A novel method for direct investigation of dark matter

The Materia OSCura A Bolle (MOSCAB) experiment uses a new technique for Dark Matter search. The Geyser technique is applied to the construction of a prototype detector with a mass of 0.5 kg and the encouraging results are reported here; an accent is placed on a big detector of 40 kg in construction...

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Detalles Bibliográficos
Autores principales: Bertoni, R, Chignoli, F, Chiesa, D, Clemenza, M, Ghezzi, A, Lucchini, G, Mazza, R, Negri, P, Pozzi, S, Pullia, A, Redaelli, N, Zanotti, L, Cundy, D
Lenguaje:eng
Publicado: 2014
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1142/S0217751X14430052
http://cds.cern.ch/record/2135824
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author Bertoni, R
Chignoli, F
Chiesa, D
Clemenza, M
Ghezzi, A
Lucchini, G
Mazza, R
Negri, P
Pozzi, S
Pullia, A
Redaelli, N
Zanotti, L
Cundy, D
author_facet Bertoni, R
Chignoli, F
Chiesa, D
Clemenza, M
Ghezzi, A
Lucchini, G
Mazza, R
Negri, P
Pozzi, S
Pullia, A
Redaelli, N
Zanotti, L
Cundy, D
author_sort Bertoni, R
collection CERN
description The Materia OSCura A Bolle (MOSCAB) experiment uses a new technique for Dark Matter search. The Geyser technique is applied to the construction of a prototype detector with a mass of 0.5 kg and the encouraging results are reported here; an accent is placed on a big detector of 40 kg in construction at the Milano Bicocca University and INFN.
id oai-inspirehep.net-1309748
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
record_format invenio
spelling oai-inspirehep.net-13097482019-09-30T06:29:59Zdoi:10.1142/S0217751X14430052http://cds.cern.ch/record/2135824engBertoni, RChignoli, FChiesa, DClemenza, MGhezzi, ALucchini, GMazza, RNegri, PPozzi, SPullia, ARedaelli, NZanotti, LCundy, DA novel method for direct investigation of dark matterAstrophysics and AstronomyThe Materia OSCura A Bolle (MOSCAB) experiment uses a new technique for Dark Matter search. The Geyser technique is applied to the construction of a prototype detector with a mass of 0.5 kg and the encouraging results are reported here; an accent is placed on a big detector of 40 kg in construction at the Milano Bicocca University and INFN.oai:inspirehep.net:13097482014
spellingShingle Astrophysics and Astronomy
Bertoni, R
Chignoli, F
Chiesa, D
Clemenza, M
Ghezzi, A
Lucchini, G
Mazza, R
Negri, P
Pozzi, S
Pullia, A
Redaelli, N
Zanotti, L
Cundy, D
A novel method for direct investigation of dark matter
title A novel method for direct investigation of dark matter
title_full A novel method for direct investigation of dark matter
title_fullStr A novel method for direct investigation of dark matter
title_full_unstemmed A novel method for direct investigation of dark matter
title_short A novel method for direct investigation of dark matter
title_sort novel method for direct investigation of dark matter
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1142/S0217751X14430052
http://cds.cern.ch/record/2135824
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