Shu-Hua Yang, Fridolin Weber

In this Letter, we study the structure of the strange stars admixed with bosonic dark matter, and find that these stars can well explain the mass and radius observations of XTE J1814-338. We also find that for the strong interaction coupling constant $\alpha_{S}=0.6$ and $B^{1/4}=135$ MeV ($B$ is the bag constant), the observations of XTE J1814-338 constrain the mass of the bosonic dark matter to $m_{\chi}\leq 307 (\lambda /\pi)^{1/4}$ MeV ($\lambda$ is the dimensionless coupling constant of the bosonic dark matter).