The Zeldovich approximation and wide-angle redshift-space distortions
Abstract
The contribution of line-of-sight (LOS) peculiar velocities to the observed redshift of objects breaks the translational symmetry of the underlying theory, modifying the predicted two-point functions. These `wide-angle effects' have mostly been studied using linear perturbation theory in the context of the multipoles of the correlation function and power spectrum. In this article, we present the first calculation of wide-angle terms in the Zeldovich approximation, which is known to be more accurate than linear theory on scales probed by the next generation of galaxy surveys. We present the exact result for dark matter and perturbatively biased tracers as well as the small angle expansion of the configuration- and Fourier-space two-point functions and the connection to the multifrequency angular power spectrum. We compare different definitions of the LOS direction and discuss how to translate between them. Lastly, we show that wide-angle terms can reach tens of percent of the total signal in a measurement at low redshift in some approximations, and that a generic feature of wide-angle effects is to slightly shift the Baryon Acoustic Oscillation scale.
- Authors:
-
- Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- OSTI Identifier:
- 1530372
- Alternate Identifier(s):
- OSTI ID: 1594732
- Grant/Contract Number:
- AC02-05CH11231; SC0017860; 1713791
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 479; Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; methods: analytical; cosmology: observations; cosmology: theory
Citation Formats
Castorina, Emanuele, and White, Martin. The Zeldovich approximation and wide-angle redshift-space distortions. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty1437.
Castorina, Emanuele, & White, Martin. The Zeldovich approximation and wide-angle redshift-space distortions. United States. https://doi.org/10.1093/mnras/sty1437
Castorina, Emanuele, and White, Martin. Tue .
"The Zeldovich approximation and wide-angle redshift-space distortions". United States. https://doi.org/10.1093/mnras/sty1437. https://www.osti.gov/servlets/purl/1530372.
@article{osti_1530372,
title = {The Zeldovich approximation and wide-angle redshift-space distortions},
author = {Castorina, Emanuele and White, Martin},
abstractNote = {The contribution of line-of-sight (LOS) peculiar velocities to the observed redshift of objects breaks the translational symmetry of the underlying theory, modifying the predicted two-point functions. These `wide-angle effects' have mostly been studied using linear perturbation theory in the context of the multipoles of the correlation function and power spectrum. In this article, we present the first calculation of wide-angle terms in the Zeldovich approximation, which is known to be more accurate than linear theory on scales probed by the next generation of galaxy surveys. We present the exact result for dark matter and perturbatively biased tracers as well as the small angle expansion of the configuration- and Fourier-space two-point functions and the connection to the multifrequency angular power spectrum. We compare different definitions of the LOS direction and discuss how to translate between them. Lastly, we show that wide-angle terms can reach tens of percent of the total signal in a measurement at low redshift in some approximations, and that a generic feature of wide-angle effects is to slightly shift the Baryon Acoustic Oscillation scale.},
doi = {10.1093/mnras/sty1437},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 479,
place = {United States},
year = {Tue Jun 05 00:00:00 EDT 2018},
month = {Tue Jun 05 00:00:00 EDT 2018}
}
Web of Science
Figures / Tables:
Works referencing / citing this record:
The reconstructed power spectrum in the Zeldovich approximation
journal, September 2019
- Chen, Shi-Fan; Vlah, Zvonimir; White, Martin
- Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 09
Erratum: The Zeldovich approximation and wide-angle redshift-space distortions
journal, September 2019
- Castorina, Emanuele; White, Martin
- Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel’dovich approximation
journal, November 2019
- Taruya, Atsushi; Saga, Shohei; Breton, Michel-Andrès
- Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 3
Ingredients for 21 cm Intensity Mapping
journal, October 2018
- Villaescusa-Navarro, Francisco; Genel, Shy; Castorina, Emanuele
- The Astrophysical Journal, Vol. 866, Issue 2
Ingredients for 21cm intensity mapping
text, January 2018
- Villaescusa-Navarro, Francisco; Genel, Shy; Castorina, Emanuele
- arXiv
Unequal time correlators and the Zeldovich approximation
text, January 2019
- Chisari, Nora Elisa; Pontzen, Andrew
- arXiv
The Reconstructed Power Spectrum in the Zeldovich Approximation
text, January 2019
- Chen, Shi-Fan; Vlah, Zvonimir; White, Martin
- arXiv
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximation
text, January 2019
- Taruya, Atsushi; Saga, Shohei; Breton, Michel-Andrès
- arXiv
Figures / Tables found in this record: