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arXiv:2206.06386·v2·Cosmology and Nongalactic Astrophysics

Observing nulling of primordial correlations via the 21 cm signal

Shyam Balaji🇫🇷 · H. V. Ragavendra🇮🇳 · Shiv K. Sethi🇮🇳 · Joseph Silk🇫🇷 · L. Sriramkumar🇮🇳

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Abstract

The 21cm line emitted by neutral hydrogen (HI) during the Dark Ages carries imprints of pristine primordial correlations. In models of inflation driven by a single, canonical scalar field, we show that a phase of ultra-slow-roll can lead to a null in all the primordial correlations at a specific wavenumber . We consider scenarios wherein the null in the correlations occurs over wavenumbers , and examine the prospects of detecting such a damping in the HI signal due to the nulls at the level of power and bi-spectra in future observational missions.

Comments: v1: 10 pages, 5 figures; v2: 11 pages, 5 figures including supplementary material, published in Phys. Rev. Lett

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