Lorentz violation with an invariant minimum speed as foundation of the Gravitational Bose Einstein Condensate of a Dark Energy Star
Claudio Nassif Cruz, Rodrigo Francisco dos Santos, and A. C. Amaro de, Faria Jr

TL;DR
This paper explores a novel model of dark energy stars using an invariant minimum speed from Symmetrical Special Relativity, proposing a phase transition that prevents event horizon formation and eliminates singularities.
Contribution
It introduces a new framework connecting Lorentz violation and minimum speed to the structure of gravastars, replacing traditional singularity-based models with a phase transition approach.
Findings
Proposes a phase transition mechanism avoiding event horizon singularities.
Links SSR's invariant minimum speed to the internal structure of dark energy stars.
Suggests a quantum interpretation for gravitational Bose Einstein condensates.
Abstract
We aim to search for the connection between the spacetime with an invariant minimum speed so-called Symmetrical Special Relativity (SSR) with Lorentz violation and the Gravitational Bose Einstein Condensate (GBEC) as the central core of a star of gravitational vacuum (gravastar), where one normally introduces a cosmological constant for representing an anti-gravity. This usual model of gravastar with an equation of state (EOS) for vacuum energy inside the core will be generalized for many modes of vacuum (dark energy star) in order to circumvent the embarrassment generated by the horizon singularity as the final stage of a gravitational collapse. In the place of the problem of a singularity of an event horizon, we introduce a phase transition between gravity and anti-gravity before reaching the Schwarzschild (divergent) radius for a given coexistence radius …
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