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dc.contributor.author | Becirevic, D. | |
dc.contributor.author | Blossier, B. | |
dc.contributor.author | Boucaud, Ph. | |
dc.contributor.author | Giménez Gómez, Vicente | |
dc.contributor.author | Lubicz, V. | |
dc.contributor.author | Mescia, Federico | |
dc.contributor.author | Simula, S. | |
dc.contributor.author | Tarantino, C. | |
dc.date.accessioned | 2014-09-25T11:16:15Z | |
dc.date.available | 2014-09-25T11:16:15Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Becirevic, D. Blossier, B. Boucaud, Ph. Giménez Gómez, Vicente Lubicz, V. Mescia, Federico Simula, S. Tarantino, C. 2006 Non-perturbatively renormalised light quark masses from a lattice simulation with N(f) = 2 Nuclear Physics B 734 1-2 138 155 | |
dc.identifier.uri | http://hdl.handle.net/10550/38968 | |
dc.description.abstract | We present results for the light quark masses obtained from a lattice QCD simulation with N-f = 2 degenerate Wilson dynamical quark flavours. The sea quark masses of our lattice, of spacing a similar or equal to 0.06 fm, are relatively heavy, i.e., they cover the range corresponding to 0.60 less than or similar to M-p/M-V less than or similar to 0.75. After implementing the non-perturbative RI-MOM method to renormalise quark masses, we obtain m(ud)((MS) over bar)(2 GeV)= 4.3 +/- 0.4(-0)(+1.1) MeV, and m(s)((MS) over bar)(2 GeV) = 101 +/- 8(-0)(+25) MeV, which are about 15% larger than they would be if renormalised perturbatively. In addition, we show that the above results are compatible with those obtained in a quenched simulation with a similar lattice. | |
dc.language.iso | eng | |
dc.relation.ispartof | Nuclear Physics B, 2006, vol. 734, num. 1-2, p. 138-155 | |
dc.subject | Física | |
dc.title | Non-perturbatively renormalised light quark masses from a lattice simulation with N(f) = 2 | |
dc.type | journal article | es_ES |
dc.date.updated | 2014-09-25T11:16:15Z | |
dc.identifier.doi | 10.1016/j.nuclphysb.2005.11.014 | |
dc.identifier.idgrec | 041521 | |
dc.rights.accessRights | open access | es_ES |