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  1. 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 ...
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  3. researchportal.port.ac.uk

    A perturbative approach to the redshift space power spectrum: beyond the Standard Model ... 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 ...
  4. researchgate.net

    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 ...
  5. inspirehep.net

    A Perturbative Approach to the Redshift Space Power Spectrum: Beyond the Standard Model. Benjamin Bose, Kazuya Koyama. Jun 8, 2016. 23 pages. ... 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 ...
  6. iopscience.iop.org

    We develop a framework to compute the redshift space power spectrum (PS), with kernels beyond Einstein-de Sitter (EdS), that can be applied to a wide variety of generalized cosmologies. ... Bose Benjamin and Koyama Kazuya 2017 A Perturbative Approach to the Redshift Space Correlation Function: Beyond the Standard Model JCAP 08 029 (arXiv:1705. ...
  7. researchportal.port.ac.uk

    A perturbative approach to the redshift space power spectrum: beyond the Standard Model. Benjamin Bose, Kazuya Koyama. Institute of Cosmology & Gravitation; Research output: Contribution to journal › Article › peer-review. 129 Downloads (Pure) Overview; Fingerprint;
  8. ui.adsabs.harvard.edu

    We extend our previous redshift space power spectrum code to the redshift space correlation function. Here we focus on the Gaussian Streaming Model (GSM). Again, the code accommodates a wide range of modified gravity and dark energy models. For the non-linear real space correlation function used in the GSM we use the Fourier transform of the RegPT 1-loop matter power spectrum. We compare ...
  9. ui.adsabs.harvard.edu

    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 to find the SPT kernels. This includes Horndeski's theory with a general potential, which accommodates both chameleon and ...

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