期刊文献+

Ratio of a strange quark mass m_s to up or down quark mass m_(u,d) predicted by a quark propagator in the framework of the chiral perturbation theory

Ratio of a strange quark mass m_s to up or down quark mass m_(u,d) predicted by a quark propagator in the framework of the chiral perturbation theory
原文传递
导出
摘要 Based on the fully dressed quark propagator and chiral perturbation theory, we study the ratio of the strange quark mass ms to up or down quark mass mu,d . The ratio is related to the determination of quark masses which are fundamental input parameters of QCD Lagrangian in the Standard Model of particle physics and can not be directly measured since the quark is confined within a hadron. An accurate determination of these QCD free parameters is extremely important for both phenomenological and theoretical applications. We begin with a brief introduction to the non-perturbation QCD theory, and then study the mass ratio in the framework of the chiral perturbation theory (χPT) with a parameterized fully dressed quark propagator which describes confining fully dressed quark propagation and is analytic everywhere in the finite complex p2-plane and has no Lehmann representation so there are no quark production thresholds in any theoretical calculations of observable data. Our prediction for the ratio ms/mu,d is consistent with other model predictions such as Lattice QCD, instanton model, QCD sum rules and the empirical values used widely in the literature. As a by-product of this study, our theoretical results, together with other predictions of physical quantities that used this quark propagator in our previous publications, clearly show that the parameterized form of the fully dressed quark propagator is an applicable and reliable approximation to the solution of the Dyson-Schwinger Equation of quark propagator in the QCD. Based on the fully dressed quark propagator and chiral perturbation theory, we study the ratio of the strange quark mass ms to up or down quark mass mu,d . The ratio is related to the determination of quark masses which are fundamental input parameters of QCD Lagrangian in the Standard Model of particle physics and can not be directly measured since the quark is confined within a hadron. An accurate determination of these QCD free parameters is extremely important for both phenomenological and theoretical applications. We begin with a brief introduction to the non-perturbation QCD theory, and then study the mass ratio in the framework of the chiral perturbation theory (χPT) with a parameterized fully dressed quark propagator which describes confining fully dressed quark propagation and is analytic everywhere in the finite complex p2-plane and has no Lehmann representation so there are no quark production thresholds in any theoretical calculations of observable data. Our prediction for the ratio ms/mu,d is consistent with other model predictions such as Lattice QCD, instanton model, QCD sum rules and the empirical values used widely in the literature. As a by-product of this study, our theoretical results, together with other predictions of physical quantities that used this quark propagator in our previous publications, clearly show that the parameterized form of the fully dressed quark propagator is an applicable and reliable approximation to the solution of the Dyson-Schwinger Equation of quark propagator in the QCD.
出处 《Chinese Physics C》 SCIE CAS CSCD 2013年第4期1-6,共6页 中国物理C(英文版)
基金 Supported by National Natural Science Foundation of China (10647002) Guangxi Natural Science Foundation for Young Researchers(0991009) Guangxi Natural Science Foundation (2011GXNSFA018140) Department of Guangxi Education (200807MS112)
关键词 light quark mass ratio chiral perturbation theory dressed quark propagator non-perturbative QCD light quark mass ratio; chiral perturbation theory; dressed quark propagator; non-perturbative QCD
  • 相关文献

参考文献21

  • 1't Hooft G. Phys. Rev. Lett.,1976,37: 8; Witten E. Nucl. Phys. B,1979,156: 269; Veneziano G. Nucl. Phys. B,1979,159: 213.
  • 2Herwijnen E V,Williams P G. Phys. Rev. D,1981,24: 240.
  • 3Herwijnen E V,Williams P G. Nucl. Phys. B,1982,196: 109.
  • 4Gasser J,Leutwyler H. Phys. Rept. C,1982,87: 77.
  • 5Gell-Mann M,Oakes R J,Renner B. Phys. Rev.,1968,175: 2195.
  • 6Gunion J F,McNamee P C,Scadron M D. Nucl. Phys. B,1977,123: 445; Caser S,Testa M. Phys. Lett. B,1976,61: 267.
  • 7Roberts C D,Williams A G. Prog. Part. Nucl. Phys.,2004,33: 477; ZHOU Li-Juan,WU Qing,PAN Ji-Huan et al. Commun. Theor. Phys.,2006,46: 101.
  • 8Gasser J,Leutwyler H. Nucl. Phys. B,1985,250: 465; Gasser J,Leutwyler H. Phys. Lett. B,1983,125: 321; Ann. of Phys.,1984,158: 142.
  • 9Colangelo G,Gasser J,Rusetsky A. Eur. Phys. J. C,2009,59: 777 (arXiv:0811.0775 [hep-ph]); Bissegger M,Fuhrer A,Gasser J et al. Nucl. Phys. B,2009,806: 178 (arXiv:0807.0515 [hep-ph]).
  • 10Weinberg S. Trans. New York Acad. Sci.,1977,38: 185.

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部