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Big bounce with finite-time singularity: The F (R) gravity description by the Big Bounce cosmologies. In this paper, we study a bounce cosmology with a Type IV singularity
ΛcDM bounce cosmology without ΛcDM: The case of modified gravity cosmological eras that constitute the ΛCDM bouncing model can be generated by F(R) gravity, which can lead
Possible evolution of a bouncing universe in cosmological models with non-minimally coupled scalar fields the evolution of the Hubble parameter of the bounce solution essentially depends on the sign of the cosmological
ΛcDM bounce cosmology without ΛcDM: The case of modified gravity cosmological eras that constitute the ΛCDM bouncing model can be generated by F(R) gravity, which can lead
Bouncing solutions in f(T) gravity analysis of the corresponding cosmological dynamics in the cases when bounces and static configurations
Possible evolution of a bouncing universe in cosmological models with non-minimally coupled scalar fields the evolution of the Hubble parameter of the bounce solution essentially depends on the sign of the cosmological
Big bounce with finite-time singularity: The F (R) gravity description by the Big Bounce cosmologies. In this paper, we study a bounce cosmology with a Type IV singularity
The Schwarzschild Singularity: A Semiclassical Bounce? by a regular bounce, described as a regular minimum of the spherical radius (instead of zero) and a
Bounce universe from string-inspired Gauss-Bonnet gravityWe explore cosmology with a bounce in Gauss-Bonnet gravity where the Gauss-Bonnet invariant couples
Bouncing universes in scalar-tensor gravity models admitting negative potentials bouncing universe in the framework of scalar-tensor gravity models in which the scalar field potential may
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