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Taser D., ULU DOĞRU M.
New Astronomy, vol.86, 2021 (SCI-Expanded)
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Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Aerospace Database, Communication Abstracts, INSPEC, Metadex, Civil Engineering Abstracts
Einstein-Rosen Universe, Scalar field, Quintessence matter, Phantom field, F R, INFLATIONARY UNIVERSE, T) GRAVITY, INHOMOGENEOUS COSMOLOGY, MODELS, SINGULARITIES, FLATNESS, HORIZON, FLUID
Çanakkale Onsekiz Mart University Affiliated:
© 2021 Elsevier B.V.Non-static Einstein–Rosen universe with scalar field is examined via two different selection of f(R,T) models. Firstly, we analyzed Einstein–Rosen universe with scalar field in f(R,T)=R+2f(T) model. Then, we constructed field equations for f(R,T)=f1(R)+f2(R)f3(T) model, as well. For both models, exact solutions of field equations have been attained without considering any approximation or restriction. Whether scalar field corresponds to phantom and/or quintessence scalar field are investigated for each models.