https://doi.org/10.1140/epja/i2006-08-025-6
Nuclear Physics in Astrophysics II
Pygmy dipole strength close to particle-separation energies --The case of the Mo isotopes
1
Institut für Kern- und Hadronenphysik, Forschungszentrum Rossendorf, Postfach 510119, 01314, Dresden, Germany
2
Institut für Kern- und Teilchenphysik, Technische Universität Dresden, 01062, Dresden, Germany
* e-mail: e.grosse@fz-rossendorf.de
Received:
4
July
2005
Accepted:
20
December
2005
Published online:
13
March
2006
The distribution of electromagnetic dipole strength in 92, 98, 100Mo has been investigated by photon scattering using bremsstrahlung from the new ELBE facility. The experimental data for well-separated nuclear resonances indicate a transition from a regular to a chaotic behaviour above 4MeV of excitation energy. As the strength distributions follow a Porter-Thomas distribution much of the dipole strength is found in weak and in unresolved resonances appearing as fluctuating cross section. An analysis of this quasi-continuum --here applied to nuclear resonance fluorescence in a novel way-- delivers dipole strength functions, which are combining smoothly to those obtained from (γ, n) data. Enhancements at 6.5MeV and at ∼ 9MeV are linked to the pygmy dipole resonances postulated to occur in heavy nuclei.
PACS: 21.10.Pc Single-particle levels and strength functions – / 24.10.Lx Monte Carlo simulations (including hadron and parton cascades and string breaking models) – / 25.20.Dc Photon absorption and scattering – / 26.50.+x Nuclear physics aspects of novae, supernovae, and other explosive environments –
© Società Italiana di Fisica and Springer-Verlag, 2006