SOX: search for short baseline neutrino oscillations with Borexino
Creators
- 1. Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Centre de Saclay, IRFU, 91191 Gif-sur-Yvette (France)
- 2. Physik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching (Germany)
- 3. Dipartimento di Fisica, Università degli Studi e INFN, 20133 Milano (Italy)
- 4. Chemical Engineering Department, Princeton University, Princeton, NJ 08544 (United States)
- 5. Institut für Experimentalphysik, Universität, 22761 Hamburg (Germany)
- 6. INFN Laboratori Nazionali del Gran Sasso, 67010 Assergi (Italy)
- 7. Physics Department, Virginia Polytechnic Institute and State University, Blacksburg, VA 24061 (United States)
- 8. Physics Department, Princeton University, Princeton, NJ 08544 (United States)
- 9. Dipartimento di Fisica, Università degli Studi e INFN, Genova 16146 (Italy)
- 10. Lomonosov Moscow State University Skobeltsyn Institute of Nuclear Physics, 119234 Moscow (Russian Federation)
- 11. Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822 (United States)
- 12. AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Sorbonne Paris Cité, 75205 Paris Cedex 13 (France)
- 13. Gran Sasso Science Institute (INFN), 67100 L'Aquila (Italy)
Description
The Borexino detector has convincingly shown its outstanding performances in the low energy regime through its accomplishments in the observation and study of the solar and geo neutrinos. It is then an ideal tool to perform a state of the art source-based experiment for testing the longstanding hypothesis of a fourth sterile neutrino with ∼ eV2 mass, as suggested by several anomalies accumulated over the past three decades in source, reactor, and accelerator-based experiments. The SOX project aims at successively deploying two intense radioactive sources, made of Cerium (antineutrino) and Chromium (neutrino), respectively, in a dedicated pit located beneath the detector. The existence of such an ∼ eV2 sterile neutrino would then show up as an unambiguous spatial and energy distortion in the count rate of neutrinos interacting within the active detector volume. This article reports on the latest developments about the first phase of the SOX experiment, namely CeSOX, and gives a realistic projection of CeSOX sensitivity to light sterile neutrinos in a simple (3+1) model. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/718/6/062066Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 718
- Journal Issue
- 6
- Journal Page Range
- [6 p.]
- ISSN
- 1742-6596
Conference
- Title
- 14. international conference on topics in astroparticle and underground physics
- Acronym
- TAUP 2015
- Dates
- 7-11 Sep 2015
- Place
- Torino (Italy)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49068567
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANTINEUTRINOS; BOREXINO DETECTOR; GEONEUTRINOS; MASS; NEUTRINO OSCILLATION; SENSITIVITY; SPECTROSCOPY; STERILE NEUTRINOS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATTER; MEASURING INSTRUMENTS; NEUTRINO DETECTORS; NEUTRINOS; POSTULATED PARTICLES; RADIATION DETECTORS
Optional Information
- Collaborations
- Borexino Collaboration