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

Sugiyama, Naonori S.; Yamauchi, Daisuke; Kobayashi, Tsutomu; Fujita, Tomohiro; Arai, Shun; Hirano, Shin’ichi; Saito, Shun; Beutler, Florian; Seo, Hee-Jong

doi:10.1093/mnras/stad1505

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

Journal Article · Thu May 18 00:00:00 EDT 2023 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stad1505· OSTI ID:2290366

Sugiyama, Naonori S. ^[1]; Yamauchi, Daisuke ^[2]; Kobayashi, Tsutomu ^[3]; Fujita, Tomohiro ^[4]; Arai, Shun ^[5]; Hirano, Shin’ichi ^[6];

^[7];

^[8];

^[9]

National Astronomical Observatory of Japan, Tokyo (Japan)
Kanagawa University (Japan)
Rikkyo University, Tokyo (Japan)
Waseda Institute for Advanced Study, Tokyo (Japan); University of Tokyo (Japan)
Nagoya University (Japan)
Tokyo Institute of Technology (Japan)
Missouri University of Science and Technology, Rolla, MO (United States); University of Tokyo, Chiba (Japan)
University of Edinburgh (United Kingdom)
Ohio University, Athens, OH (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); University of California, Berkeley, CA (United States)

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 < ξ_t and –0.504 < ξ_s 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 ξ_t = 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.

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Research Organization:: Ohio Univ., Athens, OH (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); Japan Society for the Promotion of Science (JSPS)

Grant/Contract Number:: SC0019091; AC02-05CH11231; SC0023241; JP21H01080

OSTI ID:: 2290366

Alternate ID(s):: OSTI ID: 2229046

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 523, Issue 2; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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