An iterative reconstruction of cosmological initial density fields
Abstract
We present an iterative method to reconstruct the linear-theory initial conditions from the late-time cosmological matter density field, with the intent of improving the recovery of the cosmic distance scale from the baryon acoustic oscillations. We present tests using the dark matter density field in both real and redshift space generated from an N-body simulation. In redshift space at z = 0.5, we find that the reconstructed displacement field using our iterative method are more than 80 percent correlated with the true displacement field of the dark matter particles on scales k < 0.10 h Mpc-1. Furthermore, we show that the two-point correlation function of our reconstructed density field matches that of the initial density field substantially better, especially on small scales (<40 h-1 Mpc). Our redshift-space results are improved if we use an anisotropic smoothing so as to account for the reduced small-scale information along the line of sight in redshift space.
- Authors:
-
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Tohoku Univ., Sendai (Japan)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Publication Date:
- Research Org.:
- Harvard Univ., Cambridge, MA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1540619
- Grant/Contract Number:
- SC0013718
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 478; Journal Issue: 2; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics
Citation Formats
Hada, Ryuichiro, and Eisenstein, Daniel J. An iterative reconstruction of cosmological initial density fields. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty1203.
Hada, Ryuichiro, & Eisenstein, Daniel J. An iterative reconstruction of cosmological initial density fields. United States. https://doi.org/10.1093/mnras/sty1203
Hada, Ryuichiro, and Eisenstein, Daniel J. Fri .
"An iterative reconstruction of cosmological initial density fields". United States. https://doi.org/10.1093/mnras/sty1203. https://www.osti.gov/servlets/purl/1540619.
@article{osti_1540619,
title = {An iterative reconstruction of cosmological initial density fields},
author = {Hada, Ryuichiro and Eisenstein, Daniel J.},
abstractNote = {We present an iterative method to reconstruct the linear-theory initial conditions from the late-time cosmological matter density field, with the intent of improving the recovery of the cosmic distance scale from the baryon acoustic oscillations. We present tests using the dark matter density field in both real and redshift space generated from an N-body simulation. In redshift space at z = 0.5, we find that the reconstructed displacement field using our iterative method are more than 80 percent correlated with the true displacement field of the dark matter particles on scales k < 0.10 h Mpc-1. Furthermore, we show that the two-point correlation function of our reconstructed density field matches that of the initial density field substantially better, especially on small scales (<40 h-1 Mpc). Our redshift-space results are improved if we use an anisotropic smoothing so as to account for the reduced small-scale information along the line of sight in redshift space.},
doi = {10.1093/mnras/sty1203},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 478,
place = {United States},
year = {Fri May 11 00:00:00 EDT 2018},
month = {Fri May 11 00:00:00 EDT 2018}
}
Web of Science
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