Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground

I. Alkhatib; D. W.P. Amaral; T. Aralis; T. Aramaki; I. J. Arnquist; I. Ataee Langroudy; E. Azadbakht; S. Banik; D. Barker; 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; 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. Wills; J. S. Wilson; M. J. Wilson; J. Winchell; D. H. Wright; S. Yellin; B. A. Young; T. C. Yu; E. Zhang; H. G. Zhang; X. Zhao; L. Zheng; J. Camilleri; Yu G. Kolomensky; S. Zuber

doi:10.1103/PhysRevLett.127.061801

Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground

I. Alkhatib, D. W.P. Amaral, T. Aralis, T. Aramaki, I. J. Arnquist, I. Ataee Langroudy, E. Azadbakht, S. Banik, D. Barker, 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. CameronC. 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, 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. Wills, J. S. Wilson, M. J. Wilson, J. Winchell, D. H. Wright, S. Yellin, B. A. Young, T. C. Yu, E. Zhang, H. G. Zhang, X. Zhao, L. Zheng, J. Camilleri, Yu G. Kolomensky, S. Zuber

^*Corresponding author for this work

Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

28 Scopus citations

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)-0.00+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/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.

Original language	English (US)
Article number	061801
Journal	Physical review letters
Volume	127
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevLett.127.061801
State	Published - Aug 6 2021

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1103/PhysRevLett.127.061801

Cite this

Alkhatib, I., Amaral, D. W. P., Aralis, T., Aramaki, T., Arnquist, I. J., Ataee Langroudy, I., Azadbakht, E., Banik, S., Barker, D., Bathurst, C., Bauer, D. A., Bezerra, L. V. S., Bhattacharyya, R., Binder, T., Bowles, M. A., Brink, P. L., Bunker, R., Cabrera, B., Calkins, R., ... Zuber, S. (2021). Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground. Physical review letters, 127(6), [061801]. https://doi.org/10.1103/PhysRevLett.127.061801

@article{2ac5746aa5764f08ba10f3b960034024,

title = "Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground",

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)-0.00+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/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.",

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

note = "Funding Information: Funding and support were received from the National Science Foundation, the U.S. Department of Energy (DOE), Fermilab URA Visiting Scholar Grant No. 15-S-33, NSERC Canada, the Canada First Excellence Research Fund, the Arthur B. McDonald Institute (Canada), Michael M. Garland, the Department of Atomic Energy Government of India (DAE), and the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)—Project No. 420484612 and under Germany{\textquoteright}s Excellence Strategy–EXC 2121 “Quantum Universe”—390833306. Fermilab, PNNL, SLAC, and LBNL are operated under Contracts No. DE-AC02-07CH11359, No. DE-AC05-76RL01830, No. DE-AC02-76SF00515, and No. DE-AC02-05CH11231, respectively, with the U.S. Department of Energy. Publisher Copyright: {\textcopyright} 2021 authors. Published by the American Physical Society.",

year = "2021",

month = aug,

day = "6",

doi = "10.1103/PhysRevLett.127.061801",

language = "English (US)",

volume = "127",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "6",

}

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, M, 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 2021, 'Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground', Physical review letters, vol. 127, no. 6, 061801. https://doi.org/10.1103/PhysRevLett.127.061801

TY - JOUR

T1 - Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground

AU - Alkhatib, I.

AU - Amaral, D. W.P.

AU - Aralis, T.

AU - Aramaki, T.

AU - Arnquist, I. J.

AU - Ataee Langroudy, I.

AU - Azadbakht, E.

AU - Banik, S.

AU - Barker, D.

AU - Bathurst, C.

AU - Bauer, D. A.

AU - Bezerra, L. V.S.

AU - Bhattacharyya, R.

AU - Binder, T.

AU - Bowles, M. A.

AU - Brink, P. L.

AU - Bunker, R.

AU - Cabrera, B.

AU - Calkins, R.

AU - Cameron, R. A.

AU - Cartaro, C.

AU - Cerdeño, D. G.

AU - Chang, Y. Y.

AU - Chaudhuri, M.

AU - Chen, R.

AU - Chott, N.

AU - Cooley, J.

AU - Coombes, H.

