Toward alleviating the H0 and S8 tensions with early dark energy-dark matter drag

Simon, Théo (ORCID:0000000178586441); Adi, Tal (ORCID:0000000257639353); Bernal, José_Luis (ORCID:0000000209614653); Kovetz, Ely_D (ORCID:0000000192561144); Poulin, Vivian (ORCID:0000000291175257); Smith, Tristan_L (ORCID:0000000326855405)

doi:10.1103/PhysRevD.111.023523

Experimental bounds on the neutrino lifetime depend on the nature of the neutrinos and the details of the potentially new physics responsible for neutrino decay. In the case where the decays involve active neutrinos in the final state, the neutrino masses also qualitatively impact how these manifest themselves experimentally. In order to further understand the impact of nonzero neutrino masses, we explore how observations of solar neutrinos constrain a very simple toy model. We assume that neutrinos are Dirac fermions and there is a new massless scalar that couples to neutrinos such that a heavy neutrino—

ν_{2}

with mass

m_{2}

—can decay into a lighter neutrino—

ν_{1}

with mass

m_{1}

—and a massless scalar. We find that the constraints on the new physics coupling depend, sometimes significantly, on the ratio of the daughter-to-parent neutrino masses and that, for large-enough values of the new physics coupling, the “dark side” of the solar neutrino parameter space—

\sin^{2} θ_{12} \sim 0.7

—provides a reasonable fit to solar neutrino data, if only

{}^{8}B

or

{}^{7}{Be}

neutrino data alone are considered, but no allowed region is found in the combined analysis. Our results generalize to other neutrino-decay scenarios, including those that mediate

ν_{2} \to ν_{1} {\bar{ν}}_{3} ν_{3}

when the neutrino mass ordering is inverted mass and

m_{2} > m_{1} ≫ m_{3}

, the mass of

ν_{3}

. Published by the American Physical Society2024

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