Constraints on Lightly Ionizing Particles from CDMSlite
Affiliations
- 1 Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada.
- 2 Department of Physics, Durham University, Durham DH1 3LE, United Kingdom.
- 3 Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA.
- 4 SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA.
- 5 Pacific Northwest National Laboratory, Richland, Washington, D.C. 99352, USA.
- 6 Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA.
- 7 School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India.
- 8 School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA.
- 9 Department of Physics, University of Florida, Gainesville, Florida 32611, USA.
- 10 Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
- 11 Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
- 12 TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
- 13 Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA.
- 14 Department of Physics, Stanford University, Stanford, California 94305, USA.
- 15 Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA.
- 16 Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain.
- 17 Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA.
- 18 Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada.
- 19 Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada.
- 20 Department of Physics, University of California, Berkeley, California 94720, USA.
- 21 Department of Electrical and Computer Engineering, Texas A&M University, College Station, Texas 77843, USA.
- 22 Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA.
- 23 Department of Electrical Engineering, University of Colorado Denver, Denver, Colorado 80217, USA.
- 24 Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany.
- 25 Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA.
- 26 Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.
- 27 SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada.
- 28 Laurentian University, Department of Physics, 935 Ramsey Lake Road, Sudbury, Ontario P3E 2C6, Canada.
- 29 Department of Physics, Santa Clara University, Santa Clara, California 95053, USA.
- PMID: 34477436
- DOI: 10.1103/PhysRevLett.127.081802
Constraints on Lightly Ionizing Particles from CDMSlite
Authors
Affiliations
- 1 Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada.
- 2 Department of Physics, Durham University, Durham DH1 3LE, United Kingdom.
- 3 Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA.
- 4 SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA.
- 5 Pacific Northwest National Laboratory, Richland, Washington, D.C. 99352, USA.
- 6 Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA.
- 7 School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India.
- 8 School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA.
- 9 Department of Physics, University of Florida, Gainesville, Florida 32611, USA.
- 10 Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
- 11 Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
- 12 TRIUMF, Vancouver, British Columbia V6T 2A3, Canada.
- 13 Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA.
- 14 Department of Physics, Stanford University, Stanford, California 94305, USA.
- 15 Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA.
- 16 Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain.
- 17 Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA.
- 18 Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada.
- 19 Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada.
- 20 Department of Physics, University of California, Berkeley, California 94720, USA.
- 21 Department of Electrical and Computer Engineering, Texas A&M University, College Station, Texas 77843, USA.
- 22 Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA.
- 23 Department of Electrical Engineering, University of Colorado Denver, Denver, Colorado 80217, USA.
- 24 Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany.
- 25 Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA.
- 26 Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.
- 27 SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada.
- 28 Laurentian University, Department of Physics, 935 Ramsey Lake Road, Sudbury, Ontario P3E 2C6, Canada.
- 29 Department of Physics, Santa Clara University, Santa Clara, California 95053, USA.
- PMID: 34477436
- DOI: 10.1103/PhysRevLett.127.081802
Abstract
The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to lightly ionizing particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically produced LIPs with an electric charge smaller than e/(3×10^{5}), as well as the strongest limits for charge ≤e/160, with a minimum vertical intensity of 1.36×10^{-7} cm^{-2} s^{-1} sr^{-1} at charge e/160. These results apply over a wide range of LIP masses (5 MeV/c^{2} to 100 TeV/c^{2}) and cover a wide range of βγ values (0.1-10^{6}), thus excluding nonrelativistic LIPs with βγ as small as 0.1 for the first time.
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