English

rho-omega mixing in relativistic heavy-ion collisions

Nuclear Theory 2009-10-31 v1 High Energy Physics - Phenomenology

Abstract

We show that even moderate excess of neutrons over protons in nuclear matter, such as in 208Pb{}^{208} Pb, can lead to large ρ\rho-ω\omega mixing at densities of the order of twice the nuclear saturation density and higher. The typical mixing angle is of the order of 10o10^o. The mixing may result in noticeable shifts of the positions and widths of resonances. We also analyze temperature effects and find that temperatures up to 50 MeV have practically no effect on the mixing.

Keywords

Cite

@article{arxiv.nucl-th/9804038,
  title  = {rho-omega mixing in relativistic heavy-ion collisions},
  author = {Wojciech Broniowski and Wojciech Florkowski},
  journal= {arXiv preprint arXiv:nucl-th/9804038},
  year   = {2009}
}

Comments

8 pages