dc.contributor.author | Pirner, HJ | |
dc.contributor.author | Schwenzer, Kaı Olıver | |
dc.contributor.author | Deandrea, A | |
dc.contributor.author | Meyer, J | |
dc.date.accessioned | 2021-03-04T17:55:32Z | |
dc.date.available | 2021-03-04T17:55:32Z | |
dc.identifier.citation | Meyer 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.issn | 0370-2693 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.other | av_880302e1-8dcd-4832-826e-4e1bbe80081a | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/92325 | |
dc.identifier.uri | https://doi.org/10.1016/s0370-2693(01)01482-4 | |
dc.description.abstract | We 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.iso | eng | |
dc.subject | Temel Parçacıklar ve Alanlar | |
dc.subject | Temel Bilimler | |
dc.subject | FİZİK, PARTİKLER VE ALANLAR | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Fizik | |
dc.subject | FİZİK, NÜKLEER | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Uzay bilimi | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.title | Renormalization group flow in large N-c | |
dc.type | Makale | |
dc.relation.journal | PHYSICS LETTERS B | |
dc.contributor.department | , , | |
dc.identifier.volume | 526 | |
dc.identifier.startpage | 79 | |
dc.identifier.endpage | 89 | |
dc.contributor.firstauthorID | 728616 | |