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dc.contributor.authorPirner, HJ
dc.contributor.authorSchwenzer, Kaı Olıver
dc.contributor.authorDeandrea, A
dc.contributor.authorMeyer, J
dc.date.accessioned2021-03-04T17:55:32Z
dc.date.available2021-03-04T17:55:32Z
dc.identifier.citationMeyer J., Schwenzer K. O. , Pirner H., Deandrea A., "Renormalization group flow in large N-c", PHYSICS LETTERS B, cilt.526, ss.79-89, 2002
dc.identifier.issn0370-2693
dc.identifier.othervv_1032021
dc.identifier.otherav_880302e1-8dcd-4832-826e-4e1bbe80081a
dc.identifier.urihttp://hdl.handle.net/20.500.12627/92325
dc.identifier.urihttps://doi.org/10.1016/s0370-2693(01)01482-4
dc.description.abstractWe calculate renormalization group flow equations for the linear sigma-model in large N-c approximation. The flow equations decouple and can be solved analytically. The solution is equal to a self consistent solution of the NJL model in the same approximation, which shows that flow equations are a promising method to extend the calculation to higher order in 1/N-c. Including explicit chiral symmetry breaking, the large N-c approximation describes physics reasonably well. We further compare the analytic solution to the usually used polynomial truncation and find consistency. (C) 2002 Elsevier Science B.V. All rights reserved.
dc.language.isoeng
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectTemel Bilimler
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectFİZİK, NÜKLEER
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleRenormalization group flow in large N-c
dc.typeMakale
dc.relation.journalPHYSICS LETTERS B
dc.contributor.department, ,
dc.identifier.volume526
dc.identifier.startpage79
dc.identifier.endpage89
dc.contributor.firstauthorID728616


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