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We extend the scale-dependent Gaussian Streaming Model (GSM) to produce analytical predictions for the anisotropic redshift-space correlation function for biased tracers in modified gravity models.
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K. Koyama, Ghosts in the self-accelerating universe , Class. Quant. Grav. 24
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2009
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K. Koyama, A. Taruya and T. Hiramatsu, Nonlinear evolution of the matter power spectrum in modified theories of gravity , Phys. Rev. D 79
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K. Hinterbichler and J. Khoury, Screening long-range forces through local symmetry restoration , Phys. Rev. Lett. 104
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A. De Felice and S. Tsujikawa, f(R) theories , Living Rev. Rel. 13
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2011
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2016
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2016
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A. Barreira, A. G. Sánchez and F. Schmidt, Validating estimates of the growth rate of structure with modified gravity simulations , Phys. Rev. D 94
2016
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2016
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M. White, A marked correlation function for constraining modified gravity models , JCAP 1611
2016
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P. Creminelli and F. Vernizzi, Dark Energy after GW170817 and GRB170817A , Phys. Rev. Lett. 119
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P. Arnalte-Mur, W. A. Hellwing and P. Norberg, Real- and redshift-space halo clustering in f(R) cosmologies , Monthly Notices of the Royal Astronomical Society 467
2017
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M. Fasiello and Z. Vlah, Screening in perturbative approaches to LSS , Phys. Lett. B773
2017
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C. Burrage and J. Sakstein, Tests of Chameleon Gravity , Living Rev. Rel. 21
2018
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2018
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V. Desjacques, D. Jeong and F. Schmidt, Large-Scale Galaxy Bias , Phys. Rept. 733
2018
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A. Aviles, Renormalization of Lagrangian bias via spectral parameters , Phys. Rev. D98
2018
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2019
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