Scaling of the 1-halo terms with bias
  In the Halo Model, galaxies are hosted by dark matter halos, while the halos
themselves are biased tracers of the underlying matter distribution.
Measurements of galaxy correlation functions include contributions both from
galaxies in different halos, and from galaxies in the same halo (the so-called
1-halo terms). We show that, for highly biased tracers, the 1-halo term of the
power spectrum obeys a steep scaling relation in terms of bias. We also show
that the 1-halo term of the trispectrum has a steep scaling with bias. The
steepness of these scaling relations is such that the 1-halo terms can become
key contributions to the $n$-point correlation functions, even at large scales.
We interpret these results through analytical arguments and semi-analytical
calculations in terms of the statistical properties of halos.
