Exact space-time symmetry conservation and automatic mesh refinement for classical lattice field theory

Fuente: arXiv
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Autori principali: Rothkopf, A., Horowitz, W. A., Nordström, J.
Natura: Preprint
Pubblicazione: 2024
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author Rothkopf, A.
Horowitz, W. A.
Nordström, J.
author_facet Rothkopf, A.
Horowitz, W. A.
Nordström, J.
contents The breaking of space-time symmetries and the non-conservation of the associated Noether charges constitutes a central artifact in lattice field theory. In prior work we have shown how to overcome this limitation for classical actions describing point particle motion, using the world-line formalism of general relativity. The key is to treat coordinate maps (from an abstract parameter space into space-time) as dynamical and dependent degrees of freedom, which remain continuous after discretization of the underlying parameter space. Here we present latest results where we construct a reparameterization invariant classical action for scalar fields, which features dynamical coordinate maps. We highlight the following achievements of our approach: 1) global space-time symmetries remain intact after discretization and the associated Noether charges remain exactly preserved 2) coordinate maps adapt to the dynamics of the scalar field leading to adaptive grid resolution guided by the symmetries.
format Preprint
id arxiv_https___arxiv_org_abs_2410_05896
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Exact space-time symmetry conservation and automatic mesh refinement for classical lattice field theory
Rothkopf, A.
Horowitz, W. A.
Nordström, J.
High Energy Physics - Lattice
Numerical Analysis
The breaking of space-time symmetries and the non-conservation of the associated Noether charges constitutes a central artifact in lattice field theory. In prior work we have shown how to overcome this limitation for classical actions describing point particle motion, using the world-line formalism of general relativity. The key is to treat coordinate maps (from an abstract parameter space into space-time) as dynamical and dependent degrees of freedom, which remain continuous after discretization of the underlying parameter space. Here we present latest results where we construct a reparameterization invariant classical action for scalar fields, which features dynamical coordinate maps. We highlight the following achievements of our approach: 1) global space-time symmetries remain intact after discretization and the associated Noether charges remain exactly preserved 2) coordinate maps adapt to the dynamics of the scalar field leading to adaptive grid resolution guided by the symmetries.
title Exact space-time symmetry conservation and automatic mesh refinement for classical lattice field theory
topic High Energy Physics - Lattice
Numerical Analysis
url https://arxiv.org/abs/2410.05896