Daughters mimic sterile neutrinos (almost!) perfectly

Abstract

Since only recently, cosmological observations are sensitive to hot dark matter (HDM) admixtures with sub-eV mass, $m_{\text{hdm}}^{\text{eff}}$ < eV, that are not fully-thermalised, $N_{\text{eff}}$ < 1. We argue that their almost automatic interpretation as a sterile neutrino species is neither from theoretical nor practical parsimony principles preferred over HDM formed by decay products (daughters) of an out-of-equilibrium particle decay. While daughters mimic sterile neutrinos in $N_{\text{eff}}$ and $m_{\text{hdm}}^{\text{eff}}$, there are opportunities to assess this possibility in likelihood analyses. Connecting cosmological parameters and moments of momentum distribution functions, we show that --also in the case of mass-degenerate daughters with indistinguishable main physical effects-- the mimicry breaks down when the next moment, the skewness, is considered. Predicted differences of order one in the root-mean-squares of absolute momenta are too small for current sensitivities.

revtex 12 pages + refs., 7 figures, 1 table

References in corpus (5)

• Massive neutrinos and cosmology
• Dark Radiation Emerging After Big Bang Nucleosynthesis?
• No new cosmological concordance with massive sterile neutrinos
• Dark Matter CMB Constraints and Likelihoods for Poor Particle Physicists
• Leptogenesis, Gravitino Dark Matter and Entropy Production

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• Non-thermal Hot Dark Matter from Inflaton/Moduli Decay: The Momentum Distribution and Relaxing the Cosmological Mass Bound