Disentangling RedshiftSpace Distortions and Nonlinear Bias using the 2D Power Spectrum
We present the nonlinear 2D galaxy power spectrum, P(k, µ), in redshift space, measured from the Dark Sky simulations, using galaxy catalogs constructed with both halo occupation distribution and subhalo abundance matching methods, chosen to represent an intermediate redshift sample of luminous red galaxies. We find that the information content in individual µ (cosine of the angle to the line of sight) bins is substantially richer then multipole moments, and show that this can be used to isolate the impact of nonlinear growth and redshift space distortion (RSD) effects. Using the µ < 0.2 simulation data, which we show is not impacted by RSD effects, we can successfully measure the nonlinear bias to an accuracy of ~ 5% at k < 0.6hMpc1 . This use of individual µ bins to extract the nonlinear bias successfully removes a large parameter degeneracy when constraining the linear growth rate of structure. We carry out a joint parameter estimation, using the low µ simulation data to constrain the nonlinear bias, and µ > 0.2 to constrain the growth rate and show that f can be constrained to ~ 26(22)% to a kmax < 0.4(0.6)hMpc1 from clustering alone using a simple dispersion model, for amore »
 Authors:

^{[1]};
^{[2]}
 Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States)
 Stanford Univ., CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
 Publication Date:
 Report Number(s):
 FERMILABPUB15339A
Journal ID: ISSN 00358711; arXiv eprint number arXiv:1508.01803
 Grant/Contract Number:
 AC0207CH11359
 Type:
 Accepted Manuscript
 Journal Name:
 Monthly Notices of the Royal Astronomical Society
 Additional Journal Information:
 Journal Volume: 457; Journal ID: ISSN 00358711
 Publisher:
 Royal Astronomical Society
 Research Org:
 Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
 Sponsoring Org:
 USDOE Office of Science (SC), High Energy Physics (HEP) (SC25)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTRONOMY AND ASTROPHYSICS; Nbody simulations; cosmology:theory; largescale structure of the Universe
 OSTI Identifier:
 1221340
Jennings, Elise, and Wechsler, Risa H. Disentangling RedshiftSpace Distortions and Nonlinear Bias using the 2D Power Spectrum. United States: N. p.,
Web. doi:10.1093/mnras/stv2989.
Jennings, Elise, & Wechsler, Risa H. Disentangling RedshiftSpace Distortions and Nonlinear Bias using the 2D Power Spectrum. United States. doi:10.1093/mnras/stv2989.
Jennings, Elise, and Wechsler, Risa H. 2015.
"Disentangling RedshiftSpace Distortions and Nonlinear Bias using the 2D Power Spectrum". United States.
doi:10.1093/mnras/stv2989. https://www.osti.gov/servlets/purl/1221340.
@article{osti_1221340,
title = {Disentangling RedshiftSpace Distortions and Nonlinear Bias using the 2D Power Spectrum},
author = {Jennings, Elise and Wechsler, Risa H.},
abstractNote = {We present the nonlinear 2D galaxy power spectrum, P(k, µ), in redshift space, measured from the Dark Sky simulations, using galaxy catalogs constructed with both halo occupation distribution and subhalo abundance matching methods, chosen to represent an intermediate redshift sample of luminous red galaxies. We find that the information content in individual µ (cosine of the angle to the line of sight) bins is substantially richer then multipole moments, and show that this can be used to isolate the impact of nonlinear growth and redshift space distortion (RSD) effects. Using the µ < 0.2 simulation data, which we show is not impacted by RSD effects, we can successfully measure the nonlinear bias to an accuracy of ~ 5% at k < 0.6hMpc1 . This use of individual µ bins to extract the nonlinear bias successfully removes a large parameter degeneracy when constraining the linear growth rate of structure. We carry out a joint parameter estimation, using the low µ simulation data to constrain the nonlinear bias, and µ > 0.2 to constrain the growth rate and show that f can be constrained to ~ 26(22)% to a kmax < 0.4(0.6)hMpc1 from clustering alone using a simple dispersion model, for a range of galaxy models. Our analysis of individual µ bins also reveals interesting physical effects which arise simply from different methods of populating halos with galaxies. We also find a prominent turnaround scale, at which RSD damping effects are greater then the nonlinear growth, which differs not only for each µ bin but also for each galaxy model. These features may provide unique signatures which could be used to shed light on the galaxy–dark matter connection. Furthermore, the idea of separating nonlinear growth and RSD effects making use of the full information in the 2D galaxy power spectrum yields significant improvements in constraining cosmological parameters and may be a promising probe of galaxy formation models.},
doi = {10.1093/mnras/stv2989},
journal = {Monthly Notices of the Royal Astronomical Society},
number = ,
volume = 457,
place = {United States},
year = {2015},
month = {8}
}