Relativistic mean-field description of the dynamics of giant resonances

Abstract

The relativistic mean-field theory provides a framework in which the nuclear many-body problem is described as a self-consistent system of nucleons and mesons. In the mean-field approximation, the self-consistent time evolution of the nuclear system describes the dynamics of collective motion: nuclear compressibility from monopole resonances, regular and chaotic dynamics of isoscalar and isovector collective vibrations.

arXiv commentLaTeX, 10 pages, 5 figures, Invited Talk, Topical Conference on Giant resonances, Varenna, May 1998, to be published in Nucl. Phys. A

References in corpus (4)

• A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory
• Recent Progress in Quantum Hadrodynamics
• Monopole giant resonances and nuclear compressibility in relativistic mean field theory
• Regular and chaotic dynamics in time-dependent relativistic mean-field theory

Cited by in corpus (12)

• Neutron-Rich Nuclei in Heaven and Earth
• A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models
• Isoscalar dipole mode in relativistic random phase approximation
• The time-dependent relativistic mean-field theory and the random phase approximation
• Collective multipole excitations in a microscopic relativistic approach
• Continuum Random Phase Approximation for Relativistic Point Coupling Models
• The Gamow-Teller Resonance in Finite Nuclei in the Relativistic Random Phase Approximation
• Neutral-current neutrino-nucleus cross sections based on relativistic nuclear energy density functional
• Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei
• Damping of the isovector giant dipole resonance in ${}^{40,48}$Ca
• Effects of the Dirac Sea on the Giant Monopole States
• Isovector Giant Dipole Resonance of Stable Nuclei in a Consistent Relativistic Random Phase Approximation