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/

Zendy Open

Presents the pdf analysis as premium feature

PDF Analysis

Insights

Presents the summarisation as premium feature

Summarisation

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the zaia usage as premium feature

ZAIA

Zendy Tools

Zendy Plus

Presents the access of premium content as premium feature

Premium Content

Traversable wormholes, studied by Morris and Thorne \cite{Morris1} in generalrelativity, are investigated in this research paper in $f(R,T)$ gravity byintroducing a new form of non-linear $f(R,T)$ function. By using this novelfunction, the Einstein's field equations in $f(R,T)$ gravity are derived. Toobtain the exact wormhole solutions, the relations $p_t=\omega\rho$ and$p_r=\sinh(r)p_t$, where $\rho$ is the energy density, $p_r$ is the radialpressure and $p_t$ is the tangential pressure, are used. Other than theserelations, two forms of shape function defined in literature are used, andtheir suitability is examined by exploring the regions of validity of null,weak, strong and dominant energy conditions . Consequently, the radius of thethroat or the spherical region, with satisfied energy conditions, is determinedand the presence of exotic matter is minimized.

Static Traversable Wormholes in $f(R, T)=R+2\alpha \ln T$ Gravity