2022
DOI: 10.1103/physrevd.106.083009
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Identification of the low-energy excess in dark matter searches with crystal defects

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Cited by 5 publications
(7 citation statements)
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“…Here, we are assuming that the origin of the low-energy excess observed in the low-threshold direct detection experiments is attributed to a controllable background. In a separate study, the authors have elaborated on using phonon-mediated detectors to understand the origin of these events [105]. Figure 7 represents the annual modulation of a dark matter particle with a mass of 300 MeV/c 2 and a cross-section of 10 −39 cm 2 scattering on silicon target over the year 2020.…”
Section: Resultsmentioning
confidence: 99%
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“…Here, we are assuming that the origin of the low-energy excess observed in the low-threshold direct detection experiments is attributed to a controllable background. In a separate study, the authors have elaborated on using phonon-mediated detectors to understand the origin of these events [105]. Figure 7 represents the annual modulation of a dark matter particle with a mass of 300 MeV/c 2 and a cross-section of 10 −39 cm 2 scattering on silicon target over the year 2020.…”
Section: Resultsmentioning
confidence: 99%
“…Semiconductor targets, such as silicon or germanium, can be utilized as cryogenic solidstate ionization detectors, where sensitivity to single electron ionization events has been demonstrated [67][68][69], corresponding to nuclear recoil energy detection threshold of  10 ( ) eV. The ionization threshold is the minimum energy to create a single electron-hole pair excitation via nuclear recoil interaction.…”
Section: Introductionmentioning
confidence: 99%
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“…To quantify how the energy loss effect in diamond can be used to identify the nuclear recoil origin of the spectrum, we have performed a likelihood ratio test for simulated data sets, using the three best fit functions given in table 1 as the physical recoil rate. We obtain the required number of events in a diamond detector in the event selection window eV, using 1 eV bins, for a 3σ observation of the peak/dip feature, as described in more detail in [20]. We find that unless the peak is masked by the exponential noise component, the feature can be observed with just 440 to 710 events in the selection window, depending slightly on the power law index β of the fit parameters.…”
Section: Identifying Nuclear Recoilsmentioning
confidence: 99%
“…Most of the anticipated background sources, such as photons or electrons, would give Figure 1: Energy loss, averaged over recoil direction, as a function of the recoil energy in silicon, germanium, sapphire and diamond. The figure has appeared before in [20].…”
Section: Introductionmentioning
confidence: 98%