2007
DOI: 10.1002/andp.200610230
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The conformal status of ο = -3/2 Brans-Dicke cosmology

Abstract: Following recent fit of supernovae data to Brans-Dicke theory which favours the model with ω = −3/2 [1] we discuss the status of this special case of Brans-Dicke cosmology in both isotropic and anisotropic framework. It emerges that the limit ω = −3/2 is consistent only with the vacuum field equations and it makes such a Brans-Dicke theory conformally invariant. Then it is an example of the conformal relativity theory which allows the invariance with respect to conformal transformations of the metric. Besides,… Show more

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Cited by 38 publications
(45 citation statements)
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“…An ω 0 = 0 Brans-Dicke theory [sometimes called "massive dilaton gravity" (Wands, 1994)] was originally proposed by (O' Hanlon, 1972) in order to generate a Yukawa term in the Newtonian limit and has been occasionally considered in the literature (Anderson, 1971;Barber, 2003;Dabrowski et al, 2007;Davidson, 2005;Deser, 1970;Fujii, 1982;O'Hanlon and Tupper, 1972). The field equations corresponding to the action (54) are…”
Section: A Metric Formalismmentioning
confidence: 99%
“…An ω 0 = 0 Brans-Dicke theory [sometimes called "massive dilaton gravity" (Wands, 1994)] was originally proposed by (O' Hanlon, 1972) in order to generate a Yukawa term in the Newtonian limit and has been occasionally considered in the literature (Anderson, 1971;Barber, 2003;Dabrowski et al, 2007;Davidson, 2005;Deser, 1970;Fujii, 1982;O'Hanlon and Tupper, 1972). The field equations corresponding to the action (54) are…”
Section: A Metric Formalismmentioning
confidence: 99%
“…The stringent observational bound resulting from the 2003 experiment with the Cassini spacecraft require that ∣ ω ∣ ≳ 40 000 [57, 418]. On the other hand, ω = −3/2 may be favored by cosmological observations and also offer a resolution of the Pioneer anomaly [85]. A possible resolution can be obtained by incorporating a Gauss-Bonnet term in the form of into the Brans-Dicke version of the Lagrangian Equation (6.12) with the choice of Equation (6.13), which may allow the Eddington parameter γ to be arbitrarily close to 1, while choosing an arbitrary value for ω [10].…”
Section: Efforts To Explain and Study The Anomalymentioning
confidence: 99%
“…Conformal transformations of the metric tensor [1] are interesting characteristics of the scalar-tensor theories of gravity [2][3][4][5], including its conformally invariant version [6][7][8][9]. The point is that these theories can be represented in the two conformally related frames: the Jordan frame in which the scalar field is non-minimally coupled to the metric tensor, and in the Einstein frame in which it is minimally coupled to the metric tensor.…”
Section: Introductionmentioning
confidence: 99%