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
References in corpus (10)
- phi photo-production from Li, C, Al, and Cu nuclei at Egamma=1.5 - 2.4 GeV
- Modification of the -Meson Lifetime in Nuclear Matter
- Absorption of the and Mesons in Nuclei
- Inclusive photoproduction from nuclei and in the nuclear medium
- Thermal Dileptons from Hot and Dense Strongly Interacting Matter
- The spectral function of the omega meson in nuclear matter from a coupled-channel resonance model
- The STAR Dilepton Physics Program
- The omega rho pi coupling in the VMD model revisited
- Hadrons in Medium -- Theory confronts experiment
- Analysis of self-energy at finite temperature and density in the real-time formalism
Cited by in corpus (5)
- Meson-nucleus potentials and the search for meson-nucleus bound states
- Remarks on nuclear matter: how an condensate can spike the speed of sound, and a model of baryons
- Momentum dependence of the imaginary part of the - and -nucleus optical potential
- Interactions of -Mesons in Nuclear Matter and with Nuclei
- Velocity dependence of the mass modifications of and mesons in 12 GeV reactions