scholarly journals Aspects of Ultraviolet Non-local Gravity

2021 ◽  
Author(s):  
◽  
Shubham Maheshwari
Keyword(s):  
2015 ◽  
Vol 743 ◽  
pp. 189-197 ◽  
Author(s):  
Antonio De Felice ◽  
Misao Sasaki
Keyword(s):  

2016 ◽  
Vol 2016 (4) ◽  
pp. 1-21 ◽  
Author(s):  
Cosimo Bambi ◽  
Daniele Malafarina ◽  
Leonardo Modesto
Keyword(s):  

2021 ◽  
pp. 109-127
Author(s):  
Gianluca Calcagni
Keyword(s):  

2019 ◽  
Vol 16 (10) ◽  
pp. 1950149 ◽  
Author(s):  
M. Ilyas

We investigate the different energy conditions in non-local gravity, which is obtained by adding an arbitrary function of d’Alembertian operator, [Formula: see text], to the Hilbert–Einstein action. We analyze the validity of four different energy conditions and illustrate the different constraints over parameters of the power-law solution as well as de Sitter solution.


2020 ◽  
Vol 135 (12) ◽  
Author(s):  
Francesco Bajardi ◽  
Salvatore Capozziello ◽  
Daniele Vernieri

AbstractNon-local gravity cosmologies are considered under the standard of Noether symmetry approach. In particular, we focus on non-local theories whose gravitational actions depend on curvature and Gauss–Bonnet scalar invariants. Specific functional forms of the related point-like Lagrangians are selected by Noether symmetries, and we solve the corresponding field equations finding out exact cosmological solutions.


2020 ◽  
Vol 810 ◽  
pp. 135821 ◽  
Author(s):  
S. Capozziello ◽  
M. Capriolo ◽  
S. Nojiri

2012 ◽  
Vol 21 (01) ◽  
pp. 1250006 ◽  
Author(s):  
YING-LI ZHANG ◽  
MISAO SASAKI

We consider a model of non-local gravity with a large bare cosmological constant, Λ, and study its cosmological solutions. The model is characterized by a function f(ψ) = f0eαψ, where ψ = □-1R and α is a real dimensionless parameter. In the absence of matter, we find an expanding universe solution a ∝ tn with n < 1, that is, a universe with decelerated expansion without any fine-tuning of the parameter. Thus the effect of the cosmological constant is effectively shielded in this solution. It has been known that solutions in non-local gravity often suffer from the existence of ghost modes. In the present case, we find the solution is ghost-free if α > αcr ≈ 0.17. This is quite a weak condition. We argue that the solution is stable against the inclusion of matter fields. Thus our solution opens up new possibilities for solution to the cosmological constant problem.


2019 ◽  
Vol 795 ◽  
pp. 391-397 ◽  
Author(s):  
Gianluca Calcagni ◽  
Leonardo Modesto ◽  
Giuseppe Nardelli
Keyword(s):  

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