# Discrete fuzzy de Sitter cosmology

**Authors:** Maja Buric, Dusko Latas

arXiv: 1903.08378 · 2019-07-31

## TL;DR

This paper investigates a noncommutative de Sitter cosmological model revealing a discrete, logarithmically distributed time spectrum and a resolution to the big bang singularity through a bounded universe radius.

## Contribution

It introduces a novel analysis of time as a non-self-adjoint operator with self-adjoint extensions in a noncommutative de Sitter framework, showing discrete eigenvalues and singularity resolution.

## Key findings

- Time spectrum is discrete with logarithmic eigenvalue distribution.
- Universe radius is bounded below, resolving the big bang singularity.
- Model exhibits symmetry breaking at the Planck scale.

## Abstract

We analyze the spectrum of time observable in noncommutative cosmological model introduced in [5], defined by $(\rho, s=\frac 12)\,$ representation of the de Sitter group. We find that time has peculiar property: it is not self-adjoint, but appropriate restrictions to the space of physical states give self-adjoint extensions. Extensions have discrete spectrum with logarithmic distribution of eigenvalues, $\,t_n \sim \ell\, \log\, n$+const, where $\ell$ characterizes noncommutativity and the usual assumption is $\,\ell=\ell_{Planck}$. When calculated on physical states, radius of the universe is bounded below by $\, \ell\, \sqrt{\frac 34\, \left( \frac 14 +\rho^2\right)}\, $, which resolves the big bang singularity. An immediate consequence of the model is a specific breaking of the original symmetry at the Planck scale.

## Full text

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## Figures

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## References

21 references — full list in the complete paper: https://tomesphere.com/paper/1903.08378/full.md

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Source: https://tomesphere.com/paper/1903.08378