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Berlin A, Trickle T. Absorption of Axion Dark Matter in a Magnetized Medium. PHYSICAL REVIEW LETTERS 2024; 132:181801. [PMID: 38759193 DOI: 10.1103/physrevlett.132.181801] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/05/2023] [Revised: 01/05/2024] [Accepted: 03/20/2024] [Indexed: 05/19/2024]
Abstract
Detection of axion dark matter heavier than an meV is hindered by its small wavelength, which limits the useful volume of traditional experiments. This problem can be avoided by directly detecting in-medium excitations, whose ∼meV-eV energies are decoupled from the detector size. We show that for any target inside a magnetic field, the absorption rate of electromagnetically coupled axions into in-medium excitations is determined by the dielectric function. As a result, the plethora of candidate targets previously identified for sub-GeV dark matter searches can be repurposed as broadband axion detectors. We find that a kg yr exposure with noise levels comparable to recent measurements is sufficient to probe parameter space currently unexplored by laboratory tests. Noise reduction by only a few orders of magnitude can enable sensitivity to the QCD axion in the ∼10 meV-10 eV mass range.
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Affiliation(s)
- Asher Berlin
- Theoretical Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Tanner Trickle
- Theoretical Physics Division, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
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Mokina V, Schieck J. Rare event searches with cryogenic detectors. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2024; 382:20230091. [PMID: 38104622 DOI: 10.1098/rsta.2023.0091] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/07/2023] [Accepted: 10/10/2023] [Indexed: 12/19/2023]
Abstract
Cryogenic detectors can detect the smallest energy depositions via the scattering of the incoming particle with the detector material. The deposited energy leads to minimal temperature rises of a few [Formula: see text], read out via transition edge sensors and SQUIDs. Using scintillating crystals as detector material offers the possibility of discriminating between nuclear recoils from dark matter scattering and electromagnetic background events. The CRESST experiment pioneered this technology and is still among the most sensitive experiments searching for sub-GeV dark matter particles. The technology is now also used by other experiments for dark matter searches (COSINUS) and for measuring coherent elastic neutrino-nucleus scattering (NUCLEUS). We discuss cryogenic detectors' detection principle and their application. We present the latest dark matter results from CRESST, a new type of background, and the status of the COSINUS and NUCLEUS experiments. This article is part of the theme issue 'The particle-gravity frontier'.
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Affiliation(s)
- Valentyna Mokina
- Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, Wien 1050, Austria
| | - Jochen Schieck
- Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, Wien 1050, Austria
- Atominstitut, Technische Universität Wien, Wien 1050, Austria
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3
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Albakry MF, Alkhatib I, Alonso D, Amaral DWP, Aralis T, Aramaki T, Arnquist IJ, Ataee Langroudy I, Azadbakht E, Banik S, Bathurst C, Bhattacharyya R, Brink PL, Bunker R, Cabrera B, Calkins R, Cameron RA, Cartaro C, Cerdeño DG, Chang YY, Chaudhuri M, Chen R, Chott N, Cooley J, Coombes H, Corbett J, Cushman P, Das S, De Brienne F, Rios M, Dharani S, di Vacri ML, Diamond MD, Elwan M, Fascione E, Figueroa-Feliciano E, Fink CW, Fouts K, Fritts M, Gerbier G, Germond R, Ghaith M, Golwala SR, Hall J, Harms SAS, Hassan N, Hines BA, Hong Z, Hoppe EW, Hsu L, Huber ME, Iyer V, Kashyap VKS, Kelsey MH, Kubik A, Kurinsky NA, Lee M, Litke M, Liu J, Liu Y, Loer B, Lopez Asamar E, Lukens P, MacFarlane DB, Mahapatra R, Mast N, Mayer AJ, Meyer Zu Theenhausen H, Michaud É, Michielin E, Mirabolfathi N, Mohanty B, Nebolsky B, Nelson J, Neog H, Novati V, Orrell JL, Osborne MD, Oser SM, Page WA, Pandey L, Pandey S, Partridge R, Pedreros DS, Perna L, Podviianiuk R, Ponce F, Poudel S, Pradeep A, Pyle M, Rau W, Reid E, Ren R, Reynolds T, Tanner E, Roberts A, Robinson AE, Saab T, Sadek D, Sadoulet B, Sahoo SP, Saikia I, Sander J, Sattari A, Schmidt B, Schnee RW, Scorza S, Serfass B, Poudel SS, Sincavage DJ, Sinervo P, Speaks Z, Street J, Sun H, Terry GD, Thasrawala FK, Toback D, Underwood R, Verma S, Villano AN, von Krosigk B, Watkins SL, Wen O, Williams Z, Wilson MJ, Winchell J, Wykoff K, Yellin S, Young BA, Yu TC, Zatschler B, Zatschler S, Zaytsev A, Zeolla A, Zhang E, Zheng L, Zheng Y, Zuniga A, An P, Barbeau PS, Hedges SC, Li L, Runge J. First Measurement of the Nuclear-Recoil Ionization Yield in Silicon at 100 eV. PHYSICAL REVIEW LETTERS 2023; 131:091801. [PMID: 37721818 DOI: 10.1103/physrevlett.131.091801] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/21/2023] [Revised: 07/07/2023] [Accepted: 07/26/2023] [Indexed: 09/20/2023]
Abstract
We measured the nuclear-recoil ionization yield in silicon with a cryogenic phonon-sensitive gram-scale detector. Neutrons from a monoenergetic beam scatter off of the silicon nuclei at angles corresponding to energy depositions from 4 keV down to 100 eV, the lowest energy probed so far. The results show no sign of an ionization production threshold above 100 eV. These results call for further investigation of the ionization yield theory and a comprehensive determination of the detector response function at energies below the keV scale.
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Affiliation(s)
- M F Albakry
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - I Alkhatib
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - D Alonso
- Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain
- Instituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain
| | - D W P Amaral
