Direct and Indirect Singlet Scalar Dark Matter Detection in the Lepton-Specific two-Higgs-doublet Model

TL;DR

This paper investigates light scalar dark matter within the Lepton-Specific two-Higgs-doublet Model, analyzing its detection prospects through gamma-ray signals and direct detection experiments, and identifying models consistent with observed gamma-ray excesses.

Contribution

It provides a detailed calculation of nucleon-dark matter cross sections in the 2HDM-L framework and explores how direct detection can constrain gamma-ray based dark matter interpretations.

Findings

Models with correct relic abundance can explain the Galactic Center gamma-ray excess.

Some models have direct detection cross sections compatible with recent experimental anomalies.

The study links gamma-ray observations with direct detection constraints within the 2HDM-L framework.

Abstract

A recent study of gamma-ray data from the Galactic Center motivates the investigation of light (~7-10 GeV) particle dark matter models featuring tau lepton pairs as dominant annihilation final state. The Lepton-Specific two-Higgs-doublet Model (2HDM-L) provides a natural framework where light, singlet scalar dark matter can pair-annihilate dominantly into tau leptons. We calculate the nucleon-dark matter cross section for singlet scalar dark matter within the 2HDM-L framework, and compare with recent results from direct detection experiments. We study how direct dark matter searches can be used to constrain the dark matter interpretation of gamma ray observations, for different dominant annihilation final states. We show that models exist with the correct thermal relic abundance that could fit the claimed gamma-ray excess from the Galactic Center region and have direct detection cross sections of the order of what needed to interpret recent anomalous events reported by direct detection experiments.