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The quark Schwinger-Dyson equation in temporal Euclidean space

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    SYSNO ASEP0338994
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThe quark Schwinger-Dyson equation in temporal Euclidean space
    Author(s) Šauli, Vladimír (UJF-V) RID, SAI, ORCID
    Batiz, Z. (PT)
    Source TitleJournal of Physics G-Nuclear and Particle Physics. - : Institute of Physics Publishing - ISSN 0954-3899
    Roč. 36, č. 3 (2009), 035002/1-035002/13
    Number of pages13 s.
    Languageeng - English
    CountryGB - United Kingdom
    KeywordsANALYTIC PERTURBATION-THEORY ; DYNAMICAL SYMMETRY-BREAKING ; BACKGROUND FIELD METHOD
    Subject RIVBE - Theoretical Physics
    CEZAV0Z10480505 - UJF-V (2005-2011)
    UT WOS000263259300003
    DOI10.1088/0954-3899/36/3/035002
    AnnotationWe present an elementary non-perturbative method for obtaining Green's functions (GFs) for timelike momenta. We assume that there are no singularities in the second and fourth quadrants of the complex plane of space momentum components and perform a 3D analog of Wick rotation. This procedure defines Green's functions in a timelike Euclidean space. As an example we consider the quark propagator in QCD. While for weak coupling this method is obviously equivalent to perturbation theory, for a realistic QCD coupling a complex part of the quark mass and renormalization wavefunction has been spontaneously generated even below the standard perturbative threshold. Therefore, our method favors a confinement mechanism based on the lack of real poles.
    WorkplaceNuclear Physics Institute
    ContactMarkéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228
    Year of Publishing2010
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