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - T Aralis
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - T Aramaki
- Department of Physics, Northeastern University, 360 Huntington Avenue, Boston, Massachusetts 02115, USA
| | - I J Arnquist
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - I Ataee Langroudy
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - E Azadbakht
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - S Banik
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni - 752050, India
| | - C Bathurst
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - R Bhattacharyya
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - P L Brink
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - R Bunker
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - B Cabrera
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - R Calkins
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - R A Cameron
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - C Cartaro
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - D G Cerdeño
- Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain
- Instituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain
| | - Y-Y Chang
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - M Chaudhuri
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni - 752050, India
| | - R Chen
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - N Chott
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - J Cooley
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
| | - H Coombes
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - J Corbett
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - P Cushman
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - S Das
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni - 752050, India
| | - F De Brienne
- Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
| | - M Rios
- Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain
- Instituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain
| | - S Dharani
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
- Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
| | - M L di Vacri
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - M D Diamond
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - M Elwan
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - E Fascione
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - E Figueroa-Feliciano
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - C W Fink
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - K Fouts
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - M Fritts
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - G Gerbier
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - R Germond
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - M Ghaith
- College of Natural and Health Sciences, Zayed University, Dubai, 19282, United Arab Emirates
| | - S R Golwala
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - J Hall
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
- Laurentian University, Department of Physics, 935 Ramsey Lake Road, Sudbury, Ontario P3E 2C6, Canada
| | - S A S Harms
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - N Hassan
- Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
| | - B A Hines
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - Z Hong
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - E W Hoppe
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - L Hsu
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - M E Huber
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
- Department of Electrical Engineering, University of Colorado Denver, Denver, Colorado 80217, USA
| | - V Iyer
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - V K S Kashyap
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni - 752050, India
| | - M H Kelsey
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - A Kubik
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
| | - N A Kurinsky
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - M Lee
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - M Litke
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - J Liu
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - Y Liu
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - B Loer
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - E Lopez Asamar
- Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain
- Instituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain
| | - P Lukens
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - D B MacFarlane
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - R Mahapatra
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - N Mast
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A J Mayer
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - H Meyer Zu Theenhausen
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
| | - É Michaud
- Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
| | - E Michielin
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - N Mirabolfathi
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - B Mohanty
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni - 752050, India
| | - B Nebolsky
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - J Nelson
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - H Neog
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Novati
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - J L Orrell
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - M D Osborne
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - S M Oser
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - W A Page
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - L Pandey
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - S Pandey
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - R Partridge
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - D S Pedreros
- Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
| | - L Perna
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - R Podviianiuk
