Abstract

The elastic scattering of an atomic nucleus plays a central role in dark matter direct detection experiments. In those experiments, it is usually assumed that the atomic electrons around the nucleus of the target material immediately follow the motion of the recoil nucleus. In reality, however, it takes some time for the electrons to catch up, which results in ionization and excitation of the atoms. In previous studies, those effects are taken into account by using the so-called Migdal’s approach, in which the final state ionization/excitation are treated separately from the nuclear recoil. In this paper, we reformulate the Migdal’s approach so that the “atomic recoil” cross section is obtained coherently, where we make transparent the energy-momentum conservation and the probability conservation. We show that the final state ionization/excitation can enhance the detectability of rather light dark matter in the GeV mass range via the nuclear scattering. We also discuss the coherent neutrino-nucleus scattering, where the same effects are expected.

Highlights

  • Among various candidates for dark matter, the weakly interacting massive particles (WIMPs) are the most extensively studied category of dark matter

  • As we have shown in the previous sections, a nuclear recoil is accompanied by the ionization and the excitation of the atom through the Migdal effect

  • We reformulated the Migdal effect at the nuclear recoil caused by a dark matter scattering and a coherent neutrino-nuclear scattering

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Summary

Energy eigenstates of atomic system

As we will see the plane wave function of a whole atomic system plays a central role to obtain the nuclear scattering cross section with the Migdal effect. The plane wave function of a whole atomic system plays a central role to obtain the nuclear scattering cross section with the Migdal effect. We consider an isolated neutral atom consisting of a nucleus and Ne electrons. The electrons are not necessarily bounded by the Coulomb potential of the nucleus, and the energy eigenstates can be ionic states with unbouded electrons. As typical nuclear recoil energy is smaller than O(100) keV, the Hamiltonian of the system is well approximated by the non-relativistic one,

H A p 2N 2mN
Energy eigenstates of a moving atom
Isolated nuclear recoil
Invariant amplitudes with electron cloud
Phase space integration
Atomic recoil spectrum
Single electron wave function
Ionization spectrum at the leading order
Numerical analysis
Transition probabilities
Effects on dark matter direct detection
Migdal effects on the recoil spectrum
Migdal effects in coherent neutrino-nucleus scattering
Conclusions and discussion
A The normalization of the projection operator
B Probability conservation and occupied-occupied transition
Findings
C Dirac-Hartree-Fock method
Full Text
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