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McDonald (2007) presented an approach to improving perturbation theory (PT) calculations of the dark matter power spectrum, with a derivation based on the idea of renormalization group flow with time.
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M. Pietroni, Journal of Cosmology and Astro-Particle Physics 10
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A. Taruya, T. Nishimichi, S. Saito, and T. Hiramatsu, Phys. Rev
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P. McDonald, Journal of Cosmology and Astro-Particle Physics 11
2009
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2011
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N. S. Sugiyama and T. Futamase, Astrophys. J. 760
2012
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A. Taruya, F. Bernardeau, T. Nishimichi, and S. Codis, Phys. Rev
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J. J. M. Carrasco, M. P. Hertzberg, and L. Senatore, Journal of High Energy Physics 9
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K. C. Chan and R. Scoccimarro, Phys. Rev
2012
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Z. Vlah, U. Seljak, P. McDonald, T. Okumura, and T. Baldauf, JCAP 11
2012
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S. Anselmi and M. Pietroni, JCAP 12
2012
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T. Nishimichi and A. Oka, ArXiv e-prints (2013), arXiv:1310.2672 [astro-ph.CO]
2013
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2013
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2013
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2013
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2014
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2014
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D. Blas, M. Garny, and T. Konstandin, JCAP 1
2014
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F. Bernardeau, A. Taruya, and T. Nishimichi, Phys. Rev
2014
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