Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey

Kazuhiro Yamamoto; Gen Nakamura; Gert Hütsi; Tatsuya Narikawa; Takahiro Sato

doi:10.1103/PhysRevD.81.103517

Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey

Kazuhiro Yamamoto, Gen Nakamura, Gert Hütsi, Tatsuya Narikawa, Takahiro Sato

Research output: Contribution to journal › Article › peer-review

43 Citations (Scopus)

Abstract

A constraint on the viable f(R) model is investigated by confronting theoretical predictions with the multipole power spectrum of the luminous red galaxy sample of the Sloan Digital Sky Survey, data release 7. We obtain a constraint on the Compton wavelength parameter of the f(R) model on the scales of cosmological large-scale structure. A prospect of constraining the Compton wavelength parameter with a future redshift survey is also investigated. The usefulness of the redshift-space distortion for testing the gravity theory on cosmological scales is demonstrated.

Original language	English
Article number	103517
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	81
Issue number	10
DOIs	https://doi.org/10.1103/PhysRevD.81.103517
Publication status	Published - May 13 2010
Externally published	Yes

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.81.103517

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Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey. / Yamamoto, Kazuhiro; Nakamura, Gen; Hütsi, Gert; Narikawa, Tatsuya; Sato, Takahiro.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 81, No. 10, 103517, 13.05.2010.

Research output: Contribution to journal › Article › peer-review

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Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey

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