scholarly journals Local-gravity test of unified models of inflation and dark energy in f(R) gravity

2020 ◽  
Vol 102 (4) ◽  
Author(s):  
Mai Yashiki ◽  
Nobuyuki Sakai ◽  
Ryo Saito
2010 ◽  
Vol 25 (11n12) ◽  
pp. 843-858 ◽  
Author(s):  
SHINJI TSUJIKAWA

We review a number of approaches that have been adopted to explain the origin of dark energy responsible for the late-time cosmic acceleration. This includes the cosmological constant and dynamical dark energy models such as quintessence, k -essence, Chaplygin gas, f(R) gravity, scalar-tensor theories, and braneworld models. We also discuss observational and local gravity constraints on those models and clarify which models are favored or ruled out in current observations.


Universe ◽  
2018 ◽  
Vol 4 (8) ◽  
pp. 82 ◽  
Author(s):  
Gaurav Narain ◽  
Tianjun Li

A local phenomenological model that reduces to a non-local gravitational theory giving dark energy is proposed. The non-local gravity action is known to fit the data as well as Λ-CDM thereby demanding a more fundamental local treatment. It is seen that the scale-invariant higher-derivative scalar-tensor theory of gravity, which is known to be ultraviolet perturbative renormalizable to all loops and where ghosts become innocuous, generates non-locality at low energies. The local action comprises of two real scalar fields coupled non-minimally with the higher-derivative gravity action. When one of the scalar acquiring the Vacuum Expectation Value (VEV) induces Einstein–Hilbert gravity, generates mass for fields, and gets decoupled from system, it leaves behind a residual theory which in turn leads to a non-local gravity generating dark energy effects.


2008 ◽  
Vol 77 (10) ◽  
Author(s):  
Shinji Tsujikawa ◽  
Kotub Uddin ◽  
Shuntaro Mizuno ◽  
Reza Tavakol ◽  
Jun’ichi Yokoyama

Nature ◽  
2010 ◽  
Author(s):  
Eugenie Samuel Reich
Keyword(s):  

Nature ◽  
2007 ◽  
Author(s):  
Geoff Brumfiel
Keyword(s):  

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