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - F Ponce
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - S Poudel
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - A Pradeep
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - M Pyle
- Department of Physics, University of California, Berkeley, California 94720, USA
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - W Rau
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - E Reid
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - R Ren
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - T Reynolds
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - E Tanner
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Roberts
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - A E Robinson
- Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
| | - T Saab
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - D Sadek
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - B Sadoulet
- Department of Physics, University of California, Berkeley, California 94720, USA
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - S P Sahoo
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - I Saikia
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - J Sander
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - A Sattari
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - B Schmidt
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - R W Schnee
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - S Scorza
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
- Laurentian University, Department of Physics, 935 Ramsey Lake Road, Sudbury, Ontario P3E 2C6, Canada
| | - B Serfass
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - S S Poudel
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - D J Sincavage
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - P Sinervo
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - Z Speaks
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - J Street
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - H Sun
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - G D Terry
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - F K Thasrawala
- Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
| | - D Toback
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - R Underwood
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - S Verma
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - A N Villano
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - B von Krosigk
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
| | - S L Watkins
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - O Wen
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Williams
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M J Wilson
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
| | - J Winchell
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - K Wykoff
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - S Yellin
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - B A Young
- Department of Physics, Santa Clara University, Santa Clara, California 95053, USA
| | - T C Yu
- SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - B Zatschler
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - S Zatschler
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - A Zaytsev
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
| | - A Zeolla
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - E Zhang
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - L Zheng
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - Y Zheng
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - A Zuniga
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - P An
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - P S Barbeau
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - S C Hedges
- Lawrence Livermore National Laboratory, Livermore, California 94550, USA
| | - L Li
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - J Runge
- Department of Physics, Duke University, Durham, North Carolina 27708, USA
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Sassi S, Heikinheimo M, Tuominen K, Kuronen A, Byggmästar J, Nordlund K, Mirabolfathi N. Energy loss in low energy nuclear recoils in dark matter detector materials. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.063012] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Kahn Y, Lin T. Searches for light dark matter using condensed matter systems. REPORTS ON PROGRESS IN PHYSICS. PHYSICAL SOCIETY (GREAT BRITAIN) 2022; 85:066901. [PMID: 35313296 DOI: 10.1088/1361-6633/ac5f63] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/06/2021] [Accepted: 03/21/2022] [Indexed: 06/14/2023]
Abstract
Identifying the nature of dark matter (DM) has long been a pressing question for particle physics. In the face of ever-more-powerful exclusions and null results from large-exposure searches for TeV-scale DM interacting with nuclei, a significant amount of attention has shifted to lighter (sub-GeV) DM candidates. Direct detection of the light DM in our galaxy by observing DM scattering off a target system requires new approaches compared to prior searches. Lighter DM particles have less available kinetic energy, and achieving a kinematic match between DM and the target mandates the proper treatment of collective excitations in condensed matter systems, such as charged quasiparticles or phonons. In this context, the condensed matter physics of the target material is crucial, necessitating an interdisciplinary approach. In this review, we provide a self-contained introduction to direct detection of keV-GeV DM with condensed matter systems. We give a brief survey of DM models and basics of condensed matter, while the bulk of the review deals with the theoretical treatment of DM-nucleon and DM-electron interactions. We also review recent experimental developments in detector technology, and conclude with an outlook for the field of sub-GeV DM detection over the next decade.
