Emergent Inflation and Cosmological Perturbations from Graph Spectral Geometry

Presented is a minimal model in which spacetime, inflation, and primordial fluctuations emergefrom the dynamics of a discrete graph system. The fundamental degrees of freedom are encoded ina time-dependent adjacency matrix with a simple Hamiltonian governed by connectivity and acritical density parameter. Demonstrated is, that (i) a stable fixed point of the graph dynamicsinduces an inflationary phase, (ii) cosmological perturbations arise from fluctuations of the graphLaplacian spectrum, and (iii) the primordial power spectrum is directly determined by the spectraldensity of the graph. In the infrared limit, the model reproduces Einstein gravity via a spectralaction. Observable quantities such as the spectral index, its running, tensor modes, and non-Gaussianity are derived analytically and linked to geometric properties of the underlying graph. Theframework unifies aspects of discrete quantum gravity, renormalization group flows, and emergentspacetime.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-04-20
DOI
https://doi.org/10.5281/zenodo.19662610
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
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article

Emergent Inflation and Cosmological Perturbations from Graph Spectral Geometry

Holger Döring
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Emergent Inflation and Cosmological Perturbations from Graph Spectral Geometry

Holger Döring
article en

Abstract

Presented is a minimal model in which spacetime, inflation, and primordial fluctuations emergefrom the dynamics of a discrete graph system. The fundamental degrees of freedom are encoded ina time-dependent adjacency matrix with a simple Hamiltonian governed by connectivity and acritical density parameter. Demonstrated is, that (i) a stable fixed point of the graph dynamicsinduces an inflationary phase, (ii) cosmological perturbations arise from fluctuations of the graphLaplacian spectrum, and (iii) the primordial power spectrum is directly determined by the spectraldensity of the graph. In the infrared limit, the model reproduces Einstein gravity via a spectralaction. Observable quantities such as the spectral index, its running, tensor modes, and non-Gaussianity are derived analytically and linked to geometric properties of the underlying graph. Theframework unifies aspects of discrete quantum gravity, renormalization group flows, and emergentspacetime.

Zenodo (CERN European Organization for Nuclear Research)
Technische Universität Berlin (DE)
Openalex Percentile: Top 7%
Cosmology and Gravitation Theories
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Emergent Inflation and Cosmological Perturbations from Graph Spectral Geometry — Holger Döring · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS