Neutrino-induced hyperon final-state interactions as constraints on the in-medium hyperon potential
Abstract
Hyperon single-particle potentials control propagation in nuclei and hyperon onset in dense matter, where they soften the neutron-star equation of state and reduce the maximum mass -- the ``hyperon puzzle''. We show that charged-current accelerator (anti)neutrino interactions on Ar, producing and inside the nucleus, can constrain these potentials. At SBND and DUNE energies, the trapped- fraction and escaping-hyperon momenta vary monotonically with and , with a kaon-vetoed FSI- tag adding sensitivity. Inserted in a GM1 relativistic mean-field equation of state at established hypernuclear/-atom depths, the same potentials give and , below the heaviest pulsars and above the GW170817 bound typical of GM1-class mean fields. A detector-level Fisher forecast yields MeV and -MeV for fixed low-density exponent . Since hyperons are produced below saturation, and are 99.8\% anti-correlated; marginalising over degrades the anchor to MeV (MeV with a prior), while is unchanged. For , comparable systematics arise from hyperon-nucleon final-state cross sections (MeV) and the exit-shift/gradient transport prescription (MeV). For , the same uncertainty biases the fit by MeV; removing the tag does not cure this, because the momentum spectrum carries most information and is itself -sensitive. The low-density anchor is a robust handle, at several-MeV rather than sub-MeV precision. A joint fit with terrestrial and heavy-ion priors gives Msun, set mainly by the external prior.
Keywords
Cite
@article{arxiv.2607.09273,
title = {Neutrino-induced hyperon final-state interactions as constraints on the in-medium hyperon potential},
author = {Jaroslaw Nowak},
journal= {arXiv preprint arXiv:2607.09273},
year = {2026}
}
Comments
18 pages, 17 figures