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Affiliation(s)
- Yonatan Kahn
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL 61801, United States of America
- Illinois Center for Advanced Studies of the Universe, University of Illinois at Urbana-Champaign, Urbana, IL 61801, United States of America
| | - Tongyan Lin
- Department of Physics, University of California, San Diego, CA 92093, United States of America
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6
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Hochberg Y, von Krosigk B, Kuflik E, Yu TC. Impact of Dark Compton Scattering on Direct Dark Matter Absorption Searches. PHYSICAL REVIEW LETTERS 2022; 128:191801. [PMID: 35622031 DOI: 10.1103/physrevlett.128.191801] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/28/2021] [Accepted: 04/14/2022] [Indexed: 06/15/2023]
Abstract
Direct detection experiments are gaining in mass reach. Here we show that the inclusion of dark Compton scattering, which has typically been neglected in absorption searches, has a substantial impact on the reach and discovery potential of direct detection experiments at high bosonic cold dark matter masses. We demonstrate this for relic dark photons and axionlike particles: we improve expected reach across materials, and further use results from SuperCDMS, EDELWEISS, and GERDA to place enhanced limits on dark matter parameter space. We outline the implications for detector design and analysis.
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Affiliation(s)
- Yonit Hochberg
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - Belina von Krosigk
- Institute for Astroparticle Physics (IAP), Karlsruhe Institute of Technology (KIT), 76344 Eggenstein-Leopoldshafen, Germany
- Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
| | - Eric Kuflik
- Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
| | - To Chin Yu
- Department of Physics, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
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7
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Billard J, Boulay M, Cebrián S, Covi L, Fiorillo G, Green A, Kopp J, Majorovits B, Palladino K, Petricca F, Roszkowski Chair L, Schumann M. Direct detection of dark matter-APPEC committee report. REPORTS ON PROGRESS IN PHYSICS. PHYSICAL SOCIETY (GREAT BRITAIN) 2022; 85:056201. [PMID: 35193133 DOI: 10.1088/1361-6633/ac5754] [Citation(s) in RCA: 6] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/23/2021] [Accepted: 02/22/2022] [Indexed: 06/14/2023]
Abstract
This report provides an extensive review of the experimental programme of direct detection searches of particle dark matter. It focuses mostly on European efforts, both current and planned, but does it within a broader context of a worldwide activity in the field. It aims at identifying the virtues, opportunities and challenges associated with the different experimental approaches and search techniques. It presents scientific and technological synergies, both existing and emerging, with some other areas of particle physics, notably collider and neutrino programmes, and beyond. It addresses the issue of infrastructure in light of the growing needs and challenges of the different experimental searches. Finally, the report makes a number of recommendations from the perspective of a long-term future of the field. They are introduced, along with some justification, in the opening overview and recommendations section and are next summarised at the end of the report. Overall, we recommend that the direct search for dark matter particle interactions with a detector target should be given top priority in astroparticle physics, and in all particle physics, and beyond, as a positive measurement will provide the most unambiguous confirmation of the particle nature of dark matter in the Universe.
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Affiliation(s)
- Julien Billard
- Univ Lyon, Université Lyon 1, CNRS/IN2P3, IP2I-Lyon, F-69622, Villeurbanne, France
| | - Mark Boulay
- Department of Physics, Carleton University, Ottawa, Canada
| | - Susana Cebrián
- Centro de Astropartículas y Física de Altas Energías, Universidad de Zaragoza, Zaragoza, Spain
| | - Laura Covi
- Institute for Theoretical Physics, Georg-August University, Goettingen, Germany
| | - Giuliana Fiorillo
- Physics Department, Università degli Studi 'Federico II' di Napoli and INFN Napoli, Naples, Italy
| | - Anne Green
- School of Physics and Astronomy, University of Nottingham, Nottingham, United Kingdom
| | - Joachim Kopp
- CERN, Geneva, Switzerland and Johannes Gutenberg University, Mainz, Germany
| | | | - Kimberly Palladino
- Department of Physics, University of Wisconsin-Madison, Madison, WI, United States of America
