A perturbative approach to the redshift space power spectrum: beyond the Standard Model
Research output: Contribution to journal › Article › peer-review
We develop a code to produce the power spectrum in redshift space based on standard perturbation theory (SPT) at 1-loop order. The code can be applied to a wide range of modified gravity and dark energy models using a recently proposed numerical method by A.Taruya. This includes Horndeski's theory with a general potential, which accommodates both chameleon and Vainshtein screening mechanisms and provides a non-linear extension of the effective theory of dark energy up to third order. Focus is on a recent non-linear model of the redshift space power spectrum which has been shown to model the anisotropy very well at relevant scales for the SPT framework, as well as capturing relevant non-linear effects typical of modified gravity theories. We provide consistency checks of the code against established results and elucidate it's application within the light of upcoming high precision RSD data.
| Original language | English |
|---|---|
| Article number | 032 |
| Journal | Journal of Cosmology and Astroparticle Physics |
| Volume | 2016 |
| Issue number | 08 |
| DOIs | |
| Publication status | Published - 17 Aug 2016 |
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Rights statement: The final published version of Bose, B & Koyama, K. 'A perturbative approach to the redshift space power spectrum: beyond the Standard Model' can be located at DOI: 10.1088/1475-7516/2016/08/32
Accepted author manuscript (Post-print), 1.08 MB, PDF document
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