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 𝜙4 interaction. 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
6 May 2023
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 𝜙4 interaction. 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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Published date: 6 May 2023
Keywords:
Lattice Quantum Field Theory, Holographic Cosmology, Multilevel, Finite-size scaling
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Local EPrints ID: 481355
URI: http://eprints.soton.ac.uk/id/eprint/481355
PURE UUID: 7670f4d8-8654-4b9f-8af1-d6e1576fd907
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Date deposited: 23 Aug 2023 17:05
Last modified: 17 Mar 2024 03:27
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Author:
Benjamin Thomas Kitching-Morley
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