13 results on '"Irastorza, I"'
Search Results
2. A Novel Noninvasive Method Based on Salivary Inflammatory Biomarkers for the Screening of Celiac Disease
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Sebastian-delaCruz, M., primary, Olazagoitia-Garmendia, A., additional, Huerta Madrigal, A., additional, Garcia-Etxebarria, K., additional, Mendoza, L.M., additional, Fernandez-Jimenez, N., additional, Garcia Casales, Z., additional, de la Calle Navarro, E., additional, Calvo, A.E., additional, Legarda, M., additional, Tutau, C., additional, Irastorza, I., additional, Bujanda, L., additional, Bilbao, J.R., additional, and Castellanos-Rubio, A., additional
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- 2021
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3. PP223-SUN EVALUATION OF MENUS AND FEEDING HABITS IN PRIMARY SCHOOLS OF NORTHERN SPAIN
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Irastorza, I., primary, Zulueta, B., additional, Oliver, P., additional, Garcia, Z., additional, Guerra, E., additional, and Vitoria, J.C., additional
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- 2011
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4. Gastrointestinal Complications in Liver Transplant Recipients: MITOS Study
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Herrero, J.I., primary, Benlloch, S., additional, Bernardos, A., additional, Bilbao, I., additional, Castells, L., additional, Castroagudin, J.F., additional, González, L., additional, Irastorza, I., additional, Navasa, M., additional, Otero, A., additional, Pons, J.A., additional, Rimola, A., additional, Suárez, F., additional, Casanovas, T., additional, Otero, E., additional, Rodríguez, M., additional, Serrano, T., additional, Otero, S., additional, López, I., additional, Miras, M., additional, and Prieto, M., additional
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- 2007
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5. NOSTOS experiment and new trends in rare event detection
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Giomataris, I., primary, Aune, S., additional, Colas, P., additional, Ferrer, E., additional, Irastorza, I., additional, Peyaud, B., additional, Dolbeau, J., additional, Gorodetzky, P., additional, van der Graaf, H., additional, Patzak, T., additional, Salin, P., additional, Busto, J., additional, Lepeltier, V., additional, and Vergados, I., additional
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- 2006
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6. The cern axion solar telescope (CAST): an update
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Andriamonje, S., primary, Arsov, V., additional, Aune, S., additional, Aune, T., additional, Avignone, F.T., additional, Barth, K., additional, Belov, A., additional, Beltran, B., additional, Bräuninger, H., additional, Carmona, J., additional, Cebrián, S., additional, Chesi, E., additional, Cipolla, G., additional, Collar, J., additional, Creswick, R., additional, Dafni, T., additional, Davenport, M., additional, Dedousis, S., additional, Delattre, M., additional, Delbart, A., additional, DeOliveira, R., additional, DiLella, L., additional, Eleftheriadis, C., additional, Engelhauser, J., additional, Fanourakis, G., additional, Farach, H., additional, Ferrer, E., additional, Fischer, H., additional, Formenti, F., additional, Franz, J., additional, Friedrich, P., additional, Geralis, T., additional, Giomataris, I., additional, Gninenko, S., additional, Golubev, N., additional, Hartmann, R., additional, Hasinoff, M., additional, Heinsius, F-H., additional, Hoffmann, D.H.H., additional, Irastorza, I., additional, Jacoby, J., additional, Joux, J-N., additional, Kang, D., additional, Königsmann, K., additional, Kotthaus, R., additional, Krcmar, M., additional, Kuster, M., additional, Lakic, B., additional, Lasseur, C., additional, Liolios, A., additional, Lippitsch, A., additional, Ljubicic, A., additional, Lutz, G., additional, Luzon, G., additional, Morales, A., additional, Morales, J., additional, Mutterer, M., additional, Nikolaidis, A., additional, de Solorzano, A. Ortiz, additional, Papaevangelou, T., additional, Placci, A., additional, Raffelt, G., additional, Rammos, P., additional, Robert, J.P., additional, Ruz, J., additional, Sarsa, M., additional, Schill, C., additional, Serber, W., additional, Semertzidis, Y., additional, Vieira, J., additional, Villar, J., additional, Vullierme, B., additional, Walckiers, L., additional, and Zioutas, K., additional
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- 2005
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7. Using wavelets to reject background in dark matter experiments
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Irastorza, I, primary
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- 2003
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8. Present status of IGEX dark matter search at Canfranc Underground Laboratory
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Irastorza, I, primary
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- 2002
