Cargando…
A new technique for direct investigation of dark matter
The MOSCAB experiment (Materia OSCura A Bolle) 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...
Autores principales: | , , , , , , , , , , |
---|---|
Lenguaje: | eng |
Publicado: |
2013
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.nima.2014.01.026 http://cds.cern.ch/record/1627094 |
_version_ | 1780933840271835136 |
---|---|
author | Bertoni, R. Chignoli, F. Chiesa, D. Clemenza, M. Lucchini, G. Mazza, R. Negri, P. Pullia, A. Redaelli, N. Zanotti, L. Cundy, D. |
author_facet | Bertoni, R. Chignoli, F. Chiesa, D. Clemenza, M. Lucchini, G. Mazza, R. Negri, P. Pullia, A. Redaelli, N. Zanotti, L. Cundy, D. |
author_sort | Bertoni, R. |
collection | CERN |
description | The MOSCAB experiment (Materia OSCura A Bolle) 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 | cern-1627094 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2013 |
record_format | invenio |
spelling | cern-16270942023-03-14T17:56:48Zdoi:10.1016/j.nima.2014.01.026http://cds.cern.ch/record/1627094engBertoni, R.Chignoli, F.Chiesa, D.Clemenza, M.Lucchini, G.Mazza, R.Negri, P.Pullia, A.Redaelli, N.Zanotti, L.Cundy, D.A new technique for direct investigation of dark matterAstrophysics and AstronomyThe MOSCAB experiment (Materia OSCura A Bolle) 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.The MOSCAB experiment (Materia OSCura A Bolle) 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.The MOSCAB experiment (Materia OSCura A Bolle) 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.arXiv:1311.2214oai:cds.cern.ch:16270942013-11-09 |
spellingShingle | Astrophysics and Astronomy Bertoni, R. Chignoli, F. Chiesa, D. Clemenza, M. Lucchini, G. Mazza, R. Negri, P. Pullia, A. Redaelli, N. Zanotti, L. Cundy, D. A new technique for direct investigation of dark matter |
title | A new technique for direct investigation of dark matter |
title_full | A new technique for direct investigation of dark matter |
title_fullStr | A new technique for direct investigation of dark matter |
title_full_unstemmed | A new technique for direct investigation of dark matter |
title_short | A new technique for direct investigation of dark matter |
title_sort | new technique for direct investigation of dark matter |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1016/j.nima.2014.01.026 http://cds.cern.ch/record/1627094 |
work_keys_str_mv | AT bertonir anewtechniquefordirectinvestigationofdarkmatter AT chignolif anewtechniquefordirectinvestigationofdarkmatter AT chiesad anewtechniquefordirectinvestigationofdarkmatter AT clemenzam anewtechniquefordirectinvestigationofdarkmatter AT lucchinig anewtechniquefordirectinvestigationofdarkmatter AT mazzar anewtechniquefordirectinvestigationofdarkmatter AT negrip anewtechniquefordirectinvestigationofdarkmatter AT pulliaa anewtechniquefordirectinvestigationofdarkmatter AT redaellin anewtechniquefordirectinvestigationofdarkmatter AT zanottil anewtechniquefordirectinvestigationofdarkmatter AT cundyd anewtechniquefordirectinvestigationofdarkmatter AT bertonir newtechniquefordirectinvestigationofdarkmatter AT chignolif newtechniquefordirectinvestigationofdarkmatter AT chiesad newtechniquefordirectinvestigationofdarkmatter AT clemenzam newtechniquefordirectinvestigationofdarkmatter AT lucchinig newtechniquefordirectinvestigationofdarkmatter AT mazzar newtechniquefordirectinvestigationofdarkmatter AT negrip newtechniquefordirectinvestigationofdarkmatter AT pulliaa newtechniquefordirectinvestigationofdarkmatter AT redaellin newtechniquefordirectinvestigationofdarkmatter AT zanottil newtechniquefordirectinvestigationofdarkmatter AT cundyd newtechniquefordirectinvestigationofdarkmatter |