dorsal/arxiv
View SchemaTreatment of baryonic resonances in the RQMD approach including scalar-vector mean fields
| Authors | C. Fuchs, L. Sehn, Amand Faessler, D. S. Kosov, V. S. Uma Maheswari, Z. Wang |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9702028 |
| URL | https://arxiv.org/abs/nucl-th/9702028 |
Abstract
In the relativistic Quantum Molecular Dynamics (RQMD) approach baryons are described within the framework of covariant hamilton constraint dynamics. The inclusion of a relativistic mean field results in a quasiparticle picture for the baryons. This requires to distinguish between canonical and kinetic variables of the particles. As resonances we include the $\Delta$(1232) and the $N^*$(1440) resonance. The resonance masses are distributed according Breit-Wigner functions. However, the scalar self energy leads to a shift in the masses and introduces an additional medium dependence. Consequences of this description on resonance and pion dynamics are discussed.
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"abstract": "In the relativistic Quantum Molecular Dynamics (RQMD) approach baryons are\ndescribed within the framework of covariant hamilton constraint dynamics. The\ninclusion of a relativistic mean field results in a quasiparticle picture for\nthe baryons. This requires to distinguish between canonical and kinetic\nvariables of the particles. As resonances we include the $\\Delta$(1232) and the\n$N^*$(1440) resonance. The resonance masses are distributed according\nBreit-Wigner functions. However, the scalar self energy leads to a shift in the\nmasses and introduces an additional medium dependence. Consequences of this\ndescription on resonance and pion dynamics are discussed.",
"arxiv_id": "nucl-th/9702028",
"authors": [
"C. Fuchs",
"L. Sehn",
"Amand Faessler",
"D. S. Kosov",
"V. S. Uma Maheswari",
"Z. Wang"
],
"categories": [
"nucl-th"
],
"title": "Treatment of baryonic resonances in the RQMD approach including scalar-vector mean fields",
"url": "https://arxiv.org/abs/nucl-th/9702028"
},
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