Noether symmetry for Gauss–Bonnet dilatonic gravity

被引:0
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作者
Abhik Kumar Sanyal
Claudio Rubano
Ester Piedipalumbo
机构
[1] Jangipur College,Department of Physics
[2] Complesso Universitario di Monte S. Angelo,Dipartimento di Scienze Fisiche
[3] Complesso Universitario di Monte S. Angelo,Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
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Theoretical cosmology; Dark energy; Observational cosmology;
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摘要
Noether symmetry for Gauss–Bonnet Dilatonic interaction exists for a constant dilatonic scalar potential and a linear functional dependence of the coupling parameter on the scalar field. The symmetry with the same form of the potential and coupling parameter exists all in the vacuum, radiation and matter dominated era. The late time acceleration is driven by the effective cosmological constant rather than the Gauss–Bonnet term, while the later compensates for the large value of the effective cosmological constant giving a plausible answer to the well-known coincidence problem.
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页码:2807 / 2820
页数:13
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