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A new class of self-gravitating collapsing star models with perfect fluiddistributions is discussed in this work. The paper has a comprehensive analysisof a homogeneous gravitational collapsing system wherein using aparametrization scheme for the expansion-scalar $(\Theta )$, the solutions ofthe Einstein Field Equations (EFEs) are determined independently. Thebackground geometry for the analysis is considered to be homogeneous andisotropic represented by a Friedmann-Leimatre-Robertson-Walker (FLRW) metricand by employing the boundary conditions, we have discussed the solution inmore detail. Further, all the physical and geometrical parameters are obtainedin terms of Schwarzschild mass $(M)$ that makes the model significant inastrophysical applications. The singularity analysis of the collapsing systemis also discussed by the apparent-horizon, and it has seen that the homogenousgravitational collapse turns into a new kind of scenario- Eternal collapsingobject.

Eternal homogeneous gravitational collapse: A comprehensive analysis from $\Theta$ parametrization