Constraining \(f(G)\) gravity models using energy conditions

DOI10.1007/s10773-012-1165-zzbMath1259.83019OpenAlexW1979955967MaRDI QIDQ1930075

H. Vaez, Ali Banijamali, Jafar Sadeghi

Publication date: 10 January 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-012-1165-z

zbMATH Keywords

energy conditionsmodified Gauss-Bonnet gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items

Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity, Energy conditions in higher derivative f(R,□R,T) gravity, Study of neutron star in \(f(T)\) and \(f(G)\) gravity framework with polytropic gas background, The study of anisotropic perfect fluid cosmological models in \(f(R,T)\) gravity, On a Bianchi type-I space-time with bulk viscosity in f(R,T) gravity, The study of Bianchi type-III, V, and VI₀ models in modified theory, Energy conditions in modified \(f(G)\) gravity

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