Precision cosmology and 7Li data
  At variance from 2H, 3He and 4He abundances, 7Li abundance data yield an
extra constraint to cosmological parameters, in top of those deriving from CMB,
BAO, SNIa or H0 data. This constraint, often disregarded, would favor smaller
$\Omega_b h^2$ values, also indicating a preference for Dark Energy state
equations well in the phantom regime, simultaneously softening the upper limit
on the sum of neutrino masses, up to ~1.6eV.
