2021
DOI: 10.1016/j.dark.2021.100895
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Extended General Relativity: Gravitational waves from an isotropic and homogeneous collapse

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Cited by 14 publications
(1 citation statement)
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“…The last terms in (2) are very important and cannot be neglected in the dynamics of the system. These terms g αβ δ R αβ = δ , describes the flux of the 4-vector δW α = δ β g βα − δ α βγ g βγ , through the 3D closed hypersurface ∂ M. An important case results when the varied Ricci tensor: δ R αβ , is related to the variation of the metric tensor [17] δ R αβ = λ s x α δg αβ .…”
Section: Extension Of General Relativity With An Extended Manifoldmentioning
confidence: 99%
“…The last terms in (2) are very important and cannot be neglected in the dynamics of the system. These terms g αβ δ R αβ = δ , describes the flux of the 4-vector δW α = δ β g βα − δ α βγ g βγ , through the 3D closed hypersurface ∂ M. An important case results when the varied Ricci tensor: δ R αβ , is related to the variation of the metric tensor [17] δ R αβ = λ s x α δg αβ .…”
Section: Extension Of General Relativity With An Extended Manifoldmentioning
confidence: 99%