English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

In this paper we study two different cases of inhomogeneous EOS of the formp_d = \omega(t)\rho_d+w_1 f(H, t) . We derive the energy density of dark fluidand dark matter component for both the cases. Further we calculate theevolution of energy density, gravitational constant and cosmological constant.We also explore the finite time singularity and thermodynamic stabilityconditions for the two cases of EOS. Finally, we discuss the thermodynamics ofinhomogeneous EOS with the derivation of internal energy, Temperature andentropy and also show that all the stability conditions are satisfied for thetwo cases of EOS

Energy conditions for Inhomogeneous EOS and its Thermodynamics analysis with the resolution on finite time future singularity problems