2011
DOI: 10.1016/j.physletb.2010.12.056
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Non-minimally coupled f(R) cosmology

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Cited by 54 publications
(4 citation statements)
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“…However, it has been shown that, along with a matter field, any such model could behave in quite a different manner Amendola, Gannouji, Polarski and Tsujikawa 2007). Some models where the Ricci scalar is non-minimally coupled to the matter sector are also there in literature (Thakur et al 2011). Some of the modifications of the geometry sector also involves a function of G, the Gauss-Bonnet scalar.…”
Section: Introductionmentioning
confidence: 99%
“…However, it has been shown that, along with a matter field, any such model could behave in quite a different manner Amendola, Gannouji, Polarski and Tsujikawa 2007). Some models where the Ricci scalar is non-minimally coupled to the matter sector are also there in literature (Thakur et al 2011). Some of the modifications of the geometry sector also involves a function of G, the Gauss-Bonnet scalar.…”
Section: Introductionmentioning
confidence: 99%
“…But this modification would vanish in the solar system order [10][11][12][13][14]. Of the post GR models where the coupling is not separable are called non-minimally coupled theory (NMCT) [15][16][17][18][19][20][21][22]. It appears that for non-minimally coupled theory, it will be difficult to find an algorithm to construct the EMT.…”
Section: Introductionmentioning
confidence: 99%
“…Compared to f (R) theory, the field equations are second order instead of fourth one, which is an important advantage of f (T ) theory. As a further extension, and an analogy to that of f (R) theories [15][16][17][18][19][20][21][22][23][24][25][26][27][28][29], non-minimal torsion-matter coupling f (T ) gravity has been proposed and studied [30]. In the previous research [31], using the observation data of type Ia supernovae (SNeIa), cosmic microwave background (CMB), and baryon acoustic oscillations (BAO), we established two concrete f (T ) models with non-minimal torsion-matter coupling extension, and we found that they are successful in describing the observation of the Universe and its large-scale structure and evolution.…”
Section: Introductionmentioning
confidence: 99%