- Department of Physics, Oxford University, Oxford, United Kingdom
| | | | - Leszek Roszkowski Chair
- Astrocent, Nicolaus Copernicus Astronomical Center PAS, Warsaw, Poland
- National Centre for Nuclear Research, Warsaw, Poland
| | - Marc Schumann
- Institute of Physics, University of Freiburg, Freiburg, Germany
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8
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Liu J, Dona K, Hoshino G, Knirck S, Kurinsky N, Malaker M, Miller DW, Sonnenschein A, Awida MH, Barry PS, Berggren KK, Bowring D, Carosi G, Chang C, Chou A, Khatiwada R, Lewis S, Li J, Nam SW, Noroozian O, Zhou TX. Broadband Solenoidal Haloscope for Terahertz Axion Detection. PHYSICAL REVIEW LETTERS 2022; 128:131801. [PMID: 35426699 DOI: 10.1103/physrevlett.128.131801] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/25/2021] [Accepted: 03/03/2022] [Indexed: 06/14/2023]
Abstract
We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program. This haloscope plans to search for bosonic dark matter across the [10^{-3},1] eV ([0.24, 240] THz) mass range. BREAD proposes a cylindrical metal barrel to convert dark matter into photons, which a novel parabolic reflector design focuses onto a photosensor. This unique geometry enables enclosure in standard cryostats and high-field solenoids, overcoming limitations of current dish antennas. A pilot 0.7 m^{2} barrel experiment planned at Fermilab is projected to surpass existing dark photon coupling constraints by over a decade with one-day runtime. Axion sensitivity requires <10^{-20} W/sqrt[Hz] sensor noise equivalent power with a 10 T solenoid and 10 m^{2} barrel. We project BREAD sensitivity for various sensor technologies and discuss future prospects.
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Affiliation(s)
- Jesse Liu
- Cavendish Laboratory, University of Cambridge, Cambridge CB3 0HE, United Kingdom
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - Kristin Dona
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - Gabe Hoshino
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Stefan Knirck
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Noah Kurinsky
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - Matthew Malaker
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - David W Miller
- Department of Physics, University of Chicago, Chicago, Illinois 60637, USA
- Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
| | | | - Mohamed H Awida
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Peter S Barry
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - Karl K Berggren
- Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Daniel Bowring
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Gianpaolo Carosi
- Lawrence Livermore National Laboratory, Livermore, California 94551, USA
| | - Clarence Chang
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - Aaron Chou
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Rakshya Khatiwada
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
- Department of Physics, Illinois Institute of Technology, Chicago, Illinois 60616, USA
| | - Samantha Lewis
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Juliang Li
- Argonne National Laboratory, Lemont, Illinois 60439, USA
| | - Sae Woo Nam
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - Omid Noroozian
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - Tony X Zhou
- Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
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9
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Afek G, Carney D, Moore DC. Coherent Scattering of Low Mass Dark Matter from Optically Trapped Sensors. PHYSICAL REVIEW LETTERS 2022; 128:101301. [PMID: 35333080 DOI: 10.1103/physrevlett.128.101301] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/05/2021] [Accepted: 01/21/2022] [Indexed: 06/14/2023]
Abstract
We propose a search for low mass dark matter particles through momentum recoils caused by their scattering from trapped, nanometer-scale objects. Our projections show that even with a modest array of femtogram-mass sensors, parameter space beyond the reach of existing experiments can be explored. The case of smaller, attogram-mass sensors is also analyzed-where dark matter can coherently scatter from the entire sensor-enabling a large enhancement in the scattering cross-section relative to interactions with single nuclei. Large arrays of such sensors have the potential to investigate new parameter space down to dark matter masses as low as 10 keV. If recoils from dark matter are detected by such sensors, their inherent directional sensitivity would allow an unambiguous identification of a dark matter signal.
