The bacco simulation project: bacco hybrid Lagrangian bias expansion model in redshift space
Monthly Notices of the Royal Astronomical Society(2022)
摘要
We present an emulator that accurately predicts the power spectrum of galaxies in redshift space as a function of cosmological parameters. Our emulator is based on a second-order Lagrangian bias expansion that is displaced to Eulerian space using cosmological N-body simulations. Redshift space distortions are then imprinted using the non-linear velocity field of simulated particles and haloes. We build the emulator using a forward neural network trained with the simulations of the BACCO project, which covers an eight-dimensional parameter space including massive neutrinos and dynamical dark energy. We show that our emulator provides unbiased cosmological constraints from the monopole, quadrupole, and hexadecapole of a mock galaxy catalogue that mimics the BOSS-CMASS sample down to non-linear scales (
$k\sim 0.6{h\, {\rm Mpc}^{-1}}$
). This work opens up the possibility of robustly extracting cosmological information from small scales using observations of the large-scale structure of the universe.
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关键词
cosmology: theory,large-scale structure of Universe,methods: statistical,methods: numerical
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