Gravitational Bounce from the Quantum Exclusion Principle
Enrique Gaztanaga, K. Sravan Kumar, Swaraj Pradhan, Michael Gabler

TL;DR
This paper models how quantum principles prevent singular collapse in gravitational systems, leading to a bounce and inflation-like expansion, which predicts a small non-zero spatial curvature detectable by future surveys.
Contribution
It introduces a relativistic collapse model incorporating quantum exclusion, demonstrating a bounce that unifies black hole interiors, inflation, and dark energy phenomena.
Findings
Gravitational bounce occurs at a specific radius due to quantum effects.
The model predicts a small negative spatial curvature, -0.07 to -0.05.
Bounce confined within the initial gravitational radius, mimicking a cosmological constant.
Abstract
We investigate the fully relativistic spherical collapse model of a uniform distribution of mass with initial comoving radius and spatial curvature representing an over-density or bounded perturbation within a larger background. Our model incorporates a perfect fluid with an evolving equation of state, , which asymptotically transitions from pressureless dust () to a ground state characterized by a uniform, time-independent energy density . This transition is motivated by the quantum exclusion principle, which prevents singular collapse, as observed in supernova core-collapse explosions. We analytically demonstrate that this transition induces a gravitational bounce at a radius . The bounce leads to an exponential expansion phase, where behaves…
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