Charmed Baryon in Nuclear Matter
arXiv:1704.04902 · doi:10.1103/PhysRevC.96.055208
Abstract
Density dependences of the mass and self-energies of in nulear matter are studied in the parity projected QCD sum rule. Effects of nuclear matter are taken into account through the quark and gluon condensates. It is found that the four-quark condensates give dominant contributions. As the density dependences of the four-quark condensates are not known well, we examine two hypotheses. One is based on the factorization hypothesis (F-type) and the other is derived from the perturbative chiral quark model (QM-type). The F-type strongly depends on density, while the QM-type gives a weaker dependence. It is found that, for the F-type dependence, the energy of increases as the density of nuclear matter grows, that is, feels repulsion. On the other hand, the QM-type predicts a weak attraction ( MeV at the normal nuclear density) for in nuclear matter. We carry out a similar analysis of the hyperon and find that the F-type density dependence is too strong to explain the observed binding energy of in nuclei. Thus we conclude that the weak density dependence of the four-quark condensate is more realistic. The scalar and vector self-energies of for the QM-type dependence are found to be much smaller than those of the light baryons.
14 pages, 6 figures, 2 tables, published version
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- Properties of , and heavy baryons in cold nuclear matter
- Predictions for charmed nuclei based on forces inferred from lattice QCD simulations
- Charmed baryons in nuclear matter
- Charmed hypernuclei within density-dependent relativistic mean-field theory
- Singly heavy baryons in nuclear matter from an SU(3) chiral soliton model