The hypothesis of cosmic censorship (CCH) plays a crucial
role in classical General Relativity, namely to ensure that naked singularities
would never emerge, in which case phenomena beyond our understanding and
ability to predict could occur. More than 40 years after it was first proposed,
the validity of the hypothesis remains an open question. Here CCH gets reconsidered
in both its weak and strong version, concerning point-like singularities, with
respect to the provisions of Heisenberg’s uncertainty principle. It is argued
that the shielding of the singularities from observers at infinity by an event
horizon is also quantum mechanically favored, but ultimately it seems more
appropriate to accept that singularities never actually form in the usual
sense, thus no naked singularity danger exists in the first place.
Author(s) Details Nikolaos Pappas
Division of Theoretical Physics, Department of Physics, University of Ioannina, Ioannina GR-45110, Greece and Department of Physics, University of Thessaly, Lamia, GR-35100, Greece
View Book :- http://bp.bookpi.org/index.php/bpi/catalog/book/193
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