# First constraints on fuzzy dark matter from Lyman-$\alpha$ forest data and hydrodynamical simulations

## TL;DR

This study uses hydrodynamical simulations and Lyman-alpha forest data to set new lower limits on fuzzy dark matter particle masses, challenging their role in solving small-scale structure problems.

## Contribution

First to employ hydrodynamical simulations with Lyman-alpha data to constrain fuzzy dark matter particle masses.

## Key findings

- Lower mass limits of 7.1×10⁻²² eV and 14.3×10⁻²² eV from two datasets.
- Combined data sets constrain mass to above 20×10⁻²² eV.
- Mass range 1-10×10⁻²² eV ruled out at high significance.

## Abstract

We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman-$\alpha$ forest data. Extremely light bosons with a De Broglie wavelength of $\sim 1$ kpc have been suggested as dark matter candidates that may resolve some of the current small scale problems of the cold dark matter model. For the first time we use hydrodynamical simulations to model the Lyman-$\alpha$ flux power spectrum in these models and compare with the observed flux power spectrum from two different data sets: the XQ-100 and HIRES/MIKE quasar spectra samples. After marginalization over nuisance and physical parameters and with conservative assumptions for the thermal history of the IGM that allow for jumps in the temperature of up to $5000\rm\,K$, XQ-100 provides a lower limit of 7.1$\times 10^{-22}$ eV, HIRES/MIKE returns a stronger limit of 14.3$\times 10^{-22}$ eV, while the combination of both data sets results in a limit of 20 $\times 10^{-22}$ eV (2$\sigma$ C.L.). The limits for the analysis of the combined data sets increases to 37.5$\times 10^{-22}$ eV (2$\sigma$ C.L.) when a smoother thermal history is assumed where the temperature of the IGM evolves as a power-law in redshift. Light boson masses in the range $1-10 \times10^{-22}$ eV are ruled out at high significance by our analysis, casting strong doubts that FDM helps solve the "small scale crisis" of the cold dark matter models.