paris 06, Paris, France

[15] Univ Paris 07, Paris, France

[16] Univ Hamburg, Inst Expt Phys, Hamburg, Germany

[17] Univ Oulu, CUPP, Oulu, Finland

[18] Univ Bern, Lab Hochenergie Phys, Bern, Switzerland

[19] Tech Univ Munich, Phys Dept E15, D-8046 Garching, Germany

[20] Ctr Fis Teor Particulars, Inst Super Tecn, Dept Fis, Lisbon, Portugal

[21] Werner Heisenberg Inst Phys, Max Planck Inst Phys, Munich, Germany

[22] Silesian Univ, Inst Phys, PL-40007 Katowice, Poland

[23] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England

[24] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[25] Univ Autonoma Madrid, Fac Ciencias C 11, Dept Fis Teor, Madrid, Spain

[26] Univ Autonoma Madrid, Fac Ciencias C 11, Inst Fis Teor, Madrid, Spain

[27] INFN Sez Padova, Padua, Italy

[28] Univ Bari, INFN Sez Bari, Bari, Italy

[29] Univ Bari, Dipartimento Fis, Bari, Italy

[30] Soltan Inst Nucl Studies, PL-00681 Warsaw, Poland

[31] Univ Helsinki, Dept Phys Sci, FIN-00014 Helsinki, Finland

[32] CERN, Div Theory, Dept Phys, Geneva, Switzerland

[33] Univ Wroclaw, Inst Theoret Phys, PL-50138 Wroclaw, Poland

[34] H Niewodniczanski Inst Nucl Phys, Krakow, Poland

[35] Univ Paris Sud 11, IPNO, Grp Phys Theorique, Orsay, France

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2007年 / 11期

关键词：

solar and atmospheric neutrinos; supernova neutrinos; neutrino detectors; neutrino properties;

D O I：

10.1088/1475-7516/2007/11/011

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 apparatuses employ three different and, to some extent, complementary detection techniques: GLACIER (liquid argon TPC), LENA (liquid scintillator) and MEMPHYS (water Cherenkov), 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 neutrinos and geo-neutrinos and to the possible use of these detectors in future high intensity neutrino beams.

引用

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