A tale of two modes: neutrino free-streaming in the early universe

By Lachlan Lancaster, F. Cyr-Racine, Lloyd Knox, Z. Pan. 2017

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We present updated constraints on the free-streaming nature of cosmological neutrinos from cosmic microwave background (CMB) temperature and polarization power spectra, baryonic acoustic oscillation data, and distance ladder measurements of the Hubble constant. Specifically, we consider a Fermi-like four-fermion interaction between massless neutrinos, characterized by an effective coupling constant Geff, and resulting in a neutrino opacity τ̇ν∝ Geff2 Tν5. Using a conservative flat prior on the parameter log 10( Geff MeV2), we find a bimodal posterior distribution with two clearly separated regions of high probability. The first of these modes is consistent with the standard ΛCDM cosmology and corresponds to neutrinos decoupling at redshift zν,dec > 1.3×105, that is before the Fourier modes probed by the CMB damping tail enter the causal horizon. The other mode of the posterior, dubbed the "interacting neutrino mode", corresponds to neutrino decoupling occurring within a narrow redshift window centered around zν,dec∼8300. This mode is characterized by a high value of the effective neutrino coupling constant, log 10( Geff MeV2) = −1.72 ± 0.10 (68% C.L.), together with a lower value of the scalar spectral index and amplitude of fluctuations, and a higher value of the Hubble parameter. Using both a maximum likelihood analysis and the ratio of the two mode's Bayesian evidence, we find the interacting neutrino mode to be statistically disfavored compared to the standard ΛCDM cosmology, and determine this result to be largely driven by the low-l CMB temperature data. Interestingly, the addition of CMB polarization and direct Hubble constant measurements significantly raises the statistical significance of this secondary mode, indicating that new physics in the neutrino sector could help explain the difference between local measurements of H0, and those inferred from CMB data. A robust consequence of our results is that neutrinos must be free streaming long before the epoch of matter-radiation equality in order to fit current cosmological data.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/64ebfd40fdb35e9fe05ec4c554bcee1dbbd86a48

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In Nuclear and High Energy Physics

Citations in the corpus

Cosmology Intertwined II: The Hubble Constant Tension (2020, unknown): “[111] L.”
CMB-S4 Science Case, Reference Design, and Project Plan (2019, background): “A radiation fluid whose fluctuations do not exceed the sound speed of the plasma [179, 180] could arise from large neutrino self-interactions [181, 182, 183, 184, 185], neutrino-dark sector interactions [186, 187], or dark radiation self-coupling [188, 189, 190].”