Probing Small Scale Primordial Power Spectrum with 21cm Line Global Signal
arXiv:1911.07442 · doi:10.1103/PhysRevD.101.083520
Abstract
We argue that the global signal of neutral hydrogen 21cm line can be a powerful probe of primordial power spectrum on small scales. Since the amplitude of small scale primordial fluctuations is important to determine the early structure formation and the timing when the sources of Lyman photons are produced, they in turn affect the neutral hydrogen 21cm line signal. We show that the information of the position of the absorption trough can severely constrain the small scale amplitude of primordial fluctuations once astrophysical parameters relevant to the 21cm line signal are fixed. We also discuss how the uncertainties of astrophysical parameters affect the constraints.
21 pages, 8 figures, one column, accepted for publication in PRD
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- ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
- Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal
- Constraints on Primordial Power Spectrum from Galaxy Luminosity Functions
- Small-scale primordial fluctuations in the 21cm Dark Ages signal
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- Impact of the primordial fluctuation power spectrum on the reionization history
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