Time-dependent relativistic mean-field theory

1997/09/26 by D. Vretenar, Dario Vretenar, Vretenar, Dario
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #Nuclear Theory (nucl-th) #nucl-th

paper · pdf · doi:10.48550/arxiv.nucl-th/9709061

9 Pages, LaTex, 9 ps figures, Invited talk at the International Conference on Nuclear Physics and Related Areas, Thessaloniki 1997, to appear in the conference proceedings

arxiv created 1997/09/26 · openalex publication_date 1997/09/26 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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: double giant resonances, nuclear compressibility from monopole resonances, regular and chaotic dynamics of isoscalar and isovector collective vibrations.

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