Leading isospin breaking effects on the lattice

G. M. de Divitiis, R. Frezzotti, V. Lubicz, G. Martinelli, R. Petronzio, G. C. Rossi, F. Sanfilippo, S. Simula, and N. Tantalo (RM123 Collaboration)
Phys. Rev. D 87, 114505 – Published 7 June 2013

Abstract

We present a method to evaluate on the lattice the leading isospin breaking effects due to both the small mass difference between the up and down quarks and the QED interaction. Our proposal is applicable in principle to any QCD+QED gauge invariant hadronic observable that can be computed on the lattice. It is based on the expansion of the path integral in powers of the small parameters (m^dm^u)/ΛQCD and α^em, where m^f is the renormalized quark mass and α^em the renormalized fine structure constant. In this paper we discuss in detail the general strategy of the method and the conventional, although arbitrary, separation of QCD from QED isospin breaking corrections. We obtain results for the pion mass splitting, Mπ+2Mπ02=1.44(13)(16)×103MeV2, for the Dashen’s theorem breaking parameter εγ=0.79(18)(18), for the light quark masses, [m^dm^u](MS¯,2GeV)=2.39(8)(17)MeV, [m^u/m^d](MS¯,2GeV)=0.50(2)(3), and for the flavor symmetry breaking parameters R and Q. We also update our previous results for the QCD isospin breaking corrections to the K2 decay rate and for the QCD contribution to the neutron-proton mass splitting. The numerical results of this paper have been obtained by using the gluon field configurations produced by the ETMC Collaboration with nf=2 dynamical quarks. We treated the dynamical quarks as electrically neutral particles (electroquenched approximation) and neglected a disconnected diagram in the charged and neutral pion mass splitting. We provide all the formulas necessary to remove these approximations and discuss in detail the estimate of the associated systematic uncertainties.

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  • Received 3 April 2013

DOI:https://doi.org/10.1103/PhysRevD.87.114505

© 2013 American Physical Society

Authors & Affiliations

G. M. de Divitiis1,2, R. Frezzotti1,2, V. Lubicz3,4, G. Martinelli5,6, R. Petronzio1,2, G. C. Rossi1,2, F. Sanfilippo7, S. Simula4, and N. Tantalo1,2 (RM123 Collaboration)

  • 1Dipartimento di Fisica, Università di Roma “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133 Rome, Italy
  • 2INFN, Sezione di Roma “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133 Rome, Italy
  • 3Dipartimento di Matematica e Fisica, Università Roma Tre, Via della Vasca Navale 84, I-00146 Rome, Italy
  • 4INFN, Sezione di Roma Tre, Via della Vasca Navale 84, I-00146 Rome, Italy
  • 5SISSA, Via Bonomea 265, 34136 Trieste, Italy
  • 6INFN, Sezione di Roma, Piazzale Aldo Moro 5, I-00185 Rome, Italy
  • 7Laboratoire de Physique Théorique (Bâtiment 210), Université Paris Sud, F-91405 Orasay-Cedex, France

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Issue

Vol. 87, Iss. 11 — 1 June 2013

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