{ "id": "2406.19279", "version": "v1", "published": "2024-06-27T15:49:37.000Z", "updated": "2024-06-27T15:49:37.000Z", "title": "Probing self-interacting ultra-high-energy neutrinos with cosmic 21-cm signal", "authors": [ "Mansi Dhuria", "Bishnu Gupta Teli" ], "comment": "13 pages, 5 figures", "categories": [ "hep-ph", "astro-ph.CO" ], "abstract": "In this study, we investigate the constraints on secret self-interactions of neutrinos by examining the impact of radiative scattering of ultra-high-energy (UHE) neutrinos. These neutrinos are produced from the decay of superheavy dark matter and interact with the cosmic neutrino background (C$\\nu$B). We explore how these interactions influence the 21-cm hydrogen signal during the cosmic dark ages and cosmic dawn, periods relatively free from astrophysical uncertainties, providing a clearer signal for studying non-standard neutrino interactions. By analyzing the global brightness temperature measurements, we constrain the scattering cross-section of UHE self-interacting neutrinos, determining the coupling constant $g$ to be within $\\sim 10^{-4}$ to $\\sim 10^{-3}$ for neutrino energies in the PeV to EeV range. Interestingly, these constraints are more competitive than those from existing astrophysical and collider experiments. As future 21-cm experiments focus on measuring brightness temperature across a wide range of redshifts from the cosmic dark ages to reionization, using the epoch of 21-cm to probe neutrino properties could provide crucial insights into dark matter and neutrino physics.", "revisions": [ { "version": "v1", "updated": "2024-06-27T15:49:37.000Z" } ], "analyses": { "keywords": [ "probing self-interacting ultra-high-energy neutrinos", "cosmic dark ages", "global brightness temperature measurements", "cosmic neutrino background", "superheavy dark matter" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }