Authors

I. Alkhatib
D. W. P. Amaral
T. Aralis
T. Aramaki
I. Ataee Langroudy
E. Azadbakht
S. Banik
D. Parker
C. Bathurst
D. A. Bauer
L.V.S. Bezerra
R. Bhattacharyya
T. Binder
M. A. Bowles
P. L. Brink
R. Bunker
B. Cabrera
R. Calkins
R. A. Cameron
C. Cartaro
D. G. Cerdeño
Y. -Y. Chang
M. Chaudhuri
R. Chen
N. Chott
J. Cooley
H. Coombes
J. Corbett
P. Cushman
F. De Brienne
M. L. di Vacri
M. D. Diamond
E. Fascione
E. Figueroa-Feliciano
C. W. Fink
K. Fouts
M. Fritts
G. Gerbier
R. Germond
M. Ghaith
S. R. Golwala
H. R. Harris
N. Herbert
B. A. Hines
M. I. Hollister
Z. Hong
E. W. Hoppe
L Hsu
M. E. Huber
V. Iyer
D. Jardin
A. Jastram
V. K. S. Kashyap
M. H. Kelsey
A. Kubik
N. A. Kurinsky
R. E. Lawrence
A. Li
B. Loer
E. Lopez Asamar
P. Lukens
D. MacDonell
D. B. MacFarlane
R. Mahapatra
V. Mandic
N. Mast
A. J. Mayer
H. Meyer zu Theenhausen
É. M. Michaud
E. Michielin
N. Mirabolfathi
B. Mohanty
J. D. Morales Mendoza
S. Nagorny
J. Nelson
H. Neog
V. Novati
J. L. Orrell
S. M. Oser
W. A. Page
P. Pakarha
R. Partridge
R. Podviianiuk
F. Ponce
S. Poudel
M. Pyle
W. Rau
E. Reid
R. Ren
T. Reynolds
A. Roberts
A. E. Robinson
T. Saab
B. Sadoulet
J. Sander
A. Sattari
R. W. Schnee
S. Scorza
B. Serfass
D. J. Sincavage
C. Stanford
J. Street
D. Toback
R. Underwood
S. Verma
A. N. Villano
B. von Krosigk
S. L. Watkins
L. Willis
J. S. Wilson
M. J. Wilson
J. Winchell
D. H. Wright
S. Yellin
Betty A. Young, Santa Clara UniversityFollow
T. C. Yu
E. Zhang
H. G. Zhang
X. Zhao
L. Zheng
J. Camilleri
Yu G. Kolomensky
S. Zuber

Document Type

Article

Publication Date

8-4-2021

Publisher

American Physical Society

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 𝜎𝐸=3.86±0.04⁢(stat)+0.19−0.00⁢(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/𝑐2, 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.

Comments

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.

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