paper

The Cloud Contribution to the Width in Nuclear Matter

arXiv:1307.4001 · doi:10.1016/j.physletb.2013.12.056

Abstract

The width of the meson in cold nuclear matter is computed in a hadronic many-body approach, focusing on a detailed treatment of the medium modifications of intermediate states. The and propagators are dressed by their selfenergies in nuclear matter taken from previously constrained many-body calculations. The pion selfenergy includes and excitations with short-range correlations, while the selfenergy incorporates the same dressing of its cloud with a full 3-momentum dependence and vertex corrections, as well as direct resonance-hole excitations; both contributions were quantitatively fit to total photo-absorption spectra and scattering. Our calculations account for in-medium decays of type , and 2-body absorptions . This causes deviations of the in-medium width from a linear behavior in density, with important contributions from spacelike propagators. The width from the cloud may reach up to 200 MeV at normal nuclear matter density, with a moderate 3-momentum dependence. This largely resolves the discrepancy of linear - approximations with the values deduced from nuclear photoproduction measurements.

7 pages, 4 eps figures; v2: includes 3-mom dependence of width and additional discussion

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