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Affiliation(s)
- Gadi Afek
- Wright Laboratory, Department of Physics, Yale University, New Haven, Connecticut 06520, USA
| | - Daniel Carney
- Physics Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - David C Moore
- Wright Laboratory, Department of Physics, Yale University, New Haven, Connecticut 06520, USA
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10
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Alkhatib I, Amaral DWP, Aralis T, Aramaki T, Arnquist IJ, Ataee Langroudy I, Azadbakht E, Banik S, Barker D, Bathurst C, Bauer DA, Bezerra LVS, Bhattacharyya R, Binder T, Bowles MA, Brink PL, Bunker R, Cabrera B, Calkins R, Cameron RA, Cartaro C, Cerdeño DG, Chang YY, Chaudhuri M, Chen R, Chott N, Cooley J, Coombes H, Corbett J, Cushman P, De Brienne F, di Vacri ML, Diamond MD, Fascione E, Figueroa-Feliciano E, Fink CW, Fouts K, Fritts M, Gerbier G, Germond R, Ghaith M, Golwala SR, Harris HR, Herbert N, Hines BA, Hollister MI, Hong Z, Hoppe EW, Hsu L, Huber ME, Iyer V, Jardin D, Jastram A, Kashyap VKS, Kelsey MH, Kubik A, Kurinsky NA, Lawrence RE, Li A, Loer B, Lopez Asamar E, Lukens P, MacDonell D, MacFarlane DB, Mahapatra R, Mandic V, Mast N, Mayer AJ, Meyer Zu Theenhausen H, Michaud ÉM, Michielin E, Mirabolfathi N, Mohanty B, Morales Mendoza JD, Nagorny S, Nelson J, Neog H, Novati V, Orrell JL, Oser SM, Page WA, Pakarha P, Partridge R, Podviianiuk R, Ponce F, Poudel S, Pyle M, Rau W, Reid E, Ren R, Reynolds T, Roberts A, Robinson AE, Saab T, Sadoulet B, Sander J, Sattari A, Schnee RW, Scorza S, Serfass B, Sincavage DJ, Stanford C, Street J, Toback D, Underwood R, Verma S, Villano AN, von Krosigk B, Watkins SL, Wills L, Wilson JS, Wilson MJ, Winchell J, Wright DH, Yellin S, Young BA, Yu TC, Zhang E, Zhang HG, Zhao X, Zheng L, Camilleri J, Kolomensky YG, Zuber S. Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground. PHYSICAL REVIEW LETTERS 2021; 127:061801. [PMID: 34420312 DOI: 10.1103/physrevlett.127.061801] [Citation(s) in RCA: 7] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/22/2020] [Revised: 05/06/2021] [Accepted: 07/08/2021] [Indexed: 06/13/2023]
Abstract
We present limits on spin-independent dark matter-nucleon interactions using a 10.6 g Si athermal phonon detector with a baseline energy resolution of σ_{E}=3.86±0.04(stat)_{-0.00}^{+0.19}(syst) eV. This exclusion analysis sets the most stringent dark matter-nucleon scattering cross-section limits achieved by a cryogenic detector for dark matter particle masses from 93 to 140 MeV/c^{2}, with a raw exposure of 9.9 g d acquired at an above-ground facility. This work illustrates the scientific potential of detectors with athermal phonon sensors with eV-scale energy resolution for future dark matter searches.
