Clarification of an extended theory of gravity and a reply to Gr�n and Soleng

1990 ◽  
Vol 22 (6) ◽  
pp. 707-713 ◽  
Author(s):  
Paul S. Wesson
2021 ◽  
Author(s):  
Vaibhav Kalvakota

The f (R) theory of gravity is an extended theory of gravity that is based on general relativity in the simplest case of $f(R) = R$. This theory extends such a function of the Ricci scalar into arbitrary functions that are not necessarily linear, i.e. could be of the form $f(R) = \alpha R^{2}$. The action for such a theory would be $S_{EH} = \frac{1}{2k} \int f(R) + L^{m}\; d^{4}x\sqrt{−g}$, where $S_{EH}$ is the Einstein-Hilbert action for our theory, $g$ is the determinant of the metric tensor $g_{\mu \nu}$ and $L^{m}$ is the Lagrangian density for matter. In this paper, we will look at some of the physical implications of such a theory, and the importance of such a theory in cosmology and in understanding the geometric nature of such f (R) theories of gravity.


2019 ◽  
Vol 28 (08) ◽  
pp. 1950098 ◽  
Author(s):  
P. H. R. S. Moraes ◽  
W. de Paula ◽  
R. A. C. Correa

Wormholes (WHs) are a solution for General Relativity field equations which characterize a passage or tunnel that connects two different regions of spacetime and is filled by some sort of exotic matter that does not satisfy the energy conditions. On the other hand, it is known that in extended theories of gravity, the extra degrees of freedom once provided may allow the energy conditions to be obeyed and, consequently, the matter content of the WH to be nonexotic. In this work, we obtain, as a novelty in the literature, solutions for charged WHs in the [Formula: see text]-extended theory of gravity. We show that the presence of charge in these objects may be a possibility to respect some stability conditions for their metric. Also, remarkably, the energy conditions are respected in the present approach. In addition, we argue that our framework can be very useful to study the possibility of evolving [Formula: see text] and [Formula: see text]-dimensional WH spacetime within the context of nonlinear electrodynamics, which open a new window to probe the physical quantities in a WH-type solution.


1985 ◽  
Vol 31 (10) ◽  
pp. 2488-2496 ◽  
Author(s):  
R. B. Mann ◽  
J. W. Moffat

2021 ◽  
pp. 2100086
Author(s):  
Pratik P Ray ◽  
Sankarsan Tarai ◽  
B. Mishra ◽  
S. K. Tripathy

2019 ◽  
Vol 16 (05) ◽  
pp. 1950067 ◽  
Author(s):  
Hoavo Hova ◽  
Huanxiong Yang ◽  
Samuel Owusu

In this work, we study the evolution of an isotropic universe in an extended theory of gravity obtained geometrically by transforming the normal-gauge Lyra displacement vector field [Formula: see text] as a complex vectorial function depending on a dynamical scalar field [Formula: see text]. By using the latest observational data, we observe that for [Formula: see text] the universe starts accelerating at the critical scale factor [Formula: see text] which corresponds to a redshift of [Formula: see text]. We also find that the dark energy fluid considered in this model is a generalized fluid with equation of state [Formula: see text].


2020 ◽  
Vol 63 ◽  
pp. 448-458 ◽  
Author(s):  
S.K. Tripathy ◽  
B. Mishra

2017 ◽  
Vol 771 ◽  
pp. 230-234 ◽  
Author(s):  
David C. Dunbar ◽  
John H. Godwin ◽  
Guy R. Jehu ◽  
Warren B. Perkins

2019 ◽  
Vol 134 (10) ◽  
Author(s):  
Sunil Kumar Tripathy ◽  
Rakesh Kumar Khuntia ◽  
Priyabrata Parida

2020 ◽  
Vol 102 (8) ◽  
Author(s):  
S. Ilijić ◽  
M. Sossich

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