Main Page: Difference between revisions
Line 17: | Line 17: | ||
*[[Single-Phase LAr Option]] | *[[Single-Phase LAr Option]] | ||
*[[Neutrino Induced Neutron Detectors]] | *[[Neutrino Induced Neutron Detectors]] | ||
*[[MARS Detector]] | |||
*[[Backgrounds]] | *[[Backgrounds]] | ||
*[[SNS monitoring and EPICS slow controls]] | *[[SNS monitoring and EPICS slow controls]] |
Revision as of 15:39, 10 June 2017
The COHERENT collaboration aims to measure CEvNS (Coherent Elastic Neutrino-Nucleus Scattering) using the high-quality pion-decay-at-rest neutrino source at the Spallation Neutron Source in Oak Ridge, Tennessee. The SNS provides an intense flux of neutrinos in the few tens-of-MeV range, with a sharply-pulsed timing structure that is beneficial for background rejection. The CEvNS process is cleanly predicted in the Standard Model and its measurement provides a Standard Model test; furthermore, the process is involved in supernova explosion processes and supernova neutrino detection. It also represents a background floor for dark matter direct detection. In the long term, precision measurement of CEvNS will address questions of nuclear structure. We aim to deploy multiple detector technologies in a phased approach.
If you reached this page accidentally, you can find the Public COHERENT page here
Internal Workgroup Pages
- CsI(Na) Subsystem
- HPGe PPC Subsystem
- 2-Phase LXe Subsystem
- NaI(Tl) Option
- Single-Phase LAr Option
- Neutrino Induced Neutron Detectors
- MARS Detector
- Backgrounds
- SNS monitoring and EPICS slow controls
- Data analysis
- Neutrino source simulation
- Neutrino Alley Operations
The Collaboration
- Public Presentations: public page
- Collaboration Documents: internal
- Meetings: internal
- Public_Presentations: internal
- Official Plots: Internal
Information for Collaborators
Other
Obsolete Connections
The old WIKI can still be found at http://csisns.phy.duke.edu/