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Title: New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies

Abstract

Here we report a new test of modified gravity theories using the large-scale structure of the Universe. This paper is the first attempt to (1) apply a joint analysis of the anisotropic components of galaxy two- and three-point correlation functions (2 and 3PCFs) to actual galaxy data and (2) constrain the non-linear effects of degenerate higher-order scalar-tensor (DHOST) theories on cosmological scales. Applying this analysis to the Baryon Oscillation Spectroscopic Survey (BOSS) data release 12, we obtain the lower bounds of –1.655 < ξt and –0.504 < ξs at the $$95{{\ \rm per\ cent}}$$ confidence level on the parameters characterizing the time evolution of the tidal and shift terms of the second-order velocity field. These constraints are consistent with GR predictions of ξt = 15/1144 and ξs = 0. Moreover, they represent a 35-fold and 20-fold improvement, respectively, over the joint analysis with only the isotropic 3PCF. We ensure the validity of our results by investigating various quantities, including theoretical models of the 3PCF, window function corrections, cumulative S/N, Fisher matrices, and statistical scattering effects of mock simulation data. We also find statistically significant discrepancies between the BOSS data and the Patchy mocks for the 3PCF measurement. Finally, we package all of our 3PCF analysis codes under the name hitomi and make them publicly available so that readers can reproduce all the results of this paper and easily apply them to ongoing future galaxy surveys.

Authors:
 [1];  [2];  [3];  [4];  [5];  [6]; ORCiD logo [7]; ORCiD logo [8]; ORCiD logo [9]
  1. National Astronomical Observatory of Japan, Tokyo (Japan)
  2. Kanagawa University (Japan)
  3. Rikkyo University, Tokyo (Japan)
  4. Waseda Institute for Advanced Study, Tokyo (Japan); University of Tokyo (Japan)
  5. Nagoya University (Japan)
  6. Tokyo Institute of Technology (Japan)
  7. Missouri University of Science and Technology, Rolla, MO (United States); University of Tokyo, Chiba (Japan)
  8. University of Edinburgh (United Kingdom)
  9. Ohio University, Athens, OH (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); University of California, Berkeley, CA (United States)
Publication Date:
Research Org.:
Ohio Univ., Athens, OH (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); Japan Society for the Promotion of Science (JSPS)
OSTI Identifier:
2290366
Alternate Identifier(s):
OSTI ID: 2229046
Grant/Contract Number:  
SC0019091; AC02-05CH11231; SC0023241; JP21H01080
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 523; Journal Issue: 2; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dark matter; large-scale structure of Universe; cosmology; observations; theory

Citation Formats

Sugiyama, Naonori S., Yamauchi, Daisuke, Kobayashi, Tsutomu, Fujita, Tomohiro, Arai, Shun, Hirano, Shin’ichi, Saito, Shun, Beutler, Florian, and Seo, Hee-Jong. New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies. United States: N. p., 2023. Web. doi:10.1093/mnras/stad1505.
Sugiyama, Naonori S., Yamauchi, Daisuke, Kobayashi, Tsutomu, Fujita, Tomohiro, Arai, Shun, Hirano, Shin’ichi, Saito, Shun, Beutler, Florian, & Seo, Hee-Jong. New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies. United States. https://doi.org/10.1093/mnras/stad1505
Sugiyama, Naonori S., Yamauchi, Daisuke, Kobayashi, Tsutomu, Fujita, Tomohiro, Arai, Shun, Hirano, Shin’ichi, Saito, Shun, Beutler, Florian, and Seo, Hee-Jong. Thu . "New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies". United States. https://doi.org/10.1093/mnras/stad1505.
@article{osti_2290366,
title = {New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies},
author = {Sugiyama, Naonori S. and Yamauchi, Daisuke and Kobayashi, Tsutomu and Fujita, Tomohiro and Arai, Shun and Hirano, Shin’ichi and Saito, Shun and Beutler, Florian and Seo, Hee-Jong},
abstractNote = {Here we report a new test of modified gravity theories using the large-scale structure of the Universe. This paper is the first attempt to (1) apply a joint analysis of the anisotropic components of galaxy two- and three-point correlation functions (2 and 3PCFs) to actual galaxy data and (2) constrain the non-linear effects of degenerate higher-order scalar-tensor (DHOST) theories on cosmological scales. Applying this analysis to the Baryon Oscillation Spectroscopic Survey (BOSS) data release 12, we obtain the lower bounds of –1.655 < ξt and –0.504 < ξs at the $95{{\ \rm per\ cent}}$ confidence level on the parameters characterizing the time evolution of the tidal and shift terms of the second-order velocity field. These constraints are consistent with GR predictions of ξt = 15/1144 and ξs = 0. Moreover, they represent a 35-fold and 20-fold improvement, respectively, over the joint analysis with only the isotropic 3PCF. We ensure the validity of our results by investigating various quantities, including theoretical models of the 3PCF, window function corrections, cumulative S/N, Fisher matrices, and statistical scattering effects of mock simulation data. We also find statistically significant discrepancies between the BOSS data and the Patchy mocks for the 3PCF measurement. Finally, we package all of our 3PCF analysis codes under the name hitomi and make them publicly available so that readers can reproduce all the results of this paper and easily apply them to ongoing future galaxy surveys.},
doi = {10.1093/mnras/stad1505},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 523,
place = {United States},
year = {Thu May 18 00:00:00 EDT 2023},
month = {Thu May 18 00:00:00 EDT 2023}
}

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Matching Bayesian and frequentist coverage probabilities when using an approximate data covariance matrix
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Optimising growth of structure constraints on modified gravity
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