Analysis of different scenarios with new Tsallis holographic dark energies and bulk viscous fluid in the framework of Chern-Simons modified gravity

Ranjit C., Islam S., Chattopadhyay S., GÜDEKLİ E.

International Journal of Modern Physics A, cilt.36, 2021 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 36
  • Basım Tarihi: 2021
  • Doi Numarası: 10.1142/s0217751x21501517
  • Dergi Adı: International Journal of Modern Physics A
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Environment Index, INSPEC, zbMATH
  • Anahtar Kelimeler: New Tsallis holographic dark energy, bulk viscosity, scale factor, Chern-Simons framework, PROBE WMAP OBSERVATIONS, VISCOSITY, LAMBDA, MODEL, ACCELERATION, COSMOLOGY, RELEASE
  • İstanbul Üniversitesi Adresli: Evet

Özet

© 2021 World Scientific Publishing Company.In this work, we have studied various cosmological parameters in the presence of viscous new Tsallis holographic dark energies for interacting scenarios in the framework of Chern-Simons modified gravity. The bulk viscosity has been considered with the bulk viscous pressure chosen in the form =-3H(ζ0 + ζ1H + ζ2 + H2)). Hubble parameter H has been obtained from the above choice of scale factor and in this viscous scenario, the effective pressure has been obtained in Chern-Simons framework whose field equation, cosmological consequences have been investigated. It has been observed that for the interaction scenario in the presence of bulk viscosity the EoS parameter is staying above-1, which indicates quintessence behavior. Hence, for the universe filled with a bulk viscous fluid can have the possibility of avoidance of big-rip, although the earlier transition from quintessence to phantom is not avoidable.