Singularity avoidance and time in quantum gravity
Andreas Kreienbuehl

TL;DR
This paper investigates quantum cosmology by quantizing a Friedmann-Robertson-Walker universe, showing that the choice of time variable influences the presence of singularities, with no semiclassical wave packet avoiding the Big Bang.
Contribution
It introduces a reduced square root Hamiltonian using the scale factor as time and analyzes its implications for singularity avoidance in quantum gravity.
Findings
No semiclassical wave packet avoids the Big Bang singularity
The choice of time variable affects singularity resolution
Quantization leads to a spinor equation in quantum cosmology
Abstract
We consider the quantization of a Friedmann-Robertson-Walker universe. We derive a reduced square root Hamiltonian by choosing the scale factor as time variable and quantize the theory using the Dirac method. From the resulting spinor equation we show that there is no semiclassical wave packet that avoids the Big Bang singularity. Our work raises the question concerning the relationship between the choice of time and singularity avoidance.
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