Generalised Kerr-Schild space-times: A. H. Taub. Mathematics Department, University of California, Berkeley, California, 94720

• Publisher: Elsevier Science
• Year: 1981
• Tongue: English
• Weight: 143 KB
• Volume: 133
• Category: Article
• ISSN: 0003-4916
• DOI: 10.1016/0003-4916(81)90260-8

✦ Synopsis

The shapes of nuclear configurations are calculated using Slater determinants built with cranked harmonic oscillator single particle states. The nuclear forces role is played by a volume conservation condition (of the potential or of the density) in a first part. In a second part, we have used the finite range, density dependent interaction of Gogny. A very simple classification of configurations emerges in the first part, the relevant parameter being the equatorial eccentricity of the nuclear density. A critical equatorial eccentricity is obtained which governs the accession to the case for which the nucleus is oblate and symmetric around its axis of rotation. Nuclear configurations calculated in the second part observe remarkably well these behaviours.

Three-Particle

Scattering at High Energies in a Mode! with Eikonal Hamiltonian.