The possibility that the so-called "lithium problem", i.e. the disagreement
between the theoretical abundance predicted for primordial 7Li assuming
standard nucleosynthesis and the value inferred from astrophysical
measurements, can be solved through a non-thermal BBN mechanism has been
investigated by several authors. In particular, it has been shown that the
decay of a MeV-mass particle, like, e.g., a sterile neutrino, decaying after
BBN not only solves the lithium problem, but also satisfies cosmological and
laboratory bounds, making such a scenario worth to be investigated in further
detail. In this paper, we constrain the parameters of the model with the
combination of current data, including Planck 2015 measurements of temperature
and polarization anisotropies of the CMB, FIRAS limits on spectral distortions,
astrophysical measurements of primordial abundances and laboratory constraints.
We find that a sterile neutrino with mass MS=4.35−0.17+0.13MeV (at
95% c.l.), a decay time τS=1.8−1.3+2.5⋅105s (at 95%
c.l.) and an initial density nˉS/nˉcmb=1.7−0.6+3.5⋅10−4 (at 95% c.l.) in units of the number density of CMB photons,
perfectly accounts for the difference between predicted and observed 7Li
primordial abundance. This model also predicts an increase of the effective
number of relativistic degrees of freedom at the time of CMB decoupling ΔNeffcmb≡Neffcmb−3.046=0.34−0.14+0.16 at 95% c.l..
The required abundance of sterile neutrinos is incompatible with the standard
thermal history of the Universe, but could be realized in a low reheating
temperature scenario. We provide forecasts for future experiments finding that
the combination of measurements from the COrE+ and PIXIE missions will allow to
significantly reduce the permitted region for the sterile lifetime and density.Comment: 28 pages, 13 figures, 4 tables, matching the published versio