# Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies

## TL;DR

This study explores low surface brightness galaxies as new targets for dark matter detection, analyzing gamma-ray data to set constraints on dark matter annihilation, and forecasts improved sensitivity with future detections.

## Contribution

It introduces LSBGs as novel targets for dark matter searches and provides initial gamma-ray constraints using Subaru and Fermi data.

## Key findings

- No gamma-ray excess detected in 8 LSBGs.
- Constraints set on dark matter annihilation cross-section at 10^-23 cm^3/s.
- Future LSBG detections could improve sensitivity to 3*10^-25 cm^3/s.

## Abstract

Searches for dark matter annihilation signals have been carried out in a number of target regions such as the Galactic Center and Milky Way dwarf spheroidal galaxies (dSphs), among a few others. Here we propose low surface brightness galaxies (LSBGs) asnovel targets for the indirect detection of dark matter emission. In particular, LSBGs are known to have very large dark matter contents and be less contaminated by extragalactic gamma-ray sources (e.g., blazars) compared to star forming galaxies. We report on an analysis that uses eight LSBGs (detected by Subaru Hyper Suprime-Cam survey data) with known redshifts to conduct a search for gamma-ray emission at the positions of these new objects in Fermi Large Area Telescope data. We found no excesses of gamma-ray emission and set constraints on the dark matter annihilation cross-section. We exclude (at the 95% C.L.) dark matter scenarios predicting a cross-section higher than 10^-23[cm^3/s] for dark matter particles of mass 10 GeV self-annihilating in the b_b channel. Although this constraint is weaker than the ones reported in recent studies using other targets, we note that in the near future, the number of detections of new LSBGs will increase by a few orders of magnitude. We forecast that with the use of the full catalog of soon-to-be-detected LSBGs the constraint will reach cross-section sensitivities of ~ 3*10^-25 [cm^3/s] for dark matter particles with masses less than 10 GeV.