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9. An update on the Axion Helioscopes front: current activities at CAST and the IAXO project
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Joachim Jacoby, J. I. Collar, H. Ten Kate, Fritz Caspers, Julia Vogel, J. Kaminski, H. Silva, Giovanni Cantatore, Benito Gimeno, S. C. Yildiz, M. Betz, Alexey Dudarev, Georg G. Raffelt, A. Belov, F.J. Iguaz, Rainer Kotthaus, Javier Redondo, F. Haug, K. Barth, G. Luzón, Klaus Kurt Desch, C. Eleftheriadis, S. Caspi, P. Brax, Georgios Fanourakis, W. C. Wester, Hector Gomez, J. M. Laurent, N. Breijnholt, I. Dratchnev, Toyokazu Sekiguchi, S. Neff, L. Stewart, Joerg Jaeckel, Amanda Weltman, Marin Karuza, C. Krieger, Pierre Sikivie, A. Tomás, S. Aune, C. Nones, Heinrich Bräuninger, Serkant Ali Cetin, M. Rosu, I. G. Irastorza, J. M. Carmona, Babette Döbrich, Krešimir Jakovčić, Steffen Hauf, Takashi Hiramatsu, Biljana Lakić, Milica Krčmar, Evangelos Gazis, M. Davenport, Dieter H. H. Hoffmann, T. Papaevangelou, J.A. Villar, A. V. Derbin, Ante Ljubičić, Dieter Horns, S. N. Gninenko, A. Diago, I. Ortega, S. Matsuki, E. Gruber, Sergey Troitsky, T. Dafni, J. G. Garza, I. Savvidis, Andreas Ringwald, A. Lindner, Jordi Isern, M. Arik, Javier Galan, Ken'ichi Saikawa, E. Georgiopoulou, T. Guthörl, Eduardo Guendelman, Adriane De Assis Lawisch Rodriguez, I. Shilon, D. Chelouche, S. Russenschuck, Kenichi Imai, V. N. Muratova, P. Vedrine, F.E. Christensen, T. O. Niinikoski, E. Ferrer-Ribas, F. T. Avignone, Charles J. Hailey, M. D. Hasinoff, Peter Friedrich, M. J. Pivovaroff, Konstantin Zioutas, Sami K. Solanki, Louis Walckiers, H. Riege, Pierre Brun, Konstantinos Kousouris, Markus Kuster, A. Dael, T. Geralis, Gianpaolo Carosi, J. A. Garcia, A. Gardikiotis, Yannis K. Semertzidis, Eric Armengaud, Raimo Hartmann, Theodoros Vafeiadis, J. Ruz, K. Königsmann, Masahiro Kawasaki, D. González-Díaz, I. Giomataris, K. van Bibber, Olivier Limousin, A.C. Jakobsen, A. Liolios, Dafni, T, Arik, M., Armengaud, E., Aune, S., Avignone, F. T., Barth, K., Belov, A., Betz, M., Bräuninger, H., Brax, P., Breijnholt, N., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Collar, J. I., Dael, A., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Georgiopoulou, E., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Gruber, E., Guendelman, E., Guthörl, T., Hailey, C. J., Hartmann, R., Hauf, S., Haug, F., Hasinoff, M. D., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jacoby, J., Jaeckel, J., Jakobsen, A. C., Jakovcić, K., Kaminski, J., Kawasaki, M., Karuza, M., Königsmann, K., Kotthaus, R., Krcmar, M., Kousouris, K., Krieger, C., Kuster, M., Lakić, B., Laurent, J. M., Limousin, O., Lindner, A., Liolios, A., Ljubicić, A., Luzón, G., Matsuki, S., Muratova, V. N., Neff, S., Niinikoski, T., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Riege, H., Ringwald, A., Rodríguez, A., Rosu, M., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Solanki, S. K., Stewart, L., ten Kate, H. H. J., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K., Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Arık, Metin, and Yıldız, Süleyman Cenk
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X-Ray Focusing Devices ,X-ray detector ,Particle physics ,Nuclear and High Energy Physics ,X-ray focusing device ,Axions ,Dark matter ,Magnet Development ,Micromegas detector ,axions ,dark matter ,x-ray ,detectors ,micromegas detectors ,x-ray focusing devices ,magnet development ,CAST ,IAXO ,01 natural sciences ,Axion ,Primary (astronomy) ,Observatory ,0103 physical sciences ,Dark Matter ,X-Ray Detectors ,010306 general physics ,Physics ,Helioscope ,Micromegas Detectors ,010308 nuclear & particles physics ,Magnet development ,Micromegas detectors ,X-ray detectors ,X-ray focusing devices ,Orders of magnitude (time) ,Experimental methods ,CERN Axion Solar Telescope - Abstract
Çetin, Serkant Ali (Dogus Author) -- Arık, Metin (Dogus Author) -- Yıldız, Süleyman Cenk (Dogus Author) Although they have not yet been detected, axions and axion-like particles (ALPs) continue to maintain the interest (even increasingly so) of the rare-event searches community as viable candidates for the Dark Matter of the Universe but also as a solution for several other puzzles of astrophysics. Their property of coupling to photons has inspired different experimental methods for their detection, one of which is the helioscope technique. The CERN Axion Solar Telescope (CAST) is the most sensitive helioscope built up to date and has recently published part of the latest data taken with the magnet bores gradually filled with He-3, probing the mass range up to 1.17 eV. The International AXion Observatory (IAXO) is being proposed as a facility where different axion studies can be performed, with the primary goal to study axions coming from the Sun. Designed to maximize sensitivity, it will improve the levels reached by CAST by almost 5 orders of magnitude in signal detection, that is more than one order of magnitude in terms of gay. Here we will summarize the most important aspects of the helioscopes, and focus mainly on IAXO, based on the recent papers [1, 2].
