Matter Power Spectrum in f(R) Gravity with Massive Neutrinos

DOI10.1143/PTP.124.541zbMath1205.85046arXiv1005.1171WikidataQ57731831 ScholiaQ57731831MaRDI QIDQ3064758

Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama

Publication date: 23 December 2010

Published in: Progress of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1005.1171

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Gravitational interaction in quantum theory (81V17) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Weak interaction in quantum theory (81V15) Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (5)

On cosmological signatures of baryons-dark energy elastic couplings ⋮ Constraining chameleon models with cosmology ⋮ Matter power spectra in viable \(f(R)\) gravity models with massive neutrinos ⋮ f(R) GRAVITY AND ITS COSMOLOGICAL IMPLICATIONS ⋮ Cosmological constraints with the Effective Fluid approach for Modified Gravity

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