The SNO+ experiment: overview and status
Creators
- 1. TU Dresden, IKTP, Dresden (Germany)
Description
The SNO+ (Sudbury Neutrino Observatory plus scintillator) experiment is the follow up of the SNO experiment, replacing the heavy water volume with about 780 tons of liquid scintillator (LAB). The unique location in the deepest underground laboratory in the world, and the use of ultra-clean materials makes the detector suitable for neutrinos studies like the detection of pep and CNO solar neutrinos, geo-neutrinos originated from radioactivity in the earth, the possible observation of neutrinos from supernovae and the study of reactor oscillation. Complementing this neutrino program, SNO+ will also search for neutrinoless double beta decay. In this phase the liquid scintillator will be loaded with 0.1% of natural Neodymium allowing the study of 150Nd (5.6% abundance) neutrinoless double beta decay. A review of the general SNO+ setup, the physics goals and the current status are presented.
Additional details
Identifiers
Publishing Information
- Journal Title
- Verhandlungen der Deutschen Physikalischen Gesellschaft
- Journal Issue
- Goettingen 2012 issue
- Series
- Also available as printed version: Verhandlungen der Deutschen Physikalischen Gesellschaft v. 47(1)
- Journal Page Range
- [1 p.]
- ISSN
- 0420-0195
- CODEN
- VDPEAZ
Conference
- Title
- 2012 DPG Spring meeting with the divisions of gravitation and theory of relativity, particle physics, theoretical and mathematical fundamentals of the physics
- Original Conference Title
- DPG-Fruehjahrstagung 2012 der Fachverbaende Gravitation und Relativitaetstheorie, Teilchenphysik, Theoretische und Mathematische Grundlagen der Physik
- Dates
- 27 Feb - 2 Mar 2012
- Place
- Goettingen (Germany)
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 44093839
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BETA DETECTION; CNO CYCLE; COSMIC NEUTRINOS; COSMIC RAY DETECTION; DOPED MATERIALS; DOUBLE BETA DECAY; ELECTRON ANTINEUTRINOS; HYDROGEN BURNING; LEPTON NUMBER; LIQUID SCINTILLATION DETECTORS; LIQUID SCINTILLATORS; NEODYMIUM 150; NEODYMIUM ADDITIONS; NEUTRINO DETECTION; NEUTRINO OSCILLATION; SOLAR NEUTRINOS; SUPERNOVAE; SYMMETRY BREAKING; UNDERGROUND
- Descriptors DEC
- ALLOYS; ANTILEPTONS; ANTIMATTER; ANTINEUTRINOS; ANTIPARTICLES; BETA DECAY; BETA-MINUS DECAY; BINARY STARS; CHARGED PARTICLE DETECTION; COSMIC RADIATION; DECAY; DETECTION; ELECTRON NEUTRINOS; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; EVEN-EVEN NUCLEI; FERMIONS; INTERMEDIATE MASS NUCLEI; IONIZING RADIATIONS; ISOTOPES; LEPTONS; LEVELS; MASSLESS PARTICLES; MATERIALS; MATTER; MEASURING INSTRUMENTS; NEODYMIUM ALLOYS; NEODYMIUM ISOTOPES; NEUTRINOS; NUCLEAR DECAY; NUCLEI; PHOSPHORS; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS; RARE EARTH ADDITIONS; RARE EARTH ALLOYS; RARE EARTH NUCLEI; SCINTILLATION COUNTERS; SOLAR PARTICLES; SOLAR RADIATION; STABLE ISOTOPES; STAR BURNING; STARS; STELLAR RADIATION; VARIABLE STARS
Optional Information
- Notes
- Session: T 111.1 Mi 16:45; No further information available