Abstract
The matter power spectrum has been strongly constrained by astronomical measurements at large scales, but only weakly at small scales. Compared with the standard scenario, the deviation of the matter power spectrum at small scales has influence on the cosmological structure formation, e.g., the comoving number density of dark matter halos. The thermal history of the intergalactic medium (IGM) can be changed if dark matter is made of weakly interacting massive particles and can annihilate into standard model particles. The changes of the evolution of IGM could leave imprints on the relevant astronomical observations. Taking into account the dark matter annihilation, we investigate the impact of the deviation of matter power spectrum at small scales on the global 21-cm signal. In view of the measurements of the global 21-cm signal by the EDGES experiment, we explore the allowed parameter space of ${m}_{s}$, which describes the degree of deviation, by requiring the differential brightness temperature of the global 21-cm signal $\ensuremath{\delta}{T}_{21}\ensuremath{\le}\ensuremath{-}50\text{ }\text{ }\mathrm{mK}$ at redshift $z=17$.
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