Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
| Autor: | Kaeonikhom, Chakkrit, Chantavat, Teeraparb |
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| Rok vydání: | 2018 |
| Předmět: | |
| Zdroj: | Physical Review D, 98, 083534 (2018) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1103/PhysRevD.98.083534 |
| Popis: | We apply the Lagrangian perturbation theory with time-dependent growth functions at second and third order of perturbation with the aim to model the effect of dynamical dark energy on redshift-space distortions. Our fiducial galaxy redshift surveys are modeled after the upcoming SKA and DESI redshift surveys. We include PLANCK CMB priors and the 20\% uncertainty on the linear bias parameter, incorporating the unknown instrumentation noise. After the marginalizing, our results show that the constraints on the density parameter could potentially get better than $\sim$1\%, while the constraints on $w_0$ and $w_{\rm a}$ could be better than $\sim 5\%$ and $\sim 60\%$ respectively, consistent with works done before. However, the inclusion of time-dependent growth functions would alter the nonlinear power spectrum by as much as $\sim$10\%. The inclusion of the time-dependent growth functions become crucial as the precision gets better. Comment: 12 pages, 5 figures, accepted for publication in Physical Review D |
| Databáze: | arXiv |
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