scholarly journals Non-perturbative renormalization of quark mass in N f = 2 + 1 QCD with the Schrödinger functional scheme

2010 ◽  
Vol 2010 (8) ◽  
Author(s):  
S. Aoki ◽  
◽  
K.-I. Ishikawa ◽  
N. Ishizuka ◽  
T. Izubuchi ◽  
...  
2002 ◽  
Vol 106-107 ◽  
pp. 844-846
Author(s):  
S. Aoki ◽  
Y. Aoki ◽  
S. Ejiri ◽  
M. Fukugita ◽  
S. Hashimoto ◽  
...  

Author(s):  
Giulia Maria de Divitiis ◽  
Patrick Fritzsch ◽  
Jochen Heitger ◽  
Carl Christian Köster ◽  
Simon Kuberski ◽  
...  

Abstract We determine non-perturbatively the normalisation parameter $$Z_\mathrm{m}Z_\mathrm{P}/Z_\mathrm{A}$$ZmZP/ZA as well as the Symanzik coefficients $$b_\mathrm{m}$$bm and $$b_\mathrm{A}-b_\mathrm{P}$$bA-bP, required in $$\mathrm{O}(a)$$O(a) improved quark mass renormalisation with Wilson fermions. The strategy underlying their computation involves simulations in $$N_\mathrm{f}=3$$Nf=3 QCD with $$\mathrm{O}(a)$$O(a) improved massless sea and non-degenerate valence quarks in the finite-volume Schrödinger functional scheme. Our results, which cover the typical gauge coupling range of large-volume $$N_\mathrm{f}=2+1$$Nf=2+1 QCD simulations with Wilson fermions at lattice spacings below $$0.1\,\mathrm{fm}$$0.1fm, are of particular use for the non-perturbative calculation of $$\mathrm{O}(a)$$O(a) improved renormalised quark masses.


2011 ◽  
Author(s):  
Francesco Di Renzo ◽  
Michele Brambilla ◽  
Luigi Scorzato

1997 ◽  
Vol 92 (3) ◽  
pp. 477-487 ◽  
Author(s):  
GERALD LIPPERT ◽  
JuRG HUTTER ◽  
MICHELE PARRINELLO

Author(s):  
Steven E. Vigdor

Chapter 4 deals with the stability of the proton, hence of hydrogen, and how to reconcile that stability with the baryon number nonconservation (or baryon conservation) needed to establish a matter–antimatter imbalance in the infant universe. Sakharov’s three conditions for establishing a matter–antimatter imbalance are presented. Grand unified theories and experimental searches for proton decay are described. The concept of spontaneous symmetry breaking is introduced in describing the electroweak phase transition in the infant universe. That transition is treated as the potential site for introducing the imbalance between quarks and antiquarks, via either baryogenesis or leptogenesis models. The up–down quark mass difference is presented as essential for providing the stability of hydrogen and of the deuteron, which serves as a crucial stepping stone in stellar hydrogen-burning reactions that generate the energy and elements needed for life. Constraints on quark masses from lattice QCD calculations and violations of chiral symmetry are discussed.


Sign in / Sign up

Export Citation Format

Share Document