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COHERENT Collaboration

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COHERENT Collaboration
NameCOHERENT Collaboration
Established2009
FieldNeutrino physics
HeadquartersOak Ridge National Laboratory
Notable experimentsCOHERENT at SNS

COHERENT Collaboration

The COHERENT Collaboration is an experimental collaboration focused on low-energy neutrino interactions, formed to detect coherent elastic neutrino–nucleus scattering (CEvNS). It operates primarily at the Spallation Neutron Source and involves national laboratories and universities engaged with particle physics, nuclear physics, and detector development. The collaboration bridges research at Oak Ridge National Laboratory, Los Alamos National Laboratory, and multiple academic institutions to advance precision measurements relevant to particle physics and astrophysics.

Overview

COHERENT assembles physicists and engineers from institutions including Oak Ridge National Laboratory, Los Alamos National Laboratory, Fermi National Accelerator Laboratory, Brookhaven National Laboratory, Lawrence Berkeley National Laboratory, SLAC National Accelerator Laboratory, University of Chicago, Massachusetts Institute of Technology, University of California, Berkeley, Stanford University, Columbia University, University of Oxford, Imperial College London, University of Tokyo, University of Manchester, University of Edinburgh, University of California, Los Angeles, University of California, Irvine, University of Washington, University of Colorado Boulder, California Institute of Technology, Princeton University, Yale University, Harvard University, Johns Hopkins University, University of Minnesota, University of Pennsylvania, Duke University, Rutgers University, Texas A&M University, Virginia Tech, Pennsylvania State University, Arizona State University, University of Arizona, Michigan State University, Northwestern University, University of Illinois Urbana-Champaign, University of Wisconsin–Madison, University of Notre Dame, University of Florida, University of Texas at Austin, University of California, Santa Barbara, University of California, San Diego, University of British Columbia, McGill University, TRIUMF, RIKEN, KEK, and CERN in collaborative roles.

History and Formation

The collaboration originated from proposals to measure CEvNS using pulsed neutrino sources at the Spallation Neutron Source at Oak Ridge National Laboratory after theoretical predictions by Daniel Z. Freedman, and discussions involving researchers affiliated with Los Alamos National Laboratory and Fermi National Accelerator Laboratory. Early planning engaged experts with connections to experimental programs at Super-Kamiokande, SNO, MINERvA, MiniBooNE, COBRA, XMASS, LUX-ZEPLIN, and XENON1T who contributed detector expertise. Founding meetings occurred alongside workshops hosted by American Physical Society, American Nuclear Society, Institute of Physics, and at conferences such as Neutrino 2012 and TAUP.

Scientific Goals and Research Program

COHERENT’s primary objective is the first observation and precision study of CEvNS predicted in the 1970s by Daniel Z. Freedman with implications for tests of the Standard Model (particle physics), searches for physics beyond the Standard Model (particle physics), and constraints on sterile neutrino scenarios explored in experiments like LSND and MiniBooNE. The program addresses neutrino-nucleus interaction modeling relevant to Supernova SN 1987A neutrino emission, dark matter direct-detection background estimates informed by LUX-ZEPLIN and XENONnT, and measurements that complement oscillation results from NOvA, T2K, Daya Bay, and Double Chooz. COHERENT also pursues studies of non-standard neutrino interactions connected to proposals by groups at CERN and theorists affiliated with Harvard University, Princeton University, University of California, Berkeley, and MIT.

Experimental Apparatus and Detectors

The experimental suite is deployed in the Spallation Neutron Source “neutrino alley” and utilizes a range of detector technologies contributed by teams from Lawrence Berkeley National Laboratory, Los Alamos National Laboratory, Brookhaven National Laboratory, Fermi National Accelerator Laboratory, TRIUMF, McGill University, University of Chicago, Duke University, Yale University, University of Colorado Boulder, University of Minnesota, University of Washington, University of Tennessee, University of South Carolina, and Virginia Tech. Detector systems include a low-threshold CsI scintillator array that demonstrated early CEvNS signals, high-purity germanium detector arrays informed by MAJORANA and GERDA technologies, cryogenic sapphire or silicon detectors influenced by SuperCDMS development, and noble-liquid argon detector modules paralleling designs from DarkSide and MicroBooNE. Ancillary systems rely on neutron monitoring from instruments used at Los Alamos Neutron Science Center and shielding techniques developed at Gran Sasso National Laboratory.

Key Results and Publications

COHERENT achieved the first unambiguous observation of CEvNS using a cesium iodide detector, reported alongside analyses comparing event rates with Standard Model predictions and uncertainty budgets informed by input from theorists at MIT, Princeton University, University of Chicago, Harvard University, and University of California, Berkeley. Subsequent publications detailed CEvNS measurements on argon and germanium targets, constraints on non-standard interactions discussed in papers appearing in journals frequented by contributors from Physical Review Letters, Physical Review D, Journal of High Energy Physics, and Physics Letters B. The collaboration’s dataset has been used in joint analyses with teams from NOvA, T2K, IceCube, Super-Kamiokande, KamLAND, and SNO+ to explore implications for neutrino properties and astrophysical neutrino fluxes.

Collaborating Institutions and Governance

Governance comprises institutional representatives from Oak Ridge National Laboratory, Los Alamos National Laboratory, Fermi National Accelerator Laboratory, Brookhaven National Laboratory, Lawrence Berkeley National Laboratory, TRIUMF, CERN, University of Chicago, Massachusetts Institute of Technology, Princeton University, Harvard University, Stanford University, Columbia University, University of Oxford, Imperial College London, University of Tokyo, KEK, RIKEN, McGill University, University of British Columbia, University of Toronto, University of California, Berkeley, Yale University, University of Minnesota, and University of Wisconsin–Madison. The collaboration operates with institutional boards, executive committees, and technical working groups modeled after frameworks used by ATLAS, CMS, LIGO Scientific Collaboration, and IceCube. Funding and oversight involve agencies and program offices linked to U.S. Department of Energy, National Science Foundation, Natural Sciences and Engineering Research Council of Canada, Japan Society for the Promotion of Science, and European funding bodies coordinating contributions from CERN member states.

Outreach and Education Activities

COHERENT members engage in outreach at venues such as the American Physical Society meetings, Neutrino 2014, Neutrino 2018, public events at Oak Ridge National Laboratory, university open days at University of Chicago and Massachusetts Institute of Technology, and workshops with educators from National Science Teaching Association and Society for Science & the Public. The collaboration supports graduate and undergraduate training through programs affiliated with Fermi National Accelerator Laboratory, Los Alamos National Laboratory, Lawrence Berkeley National Laboratory, TRIUMF, CERN, and host universities, and contributes to curriculum resources used in summer schools such as Triton Schools and topical schools organized by Institut d'Astrophysique de Paris and Les Houches.

Category:Neutrino experiments