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Affiliation(s)
- I Alkhatib
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - D W P Amaral
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - T Aralis
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - T Aramaki
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - I J Arnquist
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - I Ataee Langroudy
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - E Azadbakht
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - S Banik
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India
| | - D Barker
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C Bathurst
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - D A Bauer
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - L V S Bezerra
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - R Bhattacharyya
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - T Binder
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - M A Bowles
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - P L Brink
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - R Bunker
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - B Cabrera
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - R Calkins
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - R A Cameron
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - C Cartaro
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - D G Cerdeño
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
- Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, 28049 Madrid, Spain
| | - Y-Y Chang
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - M Chaudhuri
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India
| | - R Chen
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - N Chott
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - J Cooley
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - H Coombes
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - J Corbett
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - P Cushman
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F De Brienne
- Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada
| | - M L di Vacri
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - M D Diamond
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - E Fascione
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - E Figueroa-Feliciano
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - C W Fink
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - K Fouts
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - M Fritts
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - G Gerbier
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - R Germond
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - M Ghaith
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - S R Golwala
- Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, California 91125, USA
| | - H R Harris
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
- Department of Electrical and Computer Engineering, Texas A&M University, College Station, Texas 77843, USA
| | - N Herbert
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - B A Hines
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - M I Hollister
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - Z Hong
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - E W Hoppe
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - L Hsu
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - M E Huber
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
- Department of Electrical Engineering, University of Colorado Denver, Denver, Colorado 80217, USA
| | - V Iyer
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India
| | - D Jardin
- Department of Physics, Southern Methodist University, Dallas, Texas 75275, USA
| | - A Jastram
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - V K S Kashyap
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India
| | - M H Kelsey
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - A Kubik
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - N A Kurinsky
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - R E Lawrence
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - A Li
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - B Loer
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - E Lopez Asamar
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - P Lukens
- Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
| | - D MacDonell
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - D B MacFarlane
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - R Mahapatra
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - V Mandic
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - N Mast
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A J Mayer
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | | | - É M Michaud
- Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada
| | - E Michielin
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - N Mirabolfathi
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - B Mohanty
- School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India
| | - J D Morales Mendoza
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - S Nagorny
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - J Nelson
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - H Neog
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - V Novati
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - J L Orrell
- Pacific Northwest National Laboratory, Richland, Washington 99352, USA
| | - S M Oser
- Department of Physics & Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - W A Page
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - P Pakarha
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - R Partridge
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - R Podviianiuk
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - F Ponce
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - S Poudel
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - M Pyle
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - W Rau
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
| | - E Reid
- Department of Physics, Durham University, Durham DH1 3LE, United Kingdom
| | - R Ren
- Department of Physics & Astronomy, Northwestern University, Evanston, Illinois 60208-3112, USA
| | - T Reynolds
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - A Roberts
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - A E Robinson
- Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada
| | - T Saab
- Department of Physics, University of Florida, Gainesville, Florida 32611, USA
| | - B Sadoulet
- Department of Physics, University of California, Berkeley, California 94720, USA
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - J Sander
- Department of Physics, University of South Dakota, Vermillion, South Dakota 57069, USA
| | - A Sattari
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - R W Schnee
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - S Scorza
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
| | - B Serfass
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - D J Sincavage
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C Stanford
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J Street
- Department of Physics, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
| | - D Toback
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - R Underwood
- TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
- Department of Physics, Queen's University, Kingston, Ontario K7L 3N6, Canada
| | - S Verma
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - A N Villano
- Department of Physics, University of Colorado Denver, Denver, Colorado 80217, USA
| | - B von Krosigk
- Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
| | - S L Watkins
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - L Wills
- Département de Physique, Université de Montréal, Montréal, Quebec H3C 3J7, Canada
| | - J S Wilson
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - M J Wilson
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
- Institut für Experimentalphysik, Universität Hamburg, 22761 Hamburg, Germany
| | - J Winchell
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - D H Wright
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - S Yellin
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - B A Young
- Department of Physics, Santa Clara University, Santa Clara, California 95053, USA
| | - T C Yu
- SLAC National Accelerator Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Menlo Park, California 94025, USA
| | - E Zhang
- Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada
| | - H G Zhang
- School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - X Zhao
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - L Zheng
- Department of Physics and Astronomy, and the Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - J Camilleri
- Department of Physics, University of California, Berkeley, California 94720, USA
| | - Yu G Kolomensky
- Department of Physics, University of California, Berkeley, California 94720, USA
- Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - S Zuber
- Department of Physics, University of California, Berkeley, California 94720, USA
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11
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Abstract
In the direct detection of the galactic dark matter, experiments using cryogenic solid-state detectors or noble liquids play for years a very relevant role, with increasing target mass and more and more complex detection systems. But smaller projects, based on very sensitive, advanced detectors following new technologies, could help in the exploration of the different proposed dark matter scenarios too. There are experiments focused on the observation of distinctive signatures of dark matter, like an annual modulation of the interaction rates or the directionality of the signal; other ones are intended to specifically investigate low mass dark matter candidates or particular interactions. For this kind of dark matter experiments at small scale, the physics case will be discussed and selected projects will be described, summarizing the basics of their detection methods and presenting their present status, recent results and prospects.
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