2017
DOI: 10.1007/s10509-017-3035-x
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Improved Solar System bounds on the cosmologically viable f ( G ) $f(\mathcal{G})$ gravity

Abstract: In recent times, there has been an increasing interest with theories of modified gravity as a means to gain a deeper understanding of the universe's late-time acceleration phase. In this study we focused our attention on a specific cosmologically viable f (R) model. We performed a dynamic stability analysis of this model, revealing that the model supports presence of just one asymptotically stable solution which can explain the present-day acceleration of the universe.

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Cited by 5 publications
(4 citation statements)
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“…In ref. [8], improved Solar System bounds are obtained for this theory using cosmological models. These improved constraints are obtained on the behalf of supplementary advances of the perihelia given by INPOP10a and INPOP15a (France) and EPM2011 (Russia) ephemerides, where Lense-Thirring effect has been considered due to the Sun's angular momentum and the uncertainty of the Sun's quadrupole moment.…”
mentioning
confidence: 99%
“…In ref. [8], improved Solar System bounds are obtained for this theory using cosmological models. These improved constraints are obtained on the behalf of supplementary advances of the perihelia given by INPOP10a and INPOP15a (France) and EPM2011 (Russia) ephemerides, where Lense-Thirring effect has been considered due to the Sun's angular momentum and the uncertainty of the Sun's quadrupole moment.…”
mentioning
confidence: 99%
“…Vegetables have high antioxidant and phenolic components. 7,8 Phytochemicals possess various chemical entities, including polyphenols, steroidal saponins, flavonoids, organosulphur compounds, and vitamins. 9 Natural polyphenols are plentiful antioxidants in human food diets, and radical scavenging actions are associated with substituting hydroxyl groups of phenolics.…”
Section: Introductionmentioning
confidence: 99%
“…Some examples are scalar-tensor theories including the Brans-Dicke theories [7][8][9][10] and general scalar-tensor theories [11][12][13][14][15][16], Einstein-aether theory [17], Bimetric theories [18][19][20], tensor-vector-scalar theories [21][22][23][24], scalar-tensor-vector theories [25,26], and Einstein-Cartan-Sciama-Kibble theories [27,28]. There are models of higher derivative and non-local theories of gravity, such as f(R) theories [29][30][31][32][33], f(G) theories [34][35][36], Hořava-Lifschitz gravity [37][38][39], as well as Galileons [40,41]. The other forms of modified theories of gravity with higher dimensions include Kaluza-Klein theories [42][43][44], the Brane cosmology or higher co-dimension brane-worlds [45][46][47][48] and Einstein-Gauss-Bonnet gravity [49].…”
Section: Introductionmentioning
confidence: 99%