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- 2016
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10. The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)
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Javier Redondo, Biljana Lakić, Eduardo Guendelman, K. van Bibber, A. Diago, S. Matsuki, Hector Gomez, Marin Karuza, C. Eleftheriadis, Olivier Limousin, H. H. J. ten Kate, Eric Armengaud, T. Dafni, Finn Erland Christensen, I. Ortega, Pierre Sikivie, Anders Clemen Jakobsen, F.J. Iguaz, Charles J. Hailey, Diego González-Díaz, Theodoros Vafeiadis, Milica Krčmar, Takashi Hiramatsu, V. N. Muratova, Dieter H. H. Hoffmann, J.A. Villar, S. C. Yildiz, Klaus Kurt Desch, I. Shilon, B. Döbrich, Javier Galan, J. G. Garza, Pierre Brun, A. Dael, S. Gninenko, F. T. Avignone, A. Tomás, W. C. Wester, C. Krieger, I. G. Irastorza, Masahiro Kawasaki, A. Lindner, A. Dudarev, Andreas Ringwald, Michael J. Pivovaroff, M. Betz, A. V. Derbin, P. Brax, C. Nones, D. Chelouche, Ioannis Giomataris, I. Savvidis, Yannis K. Semertzidis, S. Russenschuck, Kenichi Imai, Konstantin Zioutas, Theodoros Geralis, Serkant Ali Cetin, Giovanni Cantatore, Julia Vogel, Jordi Isern, H. Silva, E. Ferrer-Ribas, Ken'ichi Saikawa, G. Luzón, Dieter Horns, P. Vedrine, G. Fanourakis, Toyokazu Sekiguchi, Fritz Caspers, J. A. Garcia, Joerg Jaeckel, Amanda Weltman, J. Ruz, M. Davenport, J. Kaminski, L. Walckiers, Krešimir Jakovčić, Gianpaolo Carosi, A. Liolios, B. Gimeno, Georg G. Raffelt, T. Papaevangelou, J. M. Carmona, S. Caspi, Konstantinos Kousouris, I. Dratchnev, Sergey Troitsky, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Vogel, J. K., Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., Jakovčić, K., Kaminski, J., Kawasaki, M., Karuza, M., Krčmar, M., Kousouris, K., Krieger, C., Lakić, B., Limousin, O., Lindner, A., Liolios, A., Luzón, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., ten Kate, H., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., and Zioutas, K.
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QCD axion ,Particle physics ,Physics::Instrumentation and Detectors ,Dark matter ,Physics and Astronomy(all) ,01 natural sciences ,7. Clean energy ,magnetic helioscope ,High Energy Physics::Theory ,QCD axions ,Astroparticle Physics ,Axion ,Observatory ,0103 physical sciences ,dark matter ,Dark Matter ,ddc:530 ,Detectors and Experimental Techniques ,010306 general physics ,Astroparticle physics ,Physics ,Helioscope ,010308 nuclear & particles physics ,Axion Dark Matter Experiment ,High Energy Physics::Phenomenology ,Strong CP problem ,IAXO ,Strong CP Problem ,ALP ,CERN Axion Solar Telescope ,Particle Physics - Experiment ,Helioscopes - Abstract
Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best (3rd generation) axion helioscope, the CERN Axion Solar Telescope (CAST), of about 5 orders of magnitude in signal strength, corresponding to a factor ∼ 20 in the axion photon coupling. IAXO's sensitivity relies on the construction of a large superconducting 8-coil toroidal magnet of 20 m length optimized for axion research. Each of the eight 60 cm diameter magnet bores is equipped with x-ray optics focusing the signal photons into ∼ 0.2 cm2 spots that are imaged by very low background x-ray detectors. The magnet will be built into a structure with elevation and azimuth drives that will allow solar tracking for 12 hours each day. This contribution is a summary of our papers [1-3] and we refer to these for further details.
