Journalartikel

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


AutorenlisteDiebel, M; Glas, D; Mosel, U; Chandra, H

Jahr der Veröffentlichung1980

Seiten253-272

ZeitschriftNuclear Physics A: Nuclear and Hadronic Physics

Bandnummer333

Heftnummer2

ISSN0375-9474

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

VerlagElsevier


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.




Zitierstile

Harvard-ZitierstilDiebel, 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-ZitierstilDiebel, 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


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