• Open Access

Dark Matter Signals from Timing Spectra at Neutrino Experiments

Bhaskar Dutta, Doojin Kim, Shu Liao, Jong-Chul Park, Seodong Shin, and Louis E. Strigari
Phys. Rev. Lett. 124, 121802 – Published 26 March 2020
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Abstract

We propose a novel strategy to search for new physics in timing spectra at low-energy neutrino experiments using a pulsed beam, envisioning the situation in which a new particle comes from the decay of its heavier partner with a finite particle width. The timing distribution of events induced by the dark matter (DM) candidate particle scattering at the detector may populate in a relatively narrow range, forming a “resonancelike” shape. Because of this structural feature, the signal may be isolated from the backgrounds, in particular when the backgrounds are uniformly distributed in energy and time. For proof of the principle, we investigate the discovery potential for DM from the decay of a dark photon in the ongoing COHERENT experiment and show the exciting prospects for exploring the associated parameter space with this experiment. We analyze the existing CsI detector data with a timing cut and an energy cut, and we find, for the first time, an excess in the timing distribution that can be explained by such DM. We compare the sensitivity to the kinetic mixing parameter (ε) for current and future COHERENT experiments with the projected limits from LDMX and DUNE.

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  • Received 30 July 2019
  • Revised 13 February 2020
  • Accepted 28 February 2020

DOI:https://doi.org/10.1103/PhysRevLett.124.121802

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Bhaskar Dutta1,*, Doojin Kim1,2,†, Shu Liao1,‡, Jong-Chul Park3,§, Seodong Shin4,5,6,∥, and Louis E. Strigari1,¶

  • 1Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
  • 2Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
  • 3Department of Physics, Chungnam National University, Daejeon 34134, Republic of Korea
  • 4Department of Physics and IPAP, Yonsei University, Seoul 03722, Republic of Korea
  • 5Center for Theoretical Physics of the Universe, Institute for Basic Science, Daejeon 34126, Republic of Korea
  • 6Department of Physics, Jeonbuk National University, Jeonju, Jeonbuk 54896, Republic of Korea

  • *dutta@physics.tamu.edu
  • doojin.kim@tamu.edu
  • ikaros@physics.tamu.edu
  • §jcpark@cnu.ac.kr
  • sshin@jbnu.ac.kr
  • strigari@tamu.edu

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Issue

Vol. 124, Iss. 12 — 27 March 2020

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