Diamond detectors for direct detection of sub-GeV dark matter

被引:88
|
作者
Kurinsky, Noah [1 ,2 ]
Yu, To Chin [3 ,4 ]
Hochberg, Yonit [5 ]
Cabrera, Blas [3 ]
机构
[1] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
[2] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[4] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[5] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
基金
以色列科学基金会;
关键词
OPTICAL-PROPERTIES; IMPURITIES; SCATTERING; MOBILITY; PHONONS; FILMS;
D O I
10.1103/PhysRevD.99.123005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose using high-purity lab-grown diamond crystal for the detection of sub-giga electron volt dark matter. Diamond targets can be sensitive to both nuclear and electron recoils from dark matter scattering in the mega-electron-volt and above mass range as well as to absorption processes of dark matter with masses between sub-electron volts to tens of electron volts. Compared to other proposed semiconducting targets such as germanium and silicon, diamond detectors can probe lower dark matter masses via nuclear recoils due to the lightness of the carbon nucleus. The expected reach for electron recoils is comparable to that of germanium and silicon, with the advantage that dark counts are expected to be under better control. Via absorption processes, unconstrained QCD axion parameter space can be successfully probed in diamond for masses of order 10 eV, further demonstrating the power of our approach.
引用
收藏
页数:19
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