TL;DR
This paper compares various target materials for light dark matter detection across multiple channels, identifying key material properties that influence experimental sensitivity and highlighting promising candidates for future experiments.
Contribution
It provides a comprehensive comparison of target materials for light dark matter detection, emphasizing the importance of specific material parameters in optimizing sensitivity.
Findings
Target material properties like sound speed and band gap are crucial for sensitivity.
Certain materials outperform current proposals for specific dark matter models.
A total of 16 promising polar crystals are evaluated across detection channels.
Abstract
Direct detection experiments for light dark matter are making enormous leaps in reaching previously unexplored model space. Several recent proposals rely on collective excitations, where the experimental sensitivity is highly dependent on detailed properties of the target material, well beyond just nucleus mass numbers as in conventional searches. It is thus important to optimize the target choice when considering which experiment to build. We carry out a comparative study of target materials across several detection channels, focusing on electron transitions and single (acoustic or optical) phonon excitations in crystals, as well as the traditional nuclear recoils. We compare materials currently in use in nuclear recoil experiments (Si, Ge, NaI, CsI, CaWO), a few which have been proposed for light dark matter experiments (GaAs, AlO, diamond), as well as 16 other promising…
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