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• W2128497557 startingPage "1450061" @default.
• W2128497557 abstract "In this work, we consider a semiclassical description of the spherically symmetric gravitational collapse with a massless scalar field. In particular, we employ an effective scenario provided by holonomy corrections from loop quantum gravity, to the homogeneous interior spacetime. The singularity that would arise at the final stage of the corresponding classical collapse, is resolved in this context and is replaced by a bounce. Our main purpose is to investigate the evolution of trapped surfaces during this semiclassical collapse. Within this setting, we obtain a threshold radius for the collapsing shells in order to have horizons formation. In addition, we study the final state of the collapse by employing a suitable matching at the boundary shell from which quantum gravity effects are carried to the exterior geometry." @default.
• W2128497557 created "2016-06-24" @default.
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• W2128497557 date "2014-06-01" @default.
• W2128497557 modified "2023-10-02" @default.
• W2128497557 title "Semiclassical dynamics of horizons in spherically symmetric collapse" @default.
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• W2128497557 doi "https://doi.org/10.1142/s0218271814500618" @default.
• W2128497557 hasPublicationYear "2014" @default.
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