# Finite-size dark matter and its effect on small-scale structure

## TL;DR

This paper explores how finite-size dark matter with velocity-dependent self-interactions can address small-scale structure issues in cosmology, highlighting the potential for direct detection experiments to probe such models.

## Contribution

It demonstrates that the velocity dependence of dark matter self-interactions is largely independent of internal structure, providing a new perspective on Puffy Dark Matter models.

## Key findings

- Velocity-dependent cross section can resolve small-scale structure problems.
- Low-threshold direct detection experiments can test Puffy Dark Matter.
- The velocity dependence is robust across different internal structures.

## Abstract

If dark matter has a finite size that is larger than its Compton wavelength, the corresponding self-interaction cross section decreases with the velocity. We investigate the implications of this Puffy Dark Matter for addressing the small-scale problems of the $\Lambda$CDM model. In particular, we show that the way the non-relativistic cross section varies with the velocity is largely independent of the dark matter internal structure when the range of the mediating force is very short. We present an explicit example in the context of a QCD-like theory of dark matter and show that low-threshold direct detection experiments have the potential to probe Puffy Dark Matter.