Shape and superdeformed structure in Hg isotopes in relativistic mean field model

S. K. Patra, S. Yoshida, N. Takigawa, and C. R. Praharaj
Phys. Rev. C 50, 1924 – Published 1 October 1994
PDFExport Citation

Abstract

Various shapes of Hg isotopes are calculated using a relativistic mean field theory. We observe shape transitions from oblate to prolate and prolate to oblate at A=178 and A=188, respectively. Both in the oblate and in the prolate solutions the sign of the hexadecupole moment changes from positive to negative values with increasing mass number. The predicted shape of the ground state agrees with the available data contrary to nonrelativistic calculations for neutron deficient isotopes. A low-lying superdeformed configuration is found in some isotopes, and found to be the ground state for Hg180. A possible discrepancy between the experimental data of the quadrupole deformation and those of the charge radii is pointed out.

  • Received 23 March 1994

DOI:https://doi.org/10.1103/PhysRevC.50.1924

©1994 American Physical Society

Authors & Affiliations

S. K. Patra, S. Yoshida, and N. Takigawa

  • Department of Physics, Faculty of Science, Tohoku University, 980-77 Sendai, Japan

C. R. Praharaj

  • Institute of Physics, Bhubaneswar-751 005, India

References (Subscription Required)

Click to Expand
Issue

Vol. 50, Iss. 4 — October 1994

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×