Spherically Symmetric, Self-Similar Spacetimes
Sanjay M. Wagh, Keshlan S. Govinder

TL;DR
This paper demonstrates that spherically symmetric, self-similar spacetimes necessarily have a separable metric form, are uniquely characterized, and can include matter with any equation of state, relevant to cosmology and gravitational collapse.
Contribution
It proves that self-similarity in spherically symmetric spacetimes implies metric separability and uniqueness, expanding understanding of their geometric and physical properties.
Findings
Self-similar spherically symmetric spacetimes have separable metrics.
Such spacetimes are uniquely characterized by a specific metric form.
They can include matter with arbitrary equations of state.
Abstract
Self-similar spacetimes are of importance to cosmology and to gravitational collapse problems. We show that self-similarity or the existence of a homothetic Killing vector field for spherically symmetric spacetimes implies the separability of the spacetime metric in terms of the co-moving coordinates and that the metric is, uniquely, the one recently reported in [cqg1]. The spacetime, in general, has non-vanishing energy-flux and shear. The spacetime admits matter with any equation of state.
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