Vacuum polarization energy for general backgrounds in one space dimension

For field theories in one time and one space dimensions we propose an efficient method to compute the vacuum polarization energy of static field configurations that do not allow a decomposition into symmetric and anti-symmetric channels. The method also applies to scenarios in which the masses of th...

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Main Author: H. Weigel
Format: Article
Language:English
Published: Elsevier 2017-03-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316308012
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spelling doaj-72cc3e4ff1a84a34a82811a03d41d6f02020-11-24T20:45:12ZengElsevierPhysics Letters B0370-26931873-24452017-03-01766C657010.1016/j.physletb.2016.12.055Vacuum polarization energy for general backgrounds in one space dimensionH. WeigelFor field theories in one time and one space dimensions we propose an efficient method to compute the vacuum polarization energy of static field configurations that do not allow a decomposition into symmetric and anti-symmetric channels. The method also applies to scenarios in which the masses of the quantum fluctuations at positive and negative spatial infinity are different. As an example we compute the vacuum polarization energy of the kink soliton in the ϕ6 model. We link the dependence of this energy on the position of the soliton to the different masses.http://www.sciencedirect.com/science/article/pii/S0370269316308012
collection DOAJ
language English
format Article
sources DOAJ
author H. Weigel
spellingShingle H. Weigel
Vacuum polarization energy for general backgrounds in one space dimension
Physics Letters B
author_facet H. Weigel
author_sort H. Weigel
title Vacuum polarization energy for general backgrounds in one space dimension
title_short Vacuum polarization energy for general backgrounds in one space dimension
title_full Vacuum polarization energy for general backgrounds in one space dimension
title_fullStr Vacuum polarization energy for general backgrounds in one space dimension
title_full_unstemmed Vacuum polarization energy for general backgrounds in one space dimension
title_sort vacuum polarization energy for general backgrounds in one space dimension
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2017-03-01
description For field theories in one time and one space dimensions we propose an efficient method to compute the vacuum polarization energy of static field configurations that do not allow a decomposition into symmetric and anti-symmetric channels. The method also applies to scenarios in which the masses of the quantum fluctuations at positive and negative spatial infinity are different. As an example we compute the vacuum polarization energy of the kink soliton in the ϕ6 model. We link the dependence of this energy on the position of the soliton to the different masses.
url http://www.sciencedirect.com/science/article/pii/S0370269316308012
work_keys_str_mv AT hweigel vacuumpolarizationenergyforgeneralbackgroundsinonespacedimension
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