Finite-time cosmological singularities and the possible fate of the Universe
Singularities in any physical theory are either remarkable indicators of the unknown
underlying fundamental theory, or indicate a change in the description of the physical reality …
underlying fundamental theory, or indicate a change in the description of the physical reality …
Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution
We systematically review some standard issues and also the latest developments of
modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time …
modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late-time …
Unified cosmic history in modified gravity: from F (R) theory to Lorentz non-invariant models
S Nojiri, SD Odintsov - Physics Reports, 2011 - Elsevier
The classical generalization of general relativity is considered as the gravitational alternative
for a unified description of the early-time inflation with late-time cosmic acceleration. The …
for a unified description of the early-time inflation with late-time cosmic acceleration. The …
[HTML][HTML] f (R) theories
A De Felice, S Tsujikawa - Living Reviews in Relativity, 2010 - Springer
Over the past decade, f (R) theories have been extensively studied as one of the simplest
modifications to General Relativity. In this article we review various applications of f (R) …
modifications to General Relativity. In this article we review various applications of f (R) …
Finite-time future singularities in modified Gauss–Bonnet and ℱ(R,G) gravity and singularity avoidance
K Bamba, SD Odintsov, L Sebastiani… - The European Physical …, 2010 - Springer
We study all four types of finite-time future singularities emerging in the late-time
accelerating (effective quintessence/phantom) era from ℱ (R, G)-gravity, where R and G are …
accelerating (effective quintessence/phantom) era from ℱ (R, G)-gravity, where R and G are …
Modified gravity models of dark energy
S Tsujikawa - Lectures on cosmology: Accelerated Expansion of the …, 2010 - Springer
We review the recent progress for modified gravity models of dark energy–including f (R)
gravity, scalar-tensor theories, and braneworld models. In f (R) gravity, where the …
gravity, scalar-tensor theories, and braneworld models. In f (R) gravity, where the …
Wormholes in -gravity within the f(R, T) formalism
We propose, as a novelty in the literature, the modeling of wormholes within a particular
case of f (R, T) gravity, namely f (R, T)= R+ α R^ 2+ λ T f (R, T)= R+ α R 2+ λ T, with R and T …
case of f (R, T) gravity, namely f (R, T)= R+ α R^ 2+ λ T f (R, T)= R+ α R 2+ λ T, with R and T …
Neutron stars in the Starobinsky model
We study the structure of neutron stars in the f (R)= R+ α R 2 theory of gravity (the
Starobinsky model) in an exact and nonperturbative approach. In this model, apart from the …
Starobinsky model) in an exact and nonperturbative approach. In this model, apart from the …
Dark energy: investigation and modeling
S Tsujikawa - Dark Matter and Dark Energy: A Challenge for Modern …, 2011 - Springer
Constantly accumulating observational data continue to confirm that about 70% of the
energy density today consists of dark energy responsible for the accelerated expansion of …
energy density today consists of dark energy responsible for the accelerated expansion of …
Galileon gravity and its relevance to late time cosmic acceleration
R Gannouji, M Sami - Physical Review D—Particles, Fields, Gravitation, and …, 2010 - APS
We consider the covariant Galileon gravity taking into account the third order and fourth
order scalar field Lagrangians L 3 (π) and L 4 (π), consisting of three and four π's with four …
order scalar field Lagrangians L 3 (π) and L 4 (π), consisting of three and four π's with four …