QCD sum rules for isobar in nuclear matter
arXiv:hep-ph/9411265 · doi:10.1103/PhysRevC.51.2260
Abstract
The self-energies of isobar propagating in nuclear matter are calculated using the finite-density QCD sum-rule methods. The calculations show that the Lorentz vector self-energy for the is significantly smaller than the nucleon vector self-energy. The magnitude of the scalar self-energy is larger than the corresponding value for the nucleon, which suggests a strong attractive net self-energy for the ; however, the prediction for the scalar self-energy is very sensitive to the density dependence of certain in-medium four-quark condensate. Phenomenological implications for the couplings of the to the nuclear scalar and vector fields are briefly discussed.
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