Cosmological constraints from the redshift dependence of the Alcock-Paczynski test and volume effect: galaxy two-point correlation function

Abstract

We propose a method using the redshift dependence of the Alcock-Paczynski (AP) test and volume effect to measure the cosmic expansion history. The galaxy two-point correlation function as a function of angle, $\xi (\mu )$, is measured at different redshifts. Assuming an incorrect cosmological model to convert galaxy redshifts to distances, the shape of $\xi (\mu )$ appears anisotropic due to the AP effect, and the amplitude shifted by the change in comoving volume. Due to the redshift dependence of the AP and volume effect, both the shape and amplitude of $\xi (\mu )$ exhibit redshift dependence. Similar to Li et.al (2014), we find the redshift-space distortions (RSD) caused by galaxy peculiar velocities, although significantly distorts $\xi (\mu )$, exhibit much less redshift evolution compared to the AP and volume effects. By focusing on the redshift dependence of $\xi (\mu )$, we can correctly recover the cosmological parameters despite the contamination of RSD. The method is tested by using the Horizon Run 3 N-body simulation, from which we made a series of $1/8$-sky mock surveys having 8 million physically self-bound halos and sampled to have roughly a uniform number density in $z=0-1.5$. We find the AP effect results in tight, unbiased constraints on the density parameter and dark energy equation of state, with 68.3% CL intervals $\delta {\Omega }_m\sim 0.03$ and $\delta w\sim 0.1$, and the volume effect leads to much tighter constraints of $\delta {\Omega }_m\sim 0.007$ and $\delta w\sim 0.035$.

9 pages, 5 figures

References in corpus (5)

• A measurement of the Alcock-Paczynski effect using cosmic voids in the SDSS
• Topology of structure in the Sloan Digital Sky Survey: model testing
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• Cosmological Tests using Redshift Space Clustering in BOSS DR11
• Using galaxy pairs as cosmological tracers

Cited by in corpus (17)

• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• Cosmic Velocity Field Reconstruction Using AI
• Alcock-Paczynski Test with the Evolution of Redshift-Space Galaxy Clustering Anisotropy
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Fast generation of mock galaxy catalogues with COLA
• Bayesian deep learning for cosmic volumes with modified gravity
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Fourier space analysis
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Tomographic Alcock-Paczynski Method with Redshift Errors
• Cosmological constraints from the density gradient weighted correlation function
• Tomographic Alcock-Paczynski Test with Marked Correlation Functions