The COHERENT Experiment: 2026 Update
Abstract
The COHERENT experiment measures neutrino-induced recoils from coherent elastic neutrino-nucleus scattering (CEvNS) with multiple nuclear targets at the Spallation Neutron Source (SNS) at the Oak Ridge National Laboratory (ORNL), USA. Several successful CEvNS measurements have been achieved in recent years with tens-of-kg detector masses, with a CsI scintillating crystal, a liquid argon single-phase detector, and high-purity germanium spectrometers. For the next phase, COHERENT aims at high-statistics detection of CEvNS events for precision tests of the standard model of particle physics, and to probe new physics beyond-the-standard model. Percent-level precision can be achieved by lowering thresholds, reducing backgrounds, and by scaling up the detector masses. It goes hand in hand with benchmarking the neutrino flux from the SNS. Further detectors will measure CEvNS in additional nuclei, including lighter target nuclei such as sodium and neon, to continue to test the expected neutron-number-squared dependence of the cross section. COHERENT can furthermore study charged-current and neutral-current inelastic neutrino-nucleus cross sections on various nuclei at neutrino energies below 50 MeV. Many of these cross sections have never been measured before, but are critical input for the interpretation of core-collapse supernova detection in large-scale neutrino experiments such as DUNE, Super-K, Hyper-K, and HALO.
Cite
@article{arxiv.2602.15652,
title = {The COHERENT Experiment: 2026 Update},
author = {M. Adhikari and M. Ahn and D. Amaya Matamoros and P. S. Barbeau and V. Belov and I. Bernardi and C. Bock and A. Bolozdynya and R. Bouabid and J. Browning and B. Cabrera-Palmer and N. Cedarblade-Jones and S. Chen and A. I. Colón Rivera and V. da Silva and J. Daughhetee and Y. Efremenko and S. R. Elliott and A. Erlandson and L. Fabris and M. L. Fischer and S. Foster and A. Galindo-Uribarri and E. Granados Vazquez and M. P. Green and B. Hackett and J. Hakenmüller and M. Harada and M. R. Heath and S. Hedges and Y. Hino and H. Huang and W. Huang and H. Jeong and B. A. Johnson and T. Johnson and A. Khromov and D. Kim and L. Kong and A. Konovalov and Y. Koshio and E. Kozlova and A. Kumpan and O. Kyzylova and Y. Lee and S. M. Lee and G. Li and L. Li and Z. Li and J. M. Link and J. Liu and Q. Liu and X. Lu and M. Luxnat and D. M. Markoff and J. Mattingly and H. McLaurin and K. McMichael and N. Meredith and Y. Nakajima and F. Nakanishi and J. Newby and B. Nolan and J. O'Reilly and A. Orvedahl and D. S. Parno and D. Pérez-Loureiro and D. Pershey and C. G. Prior and J. Queen and R. Rapp and H. Ray and O. Razuvaeva and D. Reyna and D. Rudik and J. Runge and D. J. Salvat and J. Sander and K. Scholberg and H. Sekiya and J. Seligman and A. Shakirov and G. Simakov and J. Skweres and W. M. Snow and V. Sosnovtsev and Q. Stefan and M. Stringer and C. Su and T. Subedi and B. Suh and B. Sur and R. Tayloe and Y. -T. Tsai and J. Vaccaro and E. E. van Nieuwenhuizen and C. J. Virtue and G. Visser and K. Walkup and E. M. Ward and R. Wendell and T. Wongjirad and C. Yang and Y. Yang and J. Yoo and C. -H. Yu and Y. Yu and A. Zaalishvili and J. Zettlemoyer and Y. Zheng},
journal= {arXiv preprint arXiv:2602.15652},
year = {2026}
}
Comments
originally prepared in response to a request from the Neutrinos & Cosmic Messengers section of the Update of the European Strategy for Particle Physics