2018
DOI: 10.1140/epjc/s10052-018-6343-6
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Schwinger–Dyson equation boundary conditions induced by ETC radiative corrections

Abstract: The technicolor (TC) Schwinger-Dyson equations (SDE) should include radiative corrections induced by extended technicolor (ETC) interactions when TC is embedded into a larger theory including also QCD. These radiative corrections couple the different strongly interacting Dyson equations. We discuss how the boundary conditions of the coupled SDE system are modified by these corrections, and verify that the ultraviolet behavior of the self-energies are described by a function that decreases logarithmically with … Show more

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Cited by 11 publications
(39 citation statements)
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“…However, the solutions discussed in Refs. [35,36] and in this work are related to the asymptotic behavior produced by the effective mass of the coupled SDE, and are not affected by the infrared intricacies of the strongly interacting theories.…”
Section: Introductionmentioning
confidence: 66%
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“…However, the solutions discussed in Refs. [35,36] and in this work are related to the asymptotic behavior produced by the effective mass of the coupled SDE, and are not affected by the infrared intricacies of the strongly interacting theories.…”
Section: Introductionmentioning
confidence: 66%
“…In Ref. [36] we analytically verified that the radiative corrections shown in Fig.2 act as an effective bare mass. In the case of ordinary quarks the second diagram (b 2 ) on the right-hand of Fig.2 originates an effective mass due to TC condensation; on the other hand, the techniquarks obtain a tiny effective mass due to QCD condensation [see diagram (a 2 ) in Fig.2], and an even larger mass due to the other diagrams [(a 3 ) and (a 4 )].…”
Section: Introductionmentioning
confidence: 68%
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