Some exact solutions in f(G,T)\mathcal{f(G},T) gravity via Noether symmetries

Apr 26, 2017
16 pages
Published in:
  • Mod.Phys.Lett.A 32 (2017) 16, 1750086
  • Published: Apr 26, 2017
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Abstract: (WSP)
This paper is devoted to investigate the recently proposed modified Gaussā€“Bonnet f(š¯’¢,T) gravity, with š¯’¢, the Gaussā€“Bonnet term, coupled with T, the trace of energyā€“momentum tensor. We have used the Noether symmetry methodology to discuss some cosmologically important f(š¯’¢,T) gravity models with anisotropic background. In particular, the Noether symmetry equations for modified f(š¯’¢,T) gravity are reported for locally rotationally symmetric Bianchi type I universe. Explicitly, two models have been proposed to explore the exact solutions and the conserved quantities. It is concluded that the specific models of modified Gaussā€“Bonnet gravity may be used to reconstruct Ī›CDM cosmology without involving any cosmological constant.
Note:
  • 21 pages, 8 figures
  • 04.20.Jb
  • 98.80.Jk
  • f(š¯’¢,T) gravity
  • Noether symmetries
  • Ī›CDM
  • symmetry: Noether
  • gravitation: model
  • tensor: energy-momentum
  • background: anisotropy
  • dark matter
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