scholarly journals Superpotential method for chiral cosmological models connected with modified gravity

2019 ◽  
Vol 100 (6) ◽  
Author(s):  
S. V. Chervon ◽  
I. V. Fomin ◽  
E. O. Pozdeeva ◽  
M. Sami ◽  
S. Yu. Vernov
2013 ◽  
Vol 350 (1) ◽  
pp. 375-380 ◽  
Author(s):  
D. R. K. Reddy ◽  
R. Bhuvana Vijaya ◽  
T. Vidya Sagar ◽  
R. L. Naidu

2021 ◽  
Vol 2081 (1) ◽  
pp. 012002
Author(s):  
I V Fomin ◽  
S V Chervon

Abstract We consider cosmological models based on the generalized scalar-tensor gravity, which correspond to the observational constraints on the parameters of cosmological perturbations for any model’s parameters. The estimates of the energy density of relic gravitational waves for such a cosmological models were made. The possibility of direct detection of such a gravitational waves using modern and prospective methods was discussed as well.


2020 ◽  
Vol 51 (4) ◽  
pp. 744-749 ◽  
Author(s):  
S. Yu. Vernov ◽  
V. R. Ivanov ◽  
E. O. Pozdeeva

2021 ◽  
Vol 81 (11) ◽  
Author(s):  
Vsevolod R. Ivanov ◽  
Sergey Yu. Vernov

AbstractWe consider modified gravity cosmological models that can be transformed into two-field chiral cosmological models by the conformal metric transformation. For the $$R^2$$ R 2 gravity model with an additional scalar field and the corresponding two-field model with the cosmological constant and nonstandard kinetic part of the action, the general solutions have been obtained in the spatially flat FLRW metric. We analyze the correspondence of the cosmic time solutions obtained and different possible evolutions of the Hubble parameters in the Einstein and Jordan frames.


2020 ◽  
Vol 29 (15) ◽  
pp. 2050100
Author(s):  
B. Mishra ◽  
S. K. Tripathy ◽  
Saibal Ray

In this work, we present a few simple cosmological models under the modified theory of gravity in the particular form of [Formula: see text], where [Formula: see text] is the Ricci Scalar and [Formula: see text] is the trace of the energy–momentum tensor. Two special cosmological models are studied with (i) hyperbolic scale factor and (ii) specific form of the Hubble parameter. The models are observed to predict relevant cosmological parameters closer to the observational values. Both the models reduce to overlap with the [Formula: see text]CDM model at late times. We have discussed some interesting results related to wormhole solutions as evolved from our model. The possible occurrence of Big Trip in wormholes for the models are also discussed.


2017 ◽  
Vol 95 (4) ◽  
Author(s):  
Tiberiu Harko ◽  
Francisco S. N. Lobo ◽  
Emmanuel N. Saridakis ◽  
Minas Tsoukalas

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