TY - JOUR
T1 - Properties of light quarks from lattice QCD simulations1
AU - Aubina, C.
AU - Bernard, C.
AU - Detar, C.
AU - Gottlieb, Steven
AU - Gregory, B.
AU - Heller, Urs M.
AU - Hetrick, E.
AU - Levkova, L.
AU - Maresca, F.
AU - Osborn, J.
AU - Renner, D.
AU - Sugar, L.
AU - Toussaint, D.
PY - 2005/1/1
Y1 - 2005/1/1
N2 - By numerical study of the simple bound states of light quarks, in particular the π and K mesons, we are able to deduce fundamental quark properties. Using the "improved staggered" discretization of QCD, the MILC Collaboration has performed a series of simulations of these bound states, including the effects of virtual quark-antiquark pairs ("sea" quarks). From these simulations, we have determined the masses of the up, down, and strange quarks. We find that the up quark mass is not zero (at the 10 sigma level), putting to rest a twenty-year-old suggestion that the up quark could be massless. Further, by studying the decays of the π and K mesons, we are able to determine the "CKM matrix element" Vus of the Weak Interactions. The errors on our result for Vus are comparable to the best previous determinations using alternative theoretical approaches, and are likely to be significantly reduced by simulations now in progress.
AB - By numerical study of the simple bound states of light quarks, in particular the π and K mesons, we are able to deduce fundamental quark properties. Using the "improved staggered" discretization of QCD, the MILC Collaboration has performed a series of simulations of these bound states, including the effects of virtual quark-antiquark pairs ("sea" quarks). From these simulations, we have determined the masses of the up, down, and strange quarks. We find that the up quark mass is not zero (at the 10 sigma level), putting to rest a twenty-year-old suggestion that the up quark could be massless. Further, by studying the decays of the π and K mesons, we are able to determine the "CKM matrix element" Vus of the Weak Interactions. The errors on our result for Vus are comparable to the best previous determinations using alternative theoretical approaches, and are likely to be significantly reduced by simulations now in progress.
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U2 - 10.1088/1742-6596/16/1/020
DO - 10.1088/1742-6596/16/1/020
M3 - Article
AN - SCOPUS:24344471718
SN - 1742-6588
VL - 16
SP - 160
EP - 164
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
ER -