Journal article

Yrast lines of light nuclei (A = 24–60)


Authors listDiebel, M; Glas, D; Mosel, U; Chandra, H

Publication year1980

Pages253-272

JournalNuclear Physics A: Nuclear and Hadronic Physics

Volume number333

Issue number2

ISSN0375-9474

DOI Linkhttps://doi.org/10.1016/0375-9474(80)90232-8

PublisherElsevier


Abstract

The Strutinsky method for rotating nuclei has been used to calculate yrast lines in the mass range from A = 24–60. As a basis for the diagonalization of the cranked Hamiltonian the exact eigenstates of the cranked, anisotropic harmonic oscillator are used. Problems of the Strutinsky method specific to this particular mass region are discussed. The calculated yrast lines have been searched for spin isomers, i.e. cold, oblate configurations. The yrast lines of sd shell nuclei are discussed in connection with empirical fusion bands.




Citation Styles

Harvard Citation styleDiebel, M., Glas, D., Mosel, U. and Chandra, H. (1980) Yrast lines of light nuclei (A = 24–60), Nuclear Physics A: Nuclear and Hadronic Physics, 333(2), pp. 253-272. https://doi.org/10.1016/0375-9474(80)90232-8

APA Citation styleDiebel, M., Glas, D., Mosel, U., & Chandra, H. (1980). Yrast lines of light nuclei (A = 24–60). Nuclear Physics A: Nuclear and Hadronic Physics. 333(2), 253-272. https://doi.org/10.1016/0375-9474(80)90232-8


Last updated on 2025-22-07 at 15:38