Information content in mean pairwise velocity and mean relative velocity between pairs in a triplet
arXiv:2102.06709 · doi:10.1051/0004-6361/202140552
Abstract
Velocity field provides a complementary avenue to constrain cosmological information, either through the peculiar velocity surveys or the kinetic Sunyaev Zel'dovich effect. One of the commonly used statistics is the mean radial pairwise velocity. Here, we consider the three-point mean relative velocity, i.e. the mean relative velocities between pairs in a triplet. Using halo catalogs from the Quijote suite of N-body simulations, we first showcase how the analytical prediction for the mean relative velocities between pairs in a triplet achieve better than 4-5% accuracy using standard perturbation theory at leading order for triangular configurations with a minimum separation of Mpc. Furthermore, we present the three-point relative velocity as a novel probe of neutrino mass estimation. We explore the full cosmological information content of the halo mean pairwise velocities, and the mean relative velocities between halo pairs in a triplet. We undertake this through the Fisher-matrix formalism using 22,000 simulations from the Quijote suite, and considering all triangular configurations with a minimum and a maximum separation of Mpc and Mpc, respectively. We find that the mean relative velocities in a triplet allows a 1 neutrino mass () constraint of 0.065 eV, that is roughly 13 times better than the mean pairwise velocity constraint (0.877 eV). This information gain is not limited only to neutrino mass, but extends to other cosmological parameters: , , , and achieving a gain of 8.9, 11.8, 15.5, 20.9 and 10.9 times respectively. These results illustrate the possibility of exploiting the mean three-point relative velocities for constraining the cosmological parameters accurately from future cosmic microwave background experiments and peculiar velocity surveys.
arXiv comment13 pages, 10 figures, accepted for publication in A&A
References in corpus (43)
- The Simons Observatory: Science goals and forecasts
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix
- Status of neutrino oscillations 2018: first hint for normal mass ordering and improved CP sensitivity
- Cosmicflows-3
- Neutrino oscillations refitted
- Global constraints on absolute neutrino masses and their ordering
- Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel'dovich Effect
- Towards an accurate model of the redshift space clustering of halos in the quasilinear regime
- Convolution Lagrangian perturbation theory for biased tracers
- Planck 2018 results. VI. Cosmological parameters
- DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos
- Global Analyses of Neutrino Oscillation Experiments
- The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
- On The Validity of the Streaming Model for the Redshift-Space Correlation Function in the Linear Regime
- Impact of massive neutrinos on nonlinear matter power spectrum
- Evidence for the kinematic Sunyaev-Zeľdovich effect with ACTPol and velocity reconstruction from BOSS
- Cosmological information in the redshift-space bispectrum
- Detection of the kinematic Sunyaev-Zel'dovich effect with DES Year 1 and SPT
- Constraining with the Bispectrum II: The Total Information Content of the Galaxy Bispectrum
- Are peculiar velocity surveys competitive as a cosmological probe?
- An analytic model for redshift-space distortions
- The Gaussian streaming model and Lagrangian effective field theory
- The imprint of neutrinos on clustering in redshift-space
- Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope
- Dark Energy Constraints from Galaxy Cluster Peculiar Velocities
- The Tau of Galaxy Clusters
- Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
- Cosmological Forecasts for Combined and Next Generation Peculiar Velocity Surveys
- Constraints on massive neutrinos from the pairwise kinematic Sunyaev-Zel'dovich effect
- Galaxy redshift-space bispectrum: the Importance of Being Anisotropic
- The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
- Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
- A Lagrangian Perturbation Theory in the presence of massive neutrinos
- An estimation of the Local growth rate from Cosmicflows-3 peculiar velocities
- A Future Test of Gravitation Using Galaxy Cluster Velocities
- Edgeworth streaming model for redshift space distortions
- Information Content of Higher-Order Galaxy Correlation Functions
- Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
- Measuring the evolution of intergalactic gas from z=0 to 5 using the kinematic Sunyaev-Zel'dovich effect
- On the streaming model for redshift-space distortions
- Clustering and redshift-space distortions in modified gravity models with massive neutrinos
- A semi-analytic model of pairwise velocity distribution between dark matter halos