Approaching the N=116 shell gap: Superdeformation in 195Hg*

Details Approaching the N=116 shell gap: Superdeformation in 195Hg* Approaching the N=116 shell gap: Superdeformation in 195Hg*

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aps..may.b1009h&link_type=abstract

American Physical Society, APS/AAPT Joint Meeting, May 2-5, 1996, abstract #B10.09

Physics

Scientific paper

Three superdeformed (SD) bands have been observed with Gammasphere in the nucleus 195Hg, populated following the 48Ca(150Nd,3n) reaction at 201 MeV. Two of these bands are signature partners, and their dynamic moments of inertia cal J^ rise with frequency in a fashion typical of mercury yrast SD bands. The cal J(2) of the third band is constant at low frequency, indicating that it is based on a ν j15/2 quasiparticle configuration. The γ--ray energies are not identical to any SD bands in the mercury region. It may be that the structure of these new bands is best understood in terms of a yet--unobserved 196Hg core. *Work supported by U.S. D.O.E. Nucl. Phys. Div. under contracts W-31-109-ENG-38 and DE-AC03-76SF0008, and partially by NSERC, Canada.

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