Pi- Eta Mixing from QCD Sum Rules
arXiv:hep-ph/9403380 · doi:10.1016/0370-2693(94)01461-K
Abstract
The dependence of the - mixing amplitude is examined with the use of QCD sum rules. The linear slope of the mixing function is found to be much smaller than that for - mixing. Thus the mixing amplitude is approximately the same in the space-like region as in the time-like one, and one may neglect the dependence of the mixing. A comparison between a hadron-meson, an effective chiral model, and the QCD sum rules approaches is made.
14 pages (written in REVTEX) + 1 fig. (available as hardcopy only on request), preprint no.DOE/ER/40561-133-INT94-0053
References in corpus (7)
- The Momentum Dependence of the Mixing Amplitude in a Hadronic Model
- Constraints on the momentum dependence of rho-omega mixing
- The Off Shell - Mixing in the QCD Sum Rules
- Charge-Symmetry Breaking, Rho-Omega Mixing and the Quark Propagator
- Off-shell Behavior of the Mixing Amplitude
- -Dependence of Meson Mixing in Few-Body Charge Symmetry Breaking: Mixing to One Loop in Chiral Perturbation Theory
- Modelling the Off-Shell Dependence of Mixing with Quark Loops
Cited by in corpus (8)
- The Mixed-Isospin Vector Current Correlator in Chiral Perturbation Theory and QCD Sum Rules
- Two Model-Independent Results for the Momentum Dependence of Rho-Omega Mixing
- The Kaon Parameter in the Chiral Limit
- Isospin-Violating Meson-Nucleon Vertices as an Alternate Mechanism of Charge-Symmetry Breaking
- On eta-pi mixing close to the eta-Helium threshold
- In-medium Σ^0-ΛMixing in QCD Sum Rules
- Isospin-Breaking Vacuum-to-Pi^0,Eta Pseudoscalar Matrix Elements at Next-to-Leading Order in the Chiral Expansion
- QCD Sum Rules for the Isospin-Breaking Axial Correlator with Correct Chiral Behavior