Quantization of Big Bang in crypto-Hermitian Heisenberg picture
Miloslav Znojil

TL;DR
This paper proposes a background-independent quantum model of the Universe near the Big Bang, using a simplified toy model to interpret the singularity as a quantum phase transition with novel operator properties.
Contribution
It introduces a new approach to quantizing the Big Bang using non-Hermitian operators and quantum phase transitions, replacing classical singularity regularizations.
Findings
The operator $Q(t)$ remains self-adjoint during the Eon.
The Big Bang is modeled as a quantum phase transition at an exceptional point.
Operator $Q(t)$ becomes non-diagonalizable at the singularity.
Abstract
A background-independent quantization of the Universe near its Big Bang singularity is considered using a drastically simplified toy model. Several conceptual issues are addressed. (1) The observable spatial-geometry characteristics of our empty-space expanding Universe is sampled by the time-dependent operator of the distance between two space-attached observers (``Alice and Bob''). (2) For any pre-selected guess of the simple, non-covariant time-dependent observable one of the Kato's exceptional points (viz., ) is postulated {\em real-valued}. This enables us to treat it as the time of Big Bang. (3) During our ``Eon'' (i.e., at all ) the observability status of operator is mathematically guaranteed by its self-adjoint nature with respect to an {\em ad hoc} Hilbert-space metric . (4) In adiabatic…
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