AU - Corbett, J.

AU - Cushman, P.

AU - De Brienne, F.

AU - Di Vacri, M. L.

AU - Diamond, M. D.

AU - Fascione, E.

AU - Figueroa-Feliciano, E.

AU - Fink, C. W.

AU - Fouts, K.

AU - Fritts, M.

AU - Gerbier, G.

AU - Germond, R.

AU - Ghaith, M.

AU - Golwala, S. R.

AU - Harris, H. R.

AU - Herbert, N.

AU - Hines, B. A.

AU - Hollister, M. I.

AU - Hong, Z.

AU - Hoppe, E. W.

AU - Hsu, L.

AU - Huber, M. E.

AU - Iyer, V.

AU - Jardin, D.

AU - Jastram, A.

AU - Kashyap, V. K.S.

AU - Kelsey, M. H.

AU - Kubik, A.

AU - Kurinsky, N. A.

AU - Lawrence, R. E.

AU - Li, A.

AU - Loer, B.

AU - Lopez Asamar, E.

AU - Lukens, P.

AU - MacDonell, D.

AU - MacFarlane, D. B.

AU - Mahapatra, R.

AU - Mandic, V.

AU - Mast, N.

AU - Mayer, A. J.

AU - Meyer Zu Theenhausen, H.

AU - Michaud, M.

AU - Michielin, E.

AU - Mirabolfathi, N.

AU - Mohanty, B.

AU - Morales Mendoza, J. D.

AU - Nagorny, S.

AU - Nelson, J.

AU - Neog, H.

AU - Novati, V.

AU - Orrell, J. L.

AU - Oser, S. M.

AU - Page, W. A.

AU - Pakarha, P.

AU - Partridge, R.

AU - Podviianiuk, R.

AU - Ponce, F.

AU - Poudel, S.

AU - Pyle, M.

AU - Rau, W.

AU - Reid, E.

AU - Ren, R.

AU - Reynolds, T.

AU - Roberts, A.

AU - Robinson, A. E.

AU - Saab, T.

AU - Sadoulet, B.

AU - Sander, J.

AU - Sattari, A.

AU - Schnee, R. W.

AU - Scorza, S.

AU - Serfass, B.

AU - Sincavage, D. J.

AU - Stanford, C.

AU - Street, J.

AU - Toback, D.

AU - Underwood, R.

AU - Verma, S.

AU - Villano, A. N.

AU - Von Krosigk, B.

AU - Watkins, S. L.

AU - Wills, L.

AU - Wilson, J. S.

AU - Wilson, M. J.

AU - Winchell, J.

AU - Wright, D. H.

AU - Yellin, S.

AU - Young, B. A.

AU - Yu, T. C.

AU - Zhang, E.

AU - Zhang, H. G.

AU - Zhao, X.

AU - Zheng, L.

AU - Camilleri, J.

AU - Kolomensky, Yu G.

AU - Zuber, S.

N1 - Funding Information: Funding and support were received from the National Science Foundation, the U.S. Department of Energy (DOE), Fermilab URA Visiting Scholar Grant No. 15-S-33, NSERC Canada, the Canada First Excellence Research Fund, the Arthur B. McDonald Institute (Canada), Michael M. Garland, the Department of Atomic Energy Government of India (DAE), and the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)—Project No. 420484612 and under Germany’s Excellence Strategy–EXC 2121 “Quantum Universe”—390833306. Fermilab, PNNL, SLAC, and LBNL are operated under Contracts No. DE-AC02-07CH11359, No. DE-AC05-76RL01830, No. DE-AC02-76SF00515, and No. DE-AC02-05CH11231, respectively, with the U.S. Department of Energy. Publisher Copyright: © 2021 authors. Published by the American Physical Society.

PY - 2021/8/6

Y1 - 2021/8/6

N2 - 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)-0.00+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/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.

AB - 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)-0.00+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/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.

UR - http://www.scopus.com/inward/record.url?scp=85112360072&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85112360072&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.127.061801

DO - 10.1103/PhysRevLett.127.061801

M3 - Article

C2 - 34420312

AN - SCOPUS:85112360072

VL - 127

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 6

M1 - 061801

ER -

Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this