Solar neutrino detectors as sterile neutrino hunters
Author(s): Pallavicini, Marco; Collaboration, Borexino-SOX; Benziger, Jay B.
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Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Pallavicini, Marco | - |
dc.contributor.author | Collaboration, Borexino-SOX | - |
dc.contributor.author | Benziger, Jay B. | - |
dc.date.accessioned | 2021-10-08T19:57:38Z | - |
dc.date.available | 2021-10-08T19:57:38Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.citation | Pallavicini, Marco, Collaboration, Borexino-SOX. (2017). Solar neutrino detectors as sterile neutrino hunters. XXVII INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS (NEUTRINO2016), 888 (10.1088/1742-6596/888/1/012018 | en_US |
dc.identifier.issn | 1742-6588 | - |
dc.identifier.uri | http://arks.princeton.edu/ark:/88435/pr1gs08 | - |
dc.description.abstract | The large size and the very low radioactive background of solar neutrino detectors such as Borexino at the Gran Sasso Laboratory in Italy offer a unique opportunity to probe the existence of neutrino oscillations into new sterile components by means of carefully designed and well calibrated anti-neutrino and neutrino artificial sources. In this paper we briefly summarise the key elements of the SOX experiment, a program for the search of sterile neutrinos (and other short distance effects) by means of a (144) Ce- Pr-144 anti-neutrino source and, possibly in the medium term future, with a Cr-51 neutrino source. | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartof | XXVII INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS (NEUTRINO2016) | en_US |
dc.rights | Final published version. Article is made available in OAR by the publisher's permission or policy. | en_US |
dc.title | Solar neutrino detectors as sterile neutrino hunters | en_US |
dc.type | Journal Article | en_US |
dc.identifier.doi | doi:10.1088/1742-6596/888/1/012018 | - |
pu.type.symplectic | http://www.symplectic.co.uk/publications/atom-terms/1.0/conference-proceeding | en_US |
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Pallavicini_2017_J._Phys. _Conf._Ser._888_012018.pdf | 1.17 MB | Adobe PDF | View/Download |
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