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<img src="https://coherent.phy.duke.edu/MainPageLogo.png" alt="COHERENT Logo" align="left" width="300">
== 2024-03-02 MediaWiki Software update ==
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The <big>'''COHERENT'''</big> 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.
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<img src="https://coherent.phy.duke.edu/MainPageLogo.png" alt="COHERENT Logo" align="left" width="500">


<img src="https://coherent.phy.duke.edu/CoherentLogo-Medium-e1442029154437.png" alt="COHERENT public page" align="center" width="200">
The <big>'''COHERENT'''</big> collaboration measures '''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.


<!-- <img src="https://coherent.phy.duke.edu/CoherentLogo-Medium-e1442029154437.png" alt="COHERENT public page" align="center" width="200"> -->
If you reached this page accidentally, you can find the Public <big>'''COHERENT'''</big> page [http://sites.duke.edu/coherent here]
If you reached this page accidentally, you can find the Public <big>'''COHERENT'''</big> page [http://sites.duke.edu/coherent here]


== Internal Workgroup Pages ==
== Neutrino Alley ==
*[[CsI(Na) Subsystem]]
*[[Neutrino Alley Operations]] - Find emergency numbers here
*[[Neutrino Alley Lessons Learned]]
*[[SNS monitoring and EPICS slow controls]]
*[[Backgrounds]]
*[[Walk through Neutrino Alley]]
*[[Geometry of Neutrino Alley]]
*[[Posters for Neutrino Alley]]
*[[E-Log]]
 
== Detector Subsystems ==
Active Systems
*[[Single-Phase LAr Subsystem]] - Currently CENNS-10 (COH-Ar-10)
*[[NaI(Tl) Subsystem]]
*[[MARS Neutron Detector]] ([[MARS Neutron Detector#MARS meetings|Meetings]], [[MARS Neutron Detector#Scrum|Scrum]] , [[MARS Neutron Detector#MARS papers and technical notes|Papers]], [[MARS Simulation|Simulation]], [[MARS Neutron Detector#Operations|Operation]], [[MARS analysis|Analysis]])
*[[D2O Subsystem]]
*[[NuThor Subsystem]]
*[[HPGe PPC Subsystem]]
*[[HPGe PPC Subsystem]]
*[[PbGlass Subsystem]]
Systems Under construction
* [[COH-Ar-750]]
Planned Systems
*[[Cryogenic CsI Subsystem]] ([https://code.ornl.gov/COHERENT/Cryogenic-CsI/docs/-/boards To-do's], [https://code.ornl.gov/COHERENT/Cryogenic-CsI/docs/-/blob/master/README.md#meetings Meetings], [https://coherentsns.slack.com/archives/CL7UP5LMV Slack], [https://code.ornl.gov/COHERENT/Cryogenic-CsI GitLab], [https://www.zotero.org/groups/2773710/inorganic_scintillators/library References])
Past Systems
*[[2-Phase LXe Subsystem]]
*[[2-Phase LXe Subsystem]]
*[[NaI(Tl) Option]]
*[[Scibath Neutron Detector]]
*[[Single-Phase LAr Option]]
*[[Scatter Camera Neutron Detector]]
*[[CsI(Na) Subsystem]]
*[[Neutrino Induced Neutron Detectors]]
*[[Neutrino Induced Neutron Detectors]]
*[[MARS Detector]]
 
*[[Backgrounds]]
== Supporting Science ==
*[[SNS monitoring and EPICS slow controls]]
*[[Data Analysis Tools]]
*[[Data analysis]]
*[[UsingAnalysisCluster|ORNL Cluster]]
*[[Neutrino source simulation]]
*[[Neutrino source simulation]]
*[[Neutrino Alley Operations]]
*[[CEvNS Cross Section Calculations]]
*[[Quenching Factors]]
*[[Data Coordination]]
*[[Second Target Station]]


== The Collaboration ==
== The Collaboration ==
*[https://sites.duke.edu/coherent/publications/collaboration Collaboration List]


*[https://sites.duke.edu/coherent/publications/ Collaboration Papers]
*[https://coherent.phy.duke.edu/w/img_auth.php/9/97/Code-of-conduct-aug16.pdf COHERENT Collaboration code of conduct ]


*[https://sites.duke.edu/coherent/presentations/ Public Presentations]:  public page
*[https://sites.duke.edu/coherent/for-the-public/#collaboration Collaboration List]


*[[Collaboration Documents]]: internal
*[[Official COHERENT Logo files]] and Zoom backgrounds


*[[Meetings]]: internal
*[https://sites.duke.edu/coherent/publications/ Collaboration Papers]: public page on coherent www site


*[[Public_Presentations]]: internal
*[https://sites.duke.edu/coherent/publications/ Website Posted Public Presentations]: public page on coherent www site


*[[Official Plots]]: Internal
*[[Collaboration Papers]]: internal wiki page, for journal papers and paper reviews


*[[Official COHERENT Logo files]]
*[[Collaboration Documents]]: internal wiki page:  CB documents, tech notes, proposals, white papers, theses
 
*[[Public_Presentations]]: internal wiki page
 
*[[Meetings]]: internal wiki page
 
*[[Official Plots]]: Internal wiki page
 
*[[Collaboration_Software | Collaboration Software]]: Internal wiki page for collection/organization of software in use by the collaboration.


== Information for Collaborators ==
== Information for Collaborators ==
*[[Signing up for listhost coherent@phy.duke.edu]]
*[[Signing up for the COHERENT mailing list]]


*[[Accessing the Slack Team page]]
*[[Accessing the Slack Team page]]
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*[[ShareLatex at ORNL]]
*[[ShareLatex at ORNL]]
*[[References]]
*[[Citations]]
*[[Postdoc openings, Job opportunities, Career Information]]
*[[Opportunities, Summer Schools, Seminar Series]]
*[[COHERENT How Tos]]


== Other ==
== Other ==
*[[Wiki Best Practices]]
*[[Sandbox]]
*[[Sandbox]]
*[[Quenching Factor runs at TUNL]]
*[[3D printing]]
*[[3D printing]]


== Obsolete Connections ==
== Obsolete Connections ==
'''The old WIKI can still be found at http://csisns.phy.duke.edu/ '''
'''The old WIKI can still be found at https://old-coherent.phy.duke.edu/wiki/Main_Page '''

Latest revision as of 19:26, 16 April 2024


2024-03-02 MediaWiki Software update

Software update has occurred. InCommon login is no longer supported.
Existing local wiki users shouldn't notice any difference.
People can contact problem@phy.duke.edu for account assistance. Email kate.scholberg@duke.edu if no response.


COHERENT Logo

The COHERENT collaboration measures 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

Neutrino Alley

Detector Subsystems

Active Systems

Systems Under construction

Planned Systems

Past Systems

Supporting Science

The Collaboration

Information for Collaborators

Other

Obsolete Connections

The old WIKI can still be found at https://old-coherent.phy.duke.edu/wiki/Main_Page