Visible Sterile Neutrinos as the Earliest Relic Probes of Cosmology
Graciela B. Gelmini, Philip Lu, Volodymyr Takhistov

TL;DR
This paper explores how sterile neutrinos could serve as early universe probes, especially under non-standard pre-BBN cosmologies, and discusses their detectability in upcoming experiments.
Contribution
It demonstrates that non-standard pre-BBN cosmologies weaken existing constraints on sterile neutrinos, making certain signals more accessible for upcoming laboratory detection.
Findings
Sterile neutrino signals are compatible with non-standard cosmologies.
Current cosmological limits on active-sterile mixing are not robust.
Upcoming experiments can test sterile neutrino models in these alternative cosmologies.
Abstract
A laboratory detection of a sterile neutrino could provide the first indication of the evolution of the Universe before Big-Bang Nucleosynthesis (BBN), an epoch yet untested. Such "visible" sterile neutrinos are observable in upcoming experiments such as KATRIN/TRISTAN and HUNTER in the keV mass range and PTOLEMY and others in the eV mass range. A set of standard assumptions is typically made about cosmology before the temperature of the Universe was 5 MeV. However, non-standard pre-BBN cosmologies based on alternative assumptions could arise in motivated theoretical models and are equally in agreement with all existing data. We revisit the production of sterile neutrinos of mass 0.01 eV to 1 MeV in two examples of such models: scalar-tensor and low reheating temperature pre-BBN cosmologies. In both of them, the putative 3.5 keV X-ray signal line corresponds to a sterile neutrino with a…
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