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A first study on the infrared properties of holographic models of cosmology using lattice-quantum-field theory simulations.

A first study on the infrared properties of holographic models of cosmology using lattice-quantum-field theory simulations.
A first study on the infrared properties of holographic models of cosmology using lattice-quantum-field theory simulations.
Cosmic inflation, in which the early universe undergoes a short, violent expansion, has successfully described many phenomena, including the near scale-invariance of the Cosmic Microwave Background Radiation (CMB). However, inflation is not ultraviolet-complete and suffers from self-consistency issues. Holographic Cosmology is an alternative framework in which the early universe is described by a three-dimensional dual quantum field theory (QFT). Correlations in the CMB are predicted by two-point correlators of the energy-momentum tensor (EMT) of the dual theory. A perturbative treatment of holographic cosmology has proven competitive with inflation in fits to CMB data, however, a non-perturbative treatment is needed to test the theory against all multipoles of the CMB. Lattice QFT provides such an approach by regularizing theories through placing them on a finite spacetime lattice. In this thesis, we tackle three challenges in making predictions of holographic cosmology using a lattice-regulated dual QFT with scalar fields in the adjoint of SU(N) and a 𝜙interaction. First, we provide numerical evidence supporting a conjecture that a class of super-renormalizable theories, including holographic cosmology dual theories, is non-perturbatively infrared finite. This is necessary for holographic cosmology to be predictive and implies a resolution of the Big Bang singularity within the holographic cosmology framework. Secondly, we explore a novel approach to regulating ultraviolet divergences appearing in calculations of the two-point EMT correlator. In this approach, Laplace transforms of position-space lattice data offer cancellation of quadratic divergences appearing in momentum-space. We finally investigate the feasibility of using multilevel methods to reduce statistical noise in holographic dual two-point calculations. Holographic dualities necessitate correlator calculations to be done in the critical regime where the correlation length diverges. Through a novel study of the critical-scaling properties of the multilevel algorithm, using the 2D-Ising model, we demonstrate the unsuitability of the technique in this regime.
Lattice Quantum Field Theory, Holographic Cosmology, Multilevel, Finite-size scaling
University of Southampton
Kitching-Morley, Benjamin Thomas
2fae2631-6c01-4522-800f-44308ea5ecf1
Kitching-Morley, Benjamin Thomas
2fae2631-6c01-4522-800f-44308ea5ecf1
Juttner, Andreas
a90ff7c5-ae8f-4c8e-9679-b5a95b2a6247
Skenderis, Konstantinos
09f32871-ffb1-4f4a-83bc-df05f4d17a09

Kitching-Morley, Benjamin Thomas (2023) A first study on the infrared properties of holographic models of cosmology using lattice-quantum-field theory simulations. University of Southampton, Doctoral Thesis, 166pp.

Record type: Thesis (Doctoral)

Abstract

Cosmic inflation, in which the early universe undergoes a short, violent expansion, has successfully described many phenomena, including the near scale-invariance of the Cosmic Microwave Background Radiation (CMB). However, inflation is not ultraviolet-complete and suffers from self-consistency issues. Holographic Cosmology is an alternative framework in which the early universe is described by a three-dimensional dual quantum field theory (QFT). Correlations in the CMB are predicted by two-point correlators of the energy-momentum tensor (EMT) of the dual theory. A perturbative treatment of holographic cosmology has proven competitive with inflation in fits to CMB data, however, a non-perturbative treatment is needed to test the theory against all multipoles of the CMB. Lattice QFT provides such an approach by regularizing theories through placing them on a finite spacetime lattice. In this thesis, we tackle three challenges in making predictions of holographic cosmology using a lattice-regulated dual QFT with scalar fields in the adjoint of SU(N) and a 𝜙interaction. First, we provide numerical evidence supporting a conjecture that a class of super-renormalizable theories, including holographic cosmology dual theories, is non-perturbatively infrared finite. This is necessary for holographic cosmology to be predictive and implies a resolution of the Big Bang singularity within the holographic cosmology framework. Secondly, we explore a novel approach to regulating ultraviolet divergences appearing in calculations of the two-point EMT correlator. In this approach, Laplace transforms of position-space lattice data offer cancellation of quadratic divergences appearing in momentum-space. We finally investigate the feasibility of using multilevel methods to reduce statistical noise in holographic dual two-point calculations. Holographic dualities necessitate correlator calculations to be done in the critical regime where the correlation length diverges. Through a novel study of the critical-scaling properties of the multilevel algorithm, using the 2D-Ising model, we demonstrate the unsuitability of the technique in this regime.

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More information

Published date: 6 May 2023
Keywords: Lattice Quantum Field Theory, Holographic Cosmology, Multilevel, Finite-size scaling

Identifiers

Local EPrints ID: 481355
URI: http://eprints.soton.ac.uk/id/eprint/481355
PURE UUID: 7670f4d8-8654-4b9f-8af1-d6e1576fd907
ORCID for Benjamin Thomas Kitching-Morley: ORCID iD orcid.org/0000-0003-3150-401X
ORCID for Andreas Juttner: ORCID iD orcid.org/0000-0002-3978-0927
ORCID for Konstantinos Skenderis: ORCID iD orcid.org/0000-0003-4509-5472

Catalogue record

Date deposited: 23 Aug 2023 17:05
Last modified: 17 Mar 2024 03:27

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Contributors

Author: Benjamin Thomas Kitching-Morley ORCID iD
Thesis advisor: Andreas Juttner ORCID iD
Thesis advisor: Konstantinos Skenderis ORCID iD

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