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- 2015
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11. Physics potential and prospects for the CUORICINO and CUORE experiments
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C. Rosenfeld, P. Gorla, Eugene E. Haller, Carlos Pobes, G. Ventura, A. Nucciotti, Marco Barucci, C. Brofferio, Giorgio Frossati, Monica Sisti, Alan R. Smith, L. Carbone, H. A. Farach, A. Morales, R. J. Creswick, Ettore Fiorini, A. Giuliani, Silvia Capelli, V. Palmieri, S. Pirro, I. G. Irastorza, J. Beeman, Eric B. Norman, S. Cebrián, C. Bucci, Stefano Scopel, F. T. Avignone, Oliviero Cremonesi, M. Balata, M. Vanzini, Ezio Previtali, G. Pessina, A. de Ward, M. Pedretti, C. Arnaboldi, R.J. McDonald, M. Pavan, Arnaboldi, C, Avignone, F, Beeman, J, Barucci, M, Balata, M, Brofferio, C, Bucci, C, Cebrian, S, Creswick, R, Capelli, S, Carbone, L, Cremonesi, O, de Ward, A, Fiorini, E, Farach, H, Frossati, G, Giuliani, A, Gorla, P, Haller, E, Irastorza, I, Mcdonald, R, Morales, A, Norman, E, Nucciotti, A, Pedretti, M, Pobes, C, Palmieri, V, Pavan, M, Pessina, G, Pirro, S, Previtali, E, Rosenfeld, C, Scopel, S, Smith, A, Sisti, M, Ventura, G, and Vanzini, M
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Physics ,Particle physics ,Physics::Instrumentation and Detectors ,Dark matter ,Bolometer ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Astronomy and Astrophysics ,Cryogenics ,neutrinoless double beta decay ,dark matter ,High Energy Physics - Experiment ,law.invention ,Nuclear physics ,High Energy Physics - Experiment (hep-ex) ,CUORE ,bolometer ,WIMP ,law ,Observatory ,Double beta decay ,High Energy Physics::Experiment ,Nuclear Experiment ,Axion ,FIS/04 - FISICA NUCLEARE E SUBNUCLEARE - Abstract
The CUORE experiment projects to construct and operate an array of 1000 cryogenic thermal detectors of TeO2, of a mass of 760 g each, to investigate rare events physics, in particular, double beta decay and non baryonic particle dark matter. A first step towards CUORE is CUORICINO, an array of 62 bolometers, currently being installed in the Gran Sasso Laboratory. In this paper we report the physics potential of both stages of the experiment regarding neutrinoless double beta decay of 130Te, WIMP searches and solar axions., Comment: 36 pages, 5 figures. Submitted to Astrop. Phys
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- 2003
12. CUORE: low-temperature techniques for neutrino physics
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V. Palmieri, M. Sisti, Eric B. Norman, I. G. Irastorza, M. Pedretti, S. Cebrián, E. E. Haller, Oliviero Cremonesi, G. Pessina, M. Vanzini, Marco Barucci, D Giugni, Jeffrey W. Beeman, C. Arnaboldi, C. Bucci, M. Balata, A. Morales, C. Brofferio, Edoardo Pasca, R. J. Creswick, P. Negri, Alan R. Smith, A. Nucciotti, P. Gorla, F. T. Avignone, Stefano Pirro, A. de Waard, Silvia Capelli, E. Fiorini, L. Zanotti, R.J. McDonald, H. A. Farach, Ezio Previtali, A. Giuliani, G. Ventura, M. Pavan, Giorgio Frossati, L. Carbone, Giuliani, A, Arnaboldi, C, Avignone, F, Balata, M, Barucci, M, Beeman, J, Brofferio, C, Bucci, C, Capelli, S, Carbone, L, Cebrian, S, Cremonesi, O, Creswick, R, Farach, H, Fiorini, E, Frossati, G, Giugni, D, Gorla, P, Haller, E, Irastorza, I, Mcdonald, R, Morales, A, Negri, P, Norman, E, Nucciotti, A, Palmieri, V, Pasca, E, Pavan, M, Pedretti, M, Pessina, G, Pirro, S, Previtali, E, Sisti, M, Smith, A, Vanzini, M, Ventura, G, De Waard, A, and Zanotti, L
