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  1. G400 高等研究院
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Testing local position invariance with odd multipoles of galaxy clustering statistics

http://hdl.handle.net/2237/0002013668
http://hdl.handle.net/2237/0002013668
d303631e-5ccf-4973-8edf-f6c412e2a618
名前 / ファイル ライセンス アクション
PhysRevD_111_L081303.pdf PhysRevD_111_L081303.pdf (585 KB)
アイテムタイプ itemtype_ver1(1)
公開日 2025-11-27
タイトル
タイトル Testing local position invariance with odd multipoles of galaxy clustering statistics
言語 en
著者 Inoue, Takuya

× Inoue, Takuya

en Inoue, Takuya

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Okumura, Teppei

× Okumura, Teppei

en Okumura, Teppei

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Saga, Shohei

× Saga, Shohei

en Saga, Shohei

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Taruya, Atsushi

× Taruya, Atsushi

en Taruya, Atsushi

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
権利情報 © 2025 American Physical Society
言語 en
内容記述
内容記述タイプ Abstract
内容記述 We investigate cosmological constraints on local position invariance (LPI), a key aspect of the Einstein equivalence principle (EEP), through asymmetric galaxy clustering. The LPI asserts that the outcomes of the nongravitational experiments are identical regardless of location in spacetime and has been tested through measurements of the gravitational redshift effect. Therefore, measuring the gravitational redshift effect encoded in galaxy clustering provides a powerful and novel cosmological probe of the LPI. Recent work by Saga et al. proposed its validation using the cross-correlation function between distinct galaxy samples, but their analysis focused solely on the dipole moment. In this paper, we extend their work by further analyzing a higher-order odd multipole moment, the octupole moment, in the constraints on the LPI-violating parameter, 𝛼 , expected from galaxy surveys such as Dark Energy Spectroscopic Instrument, Euclid space telescope, Subaru Prime Focus Spectrograph, and Square Kilometre Array. We demonstrate that combining the octupole and dipole moments significantly improves the constraints, particularly when the analysis is restricted to larger scales, characterized by a large minimum separation 𝑠min . For a conservative setup with 𝑠min=15  Mpc/ℎ , we find an average improvement of 11% compared to using the dipole moment alone. Our results highlight the importance of higher-order multipoles in constraining 𝛼 , providing a more robust approach to testing the EEP on cosmological scales.
言語 en
出版者
出版者 American Physical Society
言語 en
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1103/PhysRevD.111.L081303
収録物識別子
収録物識別子タイプ PISSN
収録物識別子 2470-0010
書誌情報 ja : PHYSICAL REVIEW D

巻 111, 号 8, p. L081303, 発行日 2025-04-22
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