Lorentz violation with an invariant minimum speed as foundation of the Gravitational Bose Einstein Condensate of a Dark Energy Star
arXiv:2009.03737 · doi:10.1016/j.dark.2019.100454
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 slightly larger than and slightly smaller than the core radius of GBEC, where the metric of the repulsive sector (core of GBEC) would diverge for , so that for such a given radius of phase coexistence , both divergences at of Schwarzschild metric and at of the repulsive core are eliminated, thus preventing the formation of the event horizon. So the causal structure of SSR helps us to elucidate such puzzle of singularity of event horizon by also providing a quantum interpretation for GBEC and thus by explaining the origin of a strong anisotropy due to the minimum speed that leads to the phase transition gravity/anti-gravity during the collapse of the star. Furthermore, due to the absence of an event horizon of black hole (BH) where any signal cannot propagate, the new collapsed structure presents a signal propagation in its region of coexistence of phases where the coexistence metric does not diverge.
arXiv comment18 pages. 6 figures
References in corpus (20)
- Shapiro delay measurement of a two solar mass neutron star
- Gravastars must have anisotropic pressures
- Stable dark energy stars
- How to tell a gravastar from a black hole
- No observational proof of the black-hole event-horizon
- Quantum Phase Transitions and the Breakdown of Classical General Relativity
- Gravastar Solutions with Continuous Pressures and Equation of State
- Gravitational Collapse with a Cosmological Constant
- Gravastar energy conditions revisited
- Anisotropic dark energy stars
- Star Models with Dark Energy
- Deformed Special Relativity with an energy barrier of a minimum speed
- Doubly Special Relativity with a minimum speed and the search for a quantum gravity at low energies
- Coexisting vacua and effective gravity
- Doubly Special Relativity with a minimum speed and the Uncertainty Principle
- An explanation for the tiny value of the cosmological constant and the low vacuum energy density
- Horizon closeness bounds for static black hole mimickers
- Testing Lorentz symmetry violation with an invariant minimum speed
- Lorentz violation with a universal minimum speed as foundation of de Sitter relativity
- Lorentz violation with an invariant minimum speed as foundation of the uncertainty principle in Minkowski, dS and AdS spaces
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- Bose-Einstein Condensate dark matter models in the presence of baryonic matter and random confining potentials
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- Graviton mass due to dark energy as a superconducting medium: theoretical and phenomenological aspects
- GUP, Lorentz Invariance (Non)-Violation, and Non-Commutative Geometry