Exotic Dark Matter Search with the MAJORANA DEMONSTRATOR

被引：2

作者：

Arnquist, I. J. ^{[1
]}

Avignone, F. T. ^{[2
,3
,7
,8
]}

Barabash, A. S. ^{[4
]}

Barton, C. J. ^{[5
,27
,28
]}

Bhimani, K. H. ^{[6
,7
]}

Blalock, E.

Bos, B. ^{[6
,7
]}

Busch, M. ^{[7
,9
]}

Buuck, M. ^{[10
,11
]}

Caldwell, T. S. ^{[6
]}

Chan, Y-D. ^{[12
]}

Christofferson, C. D. ^{[13
]}

Chu, P. -h. ^{[14
]}

Clark, M. L. ^{[6
,7
]}

Cuesta, C. ^{[15
]}

Detwiler, J. A. ^{[10
,11
]}

Efremenko, Yu. ^{[3
,16
]}

Ejiri, H. ^{[17
]}

Elliott, S. R. ^{[14
]}

Giovanetti, G. K. ^{[18
]}

Green, M. P. ^{[3
,7
,8
]}

Gruszko, J. ^{[6
,7
]}

Guinn, I. S.

Guiseppe, V. E. ^{[3
]}

Haufe, C. R. ^{[6
,7
]}

Henning, R. ^{[6
]}

Aguilar, D. Hervas

Hoppe, E. W.

Hostiuc, A. ^{[10
,11
]}

Kidd, M. F. ^{[19
]}

Kim, I. ^{[14
,29
]}

Kouzes, R. T. ^{[1
]}

Lannen, V. T. E. ^{[2
]}

Li, A. ^{[6
,7
,30
]}

Lopez, A. M. ^{[16
]}

Lopez-Castano, J. M. ^{[3
]}

Martin, E. L. ^{[6
,7
,31
,32
]}

Martin, R. D. ^{[20
]}

Massarczyk, R. ^{[14
]}

Meijer, S. J. ^{[14
]}

Mertens, S. ^{[21
,22
,23
]}

Oli, T. K. ^{[5
]}

Othman, G. ^{[6
,7
,33
]}

Paudel, L. S. ^{[3
,5
]}

Pettus, W. ^{[24
,25
]}

Poon, A. W. P. ^{[12
]}

Radford, D. C. ^{[3
,14
]}

Rager, J. ^{[6
,34
]}

Reine, A. L. ^{[6
,7
]}

Rielage, K. ^{[14
]}

机构：

[1] Pacific Northwest Natl Lab, Richland, WA 99354 USA

[2] Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA

[3] Oak Ridge Natl Lab, Oak Ridge, TN 37830 USA

[4] Kurchatov Inst, Inst Theoret & Expt Phys, Natl Res Ctr, Moscow 117218, Russia

[5] Univ South Dakota, Dept Phys, Vermillion, SD 57069 USA

[6] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27514 USA

[7] Triangle Univ Nucl Lab, Durham, NC 27708 USA

[8] North Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA

[9] Duke Univ, Dept Phys, Durham, NC 27708 USA

[10] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA

[11] Univ Washington, Dept Phys, Seattle, WA 98195 USA

[12] Lawrence Berkeley Natl Lab, Nucl Sci Div, Berkeley, CA 94720 USA

[13] South Dakota Mines, Rapid City, SD 57701 USA

[14] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[15] Ctr Invest Energet Medioambientales & Tecnol, CIEMAT, Madrid 28040, Spain

[16] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37916 USA

[17] Osaka Univ, Res Ctr Nucl Phys, Osaka, Ibaraki 5670047, Japan

[18] Williams Coll, Phys Dept, Williamstown, MA 01267 USA

[19] Tennessee Technol Univ, Cookeville, TN 38505 USA

[20] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6, Canada

[21] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[22] Tech Univ, Phys Dept, D-85748 Munich, Germany

[23] Tech Univ, Excellence Cluster Universe, D-85748 Munich, Germany

[24] Indiana Univ, IU Ctr Explorat Energy & Matter, Bloomington, IN 47405 USA

[25] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA

[26] Joint Inst Nucl Res, Dubna 141980, Russia

[27] Roma Tre Univ, Rome, Italy

[28] INFN Roma Tre, Rome, Italy

[29] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

[30] Univ Calif San Diego, La Jolla, CA 92093 USA

[31] Duke Univ, Durham, NC 27708 USA

[32] Argonne Natl Lab, Lemont, IL 60439 USA

[33] Univ Hamburg, Inst Expt Phys, Hamburg, Germany

[34] DEVCOM Army Res Lab Armed Forces, US Army, Adelphi, MD 20783 USA

[35] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

来源：

PHYSICAL REVIEW LETTERS | 2024年 / 132卷 / 04期

基金：

加拿大创新基金会; 加拿大自然科学与工程研究理事会; 美国国家科学基金会;

关键词：

GERMANIUM;

D O I：

10.1103/PhysRevLett.132.041001

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

With excellent energy resolution and ultralow-level radiogenic backgrounds, the high-purity germanium detectors in the MAJORANA DEMONSTRATOR enable searches for several classes of exotic dark matter (DM) models. In this work, we report new experimental limits on keV-scale sterile neutrino DM via the transition magnetic moment from conversion to active neutrinos vs -> va. We report new limits on fermionic dark matter absorption (x +A -> v+ A) and sub-GeV DM-nucleus 3 -> 2 scattering (x + x + A -> phi + A), and new exclusion limits for bosonic dark matter (axionlike particles and dark photons). These searches utilize the (1-100)-keV low-energy region of a 37.5 -kg y exposure collected by the DEMONSTRATOR between May 2016 and November 2019 using a set of 76Ge-enriched detectors whose surface exposure time was carefully controlled, resulting in extremely low levels of cosmogenic activation.

引用

页数：7

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