Singularity phenomena in viable f(R) gravity
classification
🌌 astro-ph.CO
gr-qc
keywords
singularitygravityviableaddingbackgroundconsequencescosmologicalcurvature
read the original abstract
The curvature singularity in viable f(R) gravity models is examined when the background density is dense. This singularity could be eliminated by adding the $R^{2}$ term in the Lagrangian. Some of cosmological consequences, in particular the source for the scalar mode of gravitational waves, are discussed.
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