Constraints on freeze-in dark matter from Lyman- forest and 21-cm signal : single-field models
arXiv:2407.08225 · doi:10.1103/PhysRevD.110.115003
Abstract
We report new Lyman- and 21-cm constraints on freeze-in dark matter (FIDM) which injects energy into the intergalactic medium either through annihilation or decay to photon(s) or electron-positron pair. With respect to Lyman- we fix the baseline ionization history using low redshift data about astrophysical reionization, whereas for 21-cm signal we adopt the baseline values of 21-cm power spectrum through a standard modeling of star formation developed so far. Using the latest numerical tools, we show that (i) for sterile neutrino FIDM, current Lyman- data and future sensitivity of SKA-low (1000 hrs) on the 21-cm power spectra excludes the FIDM mass up to GeV at 95 CL and GeV, respectively, and (ii) for millicharged FIDM, current Lyman- data only excludes the millicharge down to within the FIDM mass range of GeV at 95 CL, suggesting that the surviving parameter space of millicharged FIDM is still intact.
17 pages, 5 figures; v2: revised version with 19 pp and 8 figs; v3: to match the published version
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- Lyman- limit on axion-like cold dark matter
- Sensitivity toward dark matter annihilation imprints on 21-cm signal with SKA-Low: A convolutional neural network approach
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