We present the first search for evidence of neutrino self-interaction with two new, state-of-the-art likelihoods for eBOSS Lyman-$\alpha$ data. These are an effective field theory (EFT) likelihood with priors from the Sherwood simulation suite, and a compressed likelihood derived from an emulator built using the PRIYA simulation suite. Previous analyses that combined Planck measurements with eBOSS Lyman-$\alpha$ likelihoods based on earlier simulations found a preference for neutrino self-interactions. In contrast, using either of the new eBOSS Lyman-$\alpha$ likelihoods, we find that a joint analysis with the cosmic microwave background (CMB) data from Planck prefers a negligible level of neutrino self-interaction, and derive new constraints on the neutrino self-coupling: $\mathrm{ log}_{ 10}(G_\mathrm{ eff} \ \mathrm{ MeV}^2)=-5.57_{ -0.58}^{ +0.98}$ for Planck + EFT Lyman-$\alpha$, and $\mathrm{ log}_{ 10}(G_\mathrm{ eff} \ \mathrm{ MeV}^2)=-5.16_{ -0.67}^{ +1.12}$ for Planck + PRIYA Lyman-$\alpha$, at 68% confidence. We also consider Planck in combination with DESI BAO data, and find that the latter does not provide significant constraining power for neutrino self-interactions.
Categories: astro-ph.CO