$\rho -\omega$ Mixing at High Temperature and Density

Abstract

The temperature and density dependence of the $\rho -\omega$ mixing amplitude has been studied from a purely hadronic model. The in-medium baryon masses and chemical potentials have been obtained at the Mean Field (MF) Level and these results have been used to calculate the mixing amplitude. It has been observed that the mixing amplitude changes substantially at high temperature and density.

Mod. Phys. Lett. A13; page 2585

References in corpus (5)

• Constraints on the momentum dependence of rho-omega mixing
• Rho-omega Mixing and the Pion Electromagnetic Form-Factor
• Rho - omega mixing in chiral perturbation theory
• Matter induced rho-omega mixing
• Two Model-Independent Results for the Momentum Dependence of Rho-Omega Mixing

Cited by in corpus (2)

• Rho-omega mixing in asymmetric nuclear matter via QCD sum rule approach
• Meson mixing amplitudes in asymmetric nuclear matter