Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground
- Alkhatib, I;
- Amaral, DWP;
- Aralis, T;
- Aramaki, T;
- Arnquist, IJ;
- Langroudy, I Ataee;
- 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, Y-Y;
- 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;
- Asamar, E Lopez;
- Lukens, P;
- MacDonell, D;
- MacFarlane, DB;
- Mahapatra, R;
- Mandic, V;
- Mast, N;
- Mayer, AJ;
- Theenhausen, H Meyer zu;
- Michaud, ÉM;
- Michielin, E;
- Mirabolfathi, N;
- Mohanty, B;
- Mendoza, JD Morales;
- 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, Yu G;
- Zuber, S
- et al.
Published Web Location
https://journals.aps.org/prl/pdf/10.1103/PhysRevLett.127.061801Abstract
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.
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.