Multifluid cosmology in f(G) gravity

نویسندگان

چکیده

The treatment of ([Formula: see text])-covariant perturbation in a multifluid cosmology with the consideration [Formula: text] gravity, being Gauss–Bonnet term, is done this paper. We define set covariant and gauge-invariant variables to describe density, velocity entropy perturbations for both total matter component fluids. then use different techniques such as scalar decomposition, harmonic quasi-static approximation together redshift transformation get simplified equations analysis. discuss number interesting applications like case where universe filled mixture radiation fluids well dust short- long-wavelength limits. Considering polynomial model, we numerical solutions energy density show that they decay increase redshift. This feature shows under specifically considered one expects formation structure late Universe enhanced.

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ژورنال

عنوان ژورنال: International Journal of Geometric Methods in Modern Physics

سال: 2022

ISSN: ['0219-8878', '1793-6977']

DOI: https://doi.org/10.1142/s0219887823500317