We investigate the incoherent regime of the fermionic dark matter absorption by nuclei using the relativistic Fermi gas model and nuclear form factors. With the momentum transfer being roughly equal to the dark matter mass m_χ, the incoherent regime contributes significantly to the absorption process for m_χ 100 MeV with a spin-independent operator and for even smaller mass with a spin-dependent one. We also compare the situations for various target nuclei (¹³¹Xe, ⁷²Ge, ⁴⁰Ar, ²⁰Ne and ⁴He) that are typically used in the dark matter direct detection. A heavier nucleus actually has the advantage of probing the incoherent scattering of the fermionic absorption dark matter. Observing both the coherent and incoherent contributions would be an important justification of the fermionic dark matter absorption.
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Ge et al. (2024) studied this question.
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