Cosmological implications of 5-dimensional Brans–Dicke theory

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Title: Cosmological implications of 5-dimensional Brans–Dicke theory
Authors: Qiang, Li-e1, Gong, Yan1,2, Ma, Yongge3, Chen, Xuelei1,4 xuelei@cosmology.bao.ac.cn
Source: Physics Letters B. Nov2009, Vol. 681 Issue 3, p210-213. 4p.
Subjects: Gravitational fields, Metaphysical cosmology, Dimensional analysis, Celestial mechanics, Scalar field theory, Acceleration (Mechanics), Cataclysmic variable stars, Coupling constants
Abstract: Abstract: The five-dimensional Brans–Dicke theory naturally provides two scalar fields by the Killing reduction mechanism. These two scalar fields could account for the accelerated expansion of the universe. We test this model and constrain its parameter by using the type Ia supernova (SN Ia) data. We find that the best fit value of the 5-dimensional Brans–Dicke coupling constant is . This result is also consistent with other observations such as the baryon acoustic oscillation (BAO). [Copyright &y& Elsevier]
Copyright of Physics Letters B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: <searchLink fieldCode="JN" term="%22Physics+Letters+B%22">Physics Letters B</searchLink>. Nov2009, Vol. 681 Issue 3, p210-213. 4p.
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  Label: Abstract
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  Data: Abstract: The five-dimensional Brans–Dicke theory naturally provides two scalar fields by the Killing reduction mechanism. These two scalar fields could account for the accelerated expansion of the universe. We test this model and constrain its parameter by using the type Ia supernova (SN Ia) data. We find that the best fit value of the 5-dimensional Brans–Dicke coupling constant is . This result is also consistent with other observations such as the baryon acoustic oscillation (BAO). [Copyright &y& Elsevier]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Physics Letters B is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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      – Type: doi
        Value: 10.1016/j.physletb.2009.10.028
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      – Code: eng
        Text: English
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      – SubjectFull: Gravitational fields
        Type: general
      – SubjectFull: Metaphysical cosmology
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      – SubjectFull: Dimensional analysis
        Type: general
      – SubjectFull: Celestial mechanics
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      – SubjectFull: Scalar field theory
        Type: general
      – SubjectFull: Acceleration (Mechanics)
        Type: general
      – SubjectFull: Cataclysmic variable stars
        Type: general
      – SubjectFull: Coupling constants
        Type: general
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      – TitleFull: Cosmological implications of 5-dimensional Brans–Dicke theory
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              Text: Nov2009
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              Y: 2009
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