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               <dc:title>BK-parameter from Nf = 2 twisted mass lattice QCD</dc:title>
               <dc:creator>Constantinou, M.</dc:creator>
               <dc:creator>Dimopoulos, P.</dc:creator>
               <dc:creator>Frezzotti, R.</dc:creator>
               <dc:creator>Jansen, K.</dc:creator>
               <dc:creator>Gimenez, V.</dc:creator>
               <dc:creator>Lubicz, V.</dc:creator>
               <dc:creator>Mescia, Federico</dc:creator>
               <dc:creator>Panagopoulos, H.</dc:creator>
               <dc:creator>Papinutto, M.</dc:creator>
               <dc:creator>Rossi, G. C.</dc:creator>
               <dc:creator>Simula, S.</dc:creator>
               <dc:creator>Skouroupathis, A.</dc:creator>
               <dc:creator>Stylianou, F.</dc:creator>
               <dc:creator>Vladikas, A.</dc:creator>
               <dc:creator>ETM Collaboration</dc:creator>
               <dc:subject>Física de partícules</dc:subject>
               <dc:subject>Experiments</dc:subject>
               <dc:subject>Particle physics</dc:subject>
               <dc:subject>Experiments</dc:subject>
               <dc:description>We present an unquenched N f = 2 lattice computation of the B K parameter which controls K 0 − ¯¯¯¯ K 0 oscillations. A partially quenched setup is employed with two maximally twisted dynamical (sea) light Wilson quarks, and valence quarks of both the maximally twisted and the Osterwalder-Seiler variety. Suitable combinations of these two kinds of valence quarks lead to a lattice definition of the B K parameter which is both multiplicatively renormalizable and O ( a ) improved. Employing the nonperturbative RI-MOM scheme, in the continuum limit and at the physical value of the pion mass we get B RGI K = 0.729 ± 0.030 , a number well in line with the existing quenched and unquenched determinations.</dc:description>
               <dc:date>2019-04-08T12:11:20Z</dc:date>
               <dc:date>2019-04-08T12:11:20Z</dc:date>
               <dc:date>2011-01-01</dc:date>
               <dc:date>2019-04-08T12:11:20Z</dc:date>
               <dc:type>info:eu-repo/semantics/article</dc:type>
               <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
               <dc:relation>Reproducció del document publicat a: https://doi.org/10.1103/PhysRevD.83.014505</dc:relation>
               <dc:relation>Physical Review D, 2011, vol. 83, num. 1, p. 014505</dc:relation>
               <dc:relation>https://doi.org/10.1103/PhysRevD.83.014505</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/EC/FP7/249309/EU//HPLQCD</dc:relation>
               <dc:rights>(c) American Physical Society, 2011</dc:rights>
               <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
               <dc:publisher>American Physical Society</dc:publisher>
               <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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