Anisotropic Model with Constant Jerk Parameter in <i>f</i> (<i>R</i>, <i>T</i>) Gravity

Tiwari R. K., SOFUOĞLU D., Mishra S. K., Beesham A.

GRAVITATION & COSMOLOGY, cilt.28, sa.2, ss.196-203, 2022 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 28 Sayı: 2
  • Basım Tarihi: 2022
  • Doi Numarası: 10.1134/s0202289322020141
  • Dergi Adı: GRAVITATION & COSMOLOGY
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, zbMATH
  • Sayfa Sayıları: ss.196-203
  • İstanbul Üniversitesi Adresli: Evet

Özet

In the context of f (R, T) modified gravity theory, we consider a homogeneous and anisotropic Bianchi type-I cosmological model which relies on the condition of a constant jerk parameter, j = 1, corresponding to a flat Lambda CDM model. Under this condition, we obtain two different solutions, one is power-law and the other one is exponential. The power-law solution gives a decelerating model, while the exponential one yields an accelerating cosmology. We discuss the physical and geometric properties of both models, validity of the solutions, and the significance of modified f (R, T) gravity for the models.