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Physics ,Particle physics ,Physics::Instrumentation and Detectors ,Solar neutrino ,Bolometric detector ,Solar neutrino problem ,Condensed Matter Physics ,Electronic, Optical and Magnetic Materials ,Neutrino physics ,Nuclear physics ,CUORE ,Low-temperature calorimeter ,Neutrino detector ,Double beta decay ,Measurements of neutrino speed ,High Energy Physics::Experiment ,Electrical and Electronic Engineering ,Neutrino ,Neutrino oscillation ,FIS/04 - FISICA NUCLEARE E SUBNUCLEARE - Abstract
Neutrino physics represents today a hot topic in elementary particle physics, due to the observations of flavour oscillations both in the atmospheric and in the solar sector. This proves the existence of finite neutrino masses. In order to fix their absolute values, sensitive experiments on Neutrinoless Double Beta Decay (a rare nuclear process) must be carried on. The experiment here described, named Cryogenics Underground Observatory for Rare Events (CUORE), can extend the neutrino mass sensitivity down to 30 meV . CUORE will consist of a large, closely packed, high-granularity array of 1000 tellurite (TeO2) low-temperature calorimeters, operated at 10 mK and with a total mass of 800 kg . The final structure of the detector and the preliminary tests are presented and discussed.
- Published
- 2003
13. First results from the Cuoricino experiment
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A. Morales, H. A. Farach, F. T. Avignone, Ettore Fiorini, J. Beeman, Carlos Pobes, S. Pirro, C. Brofferio, R. J. McDonald, G. Ventura, S. Cebrián, Lara Risegari, Alan R. Smith, C. Rosenfeld, L. Carbone, M. Pedretti, P. Gorla, V. Palmieri, Eugene E. Haller, A. Giuliani, Edoardo Pasca, Giorgio Frossati, Eric B. Norman, L. Torres, E. Olivieri, A. de Waard, C. Bucci, Marco Barucci, D. R. Artusa, G. Pessina, Monica Sisti, Oliviero Cremonesi, Simone Capelli, M. Pyle, A. Nucciotti, I. C. Bandac, M. Pavan, Ezio Previtali, R. J. Creswick, M. Balata, C. Arnaboldi, I. G. Irastorza, A. Fascilla, Bucci, C, Arnaboldi, C, Artusa, D, Avignone, F, Balata, M, Bandac, I, Barucci, M, Brofferio, C, Beeman, J, Capelli, S, Carbone, L, Cebrian, S, Cremonesi, O, Creswick, R, Farach, H, Fascilla, A, Fiorini, E, Frossati, G, Giuliani, A, Gorla, P, Haller, E, Irastorza, I, Mcdonald, R, Morales, A, Norman, E, Nucciotti, A, Olivieri, E, Palmieri, V, Pasca, E, Pavan, M, Pedretti, M, Pessina, G, Pirro, S, Pobes, C, Previtali, E, Pyle, M, Risegari, L, Rosenfeld, C, Sisti, M, Smith, A, Torres, L, Ventura, G, and de Waard, A
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Physics ,Nuclear and High Energy Physics ,Double beta decay ,Neutrino mass ,Bolometer ,Detector ,law.invention ,Nuclear physics ,CUORE ,Observatory ,law ,Neutrino ,Instrumentation ,Tower ,Radioactive decay - Abstract
At the end of 2001 the Milano Double Beta Decay (MI-DBD) experiment on double beta decay of 130Te has been completed. The project Cryogenic Underground Observatory for Rare Events (CUORE), proposed as a natural extension of MI-DBD, will be a tightly packed array of 1000 TeO2 bolometers, each being a cube 5 cm on a side with a mass of 790 g. The array will consists of 25 vertical towers, arranged in a square of 5 towers by 5 towers, each containing 10 layers of 4 crystals. A single CUORE tower has been constructed as a smaller scale experiment called CUORICINO. The technical feasibility of CUORE is now being tested in CUORICINO, running since few weeks. The CUORICINO experiment consists of 44 TeO2 detectors 5×5×5 cm3 and 18 TeO2 detectors 3×3×6 cm3 for a total mass of approximately 41 kg. An analysis of the detector performances is presented together with the new limit obtained on neutrinoless double beta decay of 130Te.
- Published
- 2004
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