Physical Origin of Density Dependent Force of the Skyrme Type within the Quark Meson Coupling Model [electronic resource]
A density dependent, effective nucleon-nucleon force of the Skyrme type is derived from the quark-meson coupling model--a self-consistent, relativistic quark level description of nuclear matter. This new formulation requires no assumption that the mean scalar field is small and hence constitutes a s...
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Online Access |
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| Format: | Government Document Electronic eBook |
| Language: | English |
| Published: |
Washington, D.C. : Oak Ridge, Tenn. :
United States. Department of Energy. Office of Energy Research ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2006.
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| Subjects: |
MARC
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| 245 | 0 | 0 | |a Physical Origin of Density Dependent Force of the Skyrme Type within the Quark Meson Coupling Model |h [electronic resource] |
| 260 | |a Washington, D.C. : |b United States. Department of Energy. Office of Energy Research ; |a Oak Ridge, Tenn. : |b distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, |c 2006. | ||
| 336 | |a text |b txt |2 rdacontent. | ||
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| 500 | |a Published through SciTech Connect. | ||
| 500 | |a 03/17/2006. | ||
| 500 | |a "jlab-thy-06-477" | ||
| 500 | |a " doe/er/40150-3821" | ||
| 500 | |a FT. | ||
| 500 | |a Hrayr Matevosyan; Anthony Thomas; Pierre Guichon; N. Sandulescu. | ||
| 520 | 3 | |a A density dependent, effective nucleon-nucleon force of the Skyrme type is derived from the quark-meson coupling model--a self-consistent, relativistic quark level description of nuclear matter. This new formulation requires no assumption that the mean scalar field is small and hence constitutes a significant advance over earlier work. The similarity of the effective interaction to the widely used SkM* force encourages us to apply it to a wide range of nuclear problems, beginning with the binding energies and charge distributions of doubly magic nuclei. Finding impressive results in this conventional arena, we apply the same effective interaction, within the Hartree-Fock-Bogoliubov approach, to the properties of nuclei far from stability. The resulting two neutron drip lines and shell quenching are quite satisfactory. Finally, we apply the relativistic formulation to the properties of dense nuclear matter in anticipation of future application to the properties of neutron stars. | |
| 536 | |b AC05-84ER40150. | ||
| 650 | 7 | |a Charge Distribution. |2 local. | |
| 650 | 7 | |a Magic Nuclei. |2 local. | |
| 650 | 7 | |a Mesons. |2 local. | |
| 650 | 7 | |a Neutron Stars. |2 local. | |
| 650 | 7 | |a Neutrons. |2 local. | |
| 650 | 7 | |a Nuclear Matter. |2 local. | |
| 650 | 7 | |a Nuclei. |2 local. | |
| 650 | 7 | |a Origin. |2 local. | |
| 650 | 7 | |a Quarks. |2 local. | |
| 650 | 7 | |a Quenching. |2 local. | |
| 650 | 7 | |a Scalar Fields. |2 local. | |
| 650 | 7 | |a Stability. |2 local. | |
| 650 | 7 | |a Physics Of Elementary Particles And Fields. |2 edbsc. | |
| 650 | 7 | |a Classical And Quantum Mechanics, General Physics. |2 edbsc. | |
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