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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In this article, we have examined the existence of a static sphericallysymmetric solution in the Scalar Tensor Vector Gravity (STVG) and investigatedits horizon distances to develop boundary limitations for our test particle. Wehave computed the Kretschmann invariant of the metric to study thesingularities and verify that it reduces to general relativity's Kretschmanninvariant as $\alpha\rightarrow0$. Further, we investigated the orbital motionof a time-like and light-like test particle around the static solution bydeveloping an effective potential and the radius of the innermost stablecircular orbit (ISCO).

Orbital Motion of a test particle around a Schwarzschild's Black Hole in STVG gravity