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Planck stars, White Holes, Remnants and Planck-mass quasi-particles. The quantum gravity phase in black holes' evolution and its manifestations
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This is a review of some recent developments on quantum gravity aspects of black hole physics. In particular, we focus on a scenario leading to the prediction of the existence of a Planck-mass quasi-stable object, that could form a component of dark matter.
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Cited by 6 Pith papers
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Loopy Black-Hole Remnants
Within a covariant effective loop quantum gravity model, black holes evaporate asymptotically to a minimum-area remnant of mass ~20.94 μg that cannot form in finite time.
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Thermodynamics of black and white holes in ensemble of Planckons
A toy model counting pairs of Planckons gives integer black hole entropy, negative white hole entropy, charge-independent Reissner-Nordstrom entropy, and a quantized cosmological constant.
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Love Numbers of Covariant Loop Quantum Black Holes
Tidal Love numbers of three covariant loop quantum black holes are shown to be generically nonzero, Planck-scale suppressed, and model-dependent in sign and logarithmic running.
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Singularity Avoidance in Gravitational Collapse of an Inhomogeneous Fluid in Rastall Gravity
An inhomogeneous collapsing cloud in Rastall gravity can be made to bounce at a finite minimum radius, while satisfying the weak energy condition, by tuning the Rastall parameter and free functions.
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Echoes of Love Beyond the Horizon: A Bridge to Recovering Information from Black Holes
Black holes may acquire Planck-suppressed tidal Love numbers from quantum gravity, which the authors argue could carry information about the initial collapse and help resolve the information loss paradox.
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De Sitter Cores from Nonlocal Quantum Field Theories
An exponential nonlocal regulator maps a point mass to a Gaussian density whose Einstein solution has a de Sitter core, reproducing (with new labeling) the known Gaussian-sourced regular black hole.
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