Model independent measurement of the growth rate from the consistency
  relations of the LSS
  The Consistency Relations for the Large Scale Structure provide a link
between the amplitude of Baryonic Acoustic Oscillations in the squeezed
bispectrum (BS) and in the power spectrum (PS). This relation depends on the
large scale bias of the considered tracer, $b_\alpha$, and on the growth rate
of structures, $f$. Remarkably, originating from basic symmetry principles,
this relation is exact and independent on the underlying cosmological model.
  By analysing data from large volume simulations, both for dark matter and for
haloes, we illustrate how BS and PS measurements can be used to extract
$b_\alpha$ and $f$ without the need of any theoretical approximation scheme for
the computation of the BS and the PS. We show that, combining measurements of
the squeezed BS with the quadrupole to monopole ratios for the PS at large
scales can successfully break the $b_\alpha -f$ degeneracy. We forecast that
this method, applied to a Euclid-like survey, will be able to measure bias, and
then the growth rate, at better than $10\%$ level, with no extra assumption.
