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| Format: | Recurso digital |
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Zenodo
2025
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| Online Access: | https://doi.org/10.5281/zenodo.18225746 |
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Table of Contents:
- <p>We propose a theoretical framework for a class of astrophysical objects referred to as<br>black stars: ultracompact configurations that are gravitationally stable without possessing<br>classical event horizons. In this approach, spacetime curvature and gravitational response<br>emerge from an underlying vacuum dynamics, while electromagnetic radiation undergoes<br>non-dissipative spectral confinement driven by a dual resonance mechanism. As a result,<br>these objects appear observationally black not due to causal disconnection, but due to spec-<br>tral trapping and redistribution beyond detectable frequency bands. This framework provides<br>an alternative interpretation of compact dark objects that avoids singularities, preserves in-<br>formation, and remains compatible with effective field-theoretic descriptions of gravity and<br>electromagnetism.</p>