Abstract
We investigate the application of Hybrid Effective Field Theory (HEFT) --
which combines a Lagrangian bias expansion with subsequent particle dynamics
from $N$-body simulations -- to the modeling of $k$-Nearest Neighbor Cumulative
Distribution Functions ($kNN$-$CDF$s) of biased tracers of the
cosmological matter field. The $kNN$-$CDF$s are sensitive to all
higher order connected $N$-point functions in the data, but are computationally
cheap to compute. We develop the formalism to predict the $kNN$-$\rm
CDF$s of discrete tracers of a continuous field from the statistics of the
continuous field itself. Using this formalism, we demonstrate how $k\rm
NN$-$CDF$ statistics of a set of biased tracers, such as halos or
galaxies, of the cosmological matter field can be modeled given a set of
low-redshift HEFT component fields and bias parameter values. These are the
same ingredients needed to predict the two-point clustering. For a specific
sample of halos, we show that both the two-point clustering and the
$kNN$-$CDF$s can be well-fit on quasi-linear scales ($20
h^-1Mpc$) by the second-order HEFT formalism with the same
values of the bias parameters, implying that joint modeling of the two is
possible. Finally, using a Fisher matrix analysis, we show that including
$kNN$-$CDF$ measurements over the range of allowed scales in the
HEFT framework can improve the constraints on $\sigma_8$ by roughly a factor of
$3$, compared to the case where only two-point measurements are considered.
Combining the statistical power of $kNN$ measurements with the modeling
power of HEFT, therefore, represents an exciting prospect for extracting
greater information from small-scale cosmological clustering.
Description
Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
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