Spectral representation of lattice gluon and ghost propagators at zero temperature
We consider the analytic continuation of Euclidean propagator data obtained from 4D simulations to Minkowski space. In order to perform this continuation, the common approach is to first extract the Källén-Lehmann spectral density of the field. Once this is known, it can be extended to Minkowski spa...
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doaj-6db9a6429278498f90a58370d595c3032020-11-25T02:40:03ZengElsevierNuclear Physics B0550-32132020-03-01952Spectral representation of lattice gluon and ghost propagators at zero temperatureDavid Dudal0Orlando Oliveira1Martin Roelfs2Paulo Silva3KU Leuven Campus Kortrijk–Kulak, Department of Physics, Etienne Sabbelaan 53 bus 7657, 8500 Kortrijk, Belgium; Ghent University, Department of Physics and Astronomy, Krijgslaan 281-S9, 9000 Gent, BelgiumCFisUC, Department of Physics, University of Coimbra, 3004-516 Coimbra, PortugalKU Leuven Campus Kortrijk–Kulak, Department of Physics, Etienne Sabbelaan 53 bus 7657, 8500 Kortrijk, Belgium; Corresponding author.CFisUC, Department of Physics, University of Coimbra, 3004-516 Coimbra, PortugalWe consider the analytic continuation of Euclidean propagator data obtained from 4D simulations to Minkowski space. In order to perform this continuation, the common approach is to first extract the Källén-Lehmann spectral density of the field. Once this is known, it can be extended to Minkowski space to yield the Minkowski propagator. However, obtaining the Källén-Lehmann spectral density from propagator data is a well known ill-posed numerical problem. To regularise this problem we implement an appropriate version of Tikhonov regularisation supplemented with the Morozov discrepancy principle. We will then apply this to various toy model data to demonstrate the conditions of validity for this method, and finally to zero temperature gluon and ghost lattice QCD data. We carefully explain how to deal with the IR singularity of the massless ghost propagator. We also uncover the numerically different performance when using two—mathematically equivalent—versions of the Källén-Lehmann spectral integral.http://www.sciencedirect.com/science/article/pii/S0550321319303980 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
David Dudal Orlando Oliveira Martin Roelfs Paulo Silva |
spellingShingle |
David Dudal Orlando Oliveira Martin Roelfs Paulo Silva Spectral representation of lattice gluon and ghost propagators at zero temperature Nuclear Physics B |
author_facet |
David Dudal Orlando Oliveira Martin Roelfs Paulo Silva |
author_sort |
David Dudal |
title |
Spectral representation of lattice gluon and ghost propagators at zero temperature |
title_short |
Spectral representation of lattice gluon and ghost propagators at zero temperature |
title_full |
Spectral representation of lattice gluon and ghost propagators at zero temperature |
title_fullStr |
Spectral representation of lattice gluon and ghost propagators at zero temperature |
title_full_unstemmed |
Spectral representation of lattice gluon and ghost propagators at zero temperature |
title_sort |
spectral representation of lattice gluon and ghost propagators at zero temperature |
publisher |
Elsevier |
series |
Nuclear Physics B |
issn |
0550-3213 |
publishDate |
2020-03-01 |
description |
We consider the analytic continuation of Euclidean propagator data obtained from 4D simulations to Minkowski space. In order to perform this continuation, the common approach is to first extract the Källén-Lehmann spectral density of the field. Once this is known, it can be extended to Minkowski space to yield the Minkowski propagator. However, obtaining the Källén-Lehmann spectral density from propagator data is a well known ill-posed numerical problem. To regularise this problem we implement an appropriate version of Tikhonov regularisation supplemented with the Morozov discrepancy principle. We will then apply this to various toy model data to demonstrate the conditions of validity for this method, and finally to zero temperature gluon and ghost lattice QCD data. We carefully explain how to deal with the IR singularity of the massless ghost propagator. We also uncover the numerically different performance when using two—mathematically equivalent—versions of the Källén-Lehmann spectral integral. |
url |
http://www.sciencedirect.com/science/article/pii/S0550321319303980 |
work_keys_str_mv |
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