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We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward-like solutions of Einstein's field equations according to the formalism known as Horizon Quantum Mechanics.
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For the sake of completeness: the singularity theorems tell us nothing about the nature of this singularity (for a recent review on the topic, see [ 3 ] ), indeed they are not forced to be curvature singularities if we move away from the spherically symmetric case
Cited in the paper.
We write ℏ = ℓ P m P \hbar=\ell_{\rm P}m_{\rm P} and G N = ℓ P / m P G_{\rm N}=\ell_{\rm P}/m_{\rm P} in Planck units. Nonetheless, we assume c = 1 c=1
Cited in the paper.
R. Casadio, Localised particles and fuzzy horizons: A tool for probing Quantum Black Holes
Cited in the paper.
2017
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R. Casadio, A. Giugno and A. Giusti, Global and Local Horizon Quantum Mechanics , Gen. Rel. Grav. 49
2017
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R. Casadio, A. Giugno, A. Giusti and O. Micu, Horizon Quantum Mechanics of Rotating Black Holes , Eur. Phys. J. C 77
2017
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R. Casadio, A. Giugno, A. Giusti and M. Lenzi, Quantum corpuscular corrections to the Newtonian potential , Phys. Rev. D 96
2017
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