dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2014-05-27T11:18:15Z | |
dc.date.available | 2014-05-27T11:18:15Z | |
dc.date.created | 2014-05-27T11:18:15Z | |
dc.date.issued | 1997-07-31 | |
dc.identifier | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 406, n. 1-2, p. 130-136, 1997. | |
dc.identifier | 0370-2693 | |
dc.identifier | http://hdl.handle.net/11449/65153 | |
dc.identifier | 10.1016/S0370-2693(97)00673-4 | |
dc.identifier | WOS:A1997XP70100022 | |
dc.identifier | 2-s2.0-0041155142 | |
dc.description.abstract | Nonperturbative infrared finite solutions for the gluon polarization tensor have been found, and the possibility that gluons may have a dynamically generated mass is supported by recent Monte Carlo simulation on the lattice. These solutions differ among themselves, due to different approximations performed when solving the Schwinger-Dyson equations for the gluon polarization tensor. Only approximations that minimize energy are meaningful, and, according to this, we compute an effective potential for composite operators as a function of these solutions in order to distinguish which one is selected by the vacuum. © 1997 Elsevier Science B.V. | |
dc.language | eng | |
dc.relation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | |
dc.relation | 4.254 | |
dc.relation | 2,336 | |
dc.rights | Acesso restrito | |
dc.source | Scopus | |
dc.title | Infrared finite solutions for the gluon propagator and the QCD vacuum energy | |
dc.type | Artículos de revistas | |