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Feng, B., et al. (2005) Dark Energy Constraints from the Cosmic Age and Supernova. Physics Letters B, 607, 35-41.
https://doi.org/10.1016/j.physletb.2004.12.071

has been cited by the following article:

• TITLE: Late Time Behavior of the Cosmological Model in Modified Theory of Gravity

  AUTHORS: Sankarsan Tarai, Jagadish Kumar

  KEYWORDS: f (R, T) Gravity, Bianchi Type VIh, Perfect Fluid

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.8 No.4, October 13, 2022

  ABSTRACT: We report a viable exponential gravity model for the accelerated expansion of the universe in Bianchi VIh space-time. By considering the estimated physical parameters, the cosmological models are constructed and analyzed in detail. We found that the state parameter in both the models increases to a higher negative range in an early epoch of the phantom domain and it goes to the positive domain at a late phase of the evolution. The effective cosmological constant remains in a positive domain for both models, which is a good sign of accelerating expansion of the universe.