Comment to ``Quantization of FRW spacetimes in the presence of a cosmological constant and radiation''

Details Comment to ``Quantization of FRW spacetimes in the presence of a cosmological constant and radiation'' Comment to ``Quantization of FRW spacetimes in the presence of a cosmological constant and radiation''

2006-11-04

arxiv.org/abs/gr-qc/0611029v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, 3 figures, 2 tables Changes in the figures

Scientific paper

10.1103/PhysRevD.75.068503

The quantization of the Friedmann-Robertson-Walker spacetime in the presence of a negative cosmological constant was used in a recent paper to conclude that there are solutions that avoid singularities (big bang--big crunch) at the quantum level. We show that a proper study of their model{\sl does not prevent} the occurrence of singularities at the quantum level, in fact the quantum probability of such event is larger than the classical one. Our numerical simulations based on the powerful variational sinc collocation method (VSCM) also show that the precision of the results of that paper is much lower than the 20 significant digits reported by the authors.

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