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Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory

, , and . (2021)cite arxiv:2107.10287Comment: To be submitted to MNRAS.

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.

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Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory

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