scholarly journals Energy Conditions and Constraints on the Generalized Non-Local Gravity Model

2017 ◽  
Vol 34 (7) ◽  
pp. 079801 ◽  
Author(s):  
Ya-Bo Wu ◽  
Xue Zhang ◽  
Bo-Hai Chen ◽  
Nan Zhang ◽  
Meng-Meng Wu
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.


2017 ◽  
Vol 14 (02) ◽  
pp. 1750019 ◽  
Author(s):  
F. Briscese ◽  
M. L. Pucheu

We derive the dynamical equations for a non-local gravity model in the Palatini formalism and we discuss some of the properties of this model. We have show that, in some specific case, the vacuum solutions of general relativity are also vacuum solutions of the non-local model, so we conclude that, at least in this case, the singularities of Einstein’s gravity are not removed.


Meccanica ◽  
2021 ◽  
Author(s):  
A. Sapora ◽  
G. Efremidis ◽  
P. Cornetti

AbstractTwo nonlocal approaches are applied to the borehole geometry, herein simply modelled as a circular hole in an infinite elastic medium, subjected to remote biaxial loading and/or internal pressure. The former approach lies within the framework of Gradient Elasticity (GE). Its characteristic is nonlocal in the elastic material behaviour and local in the failure criterion, hence simply related to the stress concentration factor. The latter approach is the Finite Fracture Mechanics (FFM), a well-consolidated model within the framework of brittle fracture. Its characteristic is local in the elastic material behaviour and non-local in the fracture criterion, since crack onset occurs when two (stress and energy) conditions in front of the stress concentration point are simultaneously met. Although the two approaches have a completely different origin, they present some similarities, both involving a characteristic length. Notably, they lead to almost identical critical load predictions as far as the two internal lengths are properly related. A comparison with experimental data available in the literature is also provided.


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):  

2021 ◽  
Author(s):  
◽  
Shubham Maheshwari
Keyword(s):  

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.


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