# Direct Detection of Bound States of Asymmetric Dark Matter

## TL;DR

This paper evaluates the capabilities of various direct detection experiments to identify large bound states of asymmetric dark matter, emphasizing the importance of energy thresholds and experimental design for detecting extended or light-mediator dark matter.

## Contribution

It provides a comprehensive analysis of detection strategies for large dark matter bound states, highlighting the roles of energy thresholds and experimental setups in sensitivity.

## Key findings

- Large exposure, low-threshold experiments are most effective for point-like dark matter.
- Sensitivity decreases for extended dark states or light mediators in high-threshold experiments.
- Low-threshold, low-exposure experiments with superfluid helium or superconductors can be more sensitive to certain dark states.

## Abstract

We study the reach of direct detection experiments for large bound states (containing $10^4$ or more dark nucleons) of Asymmetric Dark Matter. We consider ordinary nuclear recoils, excitation of collective modes (phonons), and electronic excitations, paying careful attention to the impact of the energy threshold of the experiment. Large exposure experiments with keV energy thresholds provide the best (future) limits when the Dark Matter is small enough to be treated as a point particle, but rapidly lose sensitivity for more extended dark bound states, or when the mediator is light. In those cases, low threshold, low exposure experiments (such as with a superfluid helium, polar material or superconducting target) are often more sensitive due to coherent enhancement over the dark nucleons. We also discuss indirect constraints on composite Asymmetric Dark Matter arising from self-interaction, formation history and the properties of the composite states themselves.