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Highly deformed Bands in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">Hf</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>175</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:mrow></mml:math>

D. T. ScholesSchuster Laboratory, University of Manchester, Manchester M13 9PL, United KingdomD. M. CullenSchuster Laboratory, University of Manchester, Manchester M13 9PL, United KingdomF. G. KondevNuclear Engineering, Argonne National Laboratory, Argonne, Illinois 60439, USAR. V. F. JanssensPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAM. P. CarpenterPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAD. J. HartleyDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAM. DjongolovDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAG. SlettenG.B. HagemannC. WheldonDepartment of Physics, University of Surrey, Guildford GU2 7XH, United KingdomP. M. WalkerDepartment of Physics, University of Surrey, Guildford GU2 7XH, United KingdomK. Abu SaleemPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAI. AhmadPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAD. L. BalabanskiDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAP. ChowdhuryDepartment of Physics, University of Massachusetts, Lowell, Massachusetts 01854, USAM. DanchevDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAG.D. DracoulisDepartment of Nuclear Physics, Australian National University, Canberra, Australian Capital Territory 0200, AustraliaH. M. El-MasriDepartment of Physics, University of Surrey, Guildford GU2 7XH, United KingdomJ. TM. GoonDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAA. HeinzPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAR. A. KayeDepartment of Chemistry and Physics, Purdue University, Calumet, Hammond, Indiana 46323, USAT. L. KhooPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAT. LauritsenPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAC. J. ListerPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAE. F. MoorePhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAL. L. RiedingerDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAM. A. RileyDepartment of Physics, Florida State University, Tallahassee, Florida 32306, USAD. SeweryniakPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAI. ShestakovaDepartment of Physics, University of Massachusetts, Lowell, Massachusetts 01854, USAI. WiedenhöverPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAO. ZeidanDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAJing-ye ZhangDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
2004lv
ABI

Аннотация

Two high-spin regularly spaced rotational bands with large dynamical moments of inertia have been identified in $^{175}\mathrm{Hf}$ with the Gammasphere spectrometer. These new bands are very similar to the previously identified triaxial superdeformed bands in the hafnium nuclei. However, the new bands in $^{175}\mathrm{Hf}$ have been linked into the known level scheme and thereby provide the first firm spin assignments for these structures in this region. In order to understand the new bands, theoretical calculations have been performed based on the ULTIMATE CRANKER code. The new bands in $^{175}\mathrm{Hf}$ are deduced to be built upon highly deformed structures. No experimental evidence for triaxiality was established and this work suggests that the structure of the so-called ``triaxial'' superdeformed bands in the $\mathrm{Hf}$ nuclei may be quite different from those identified in the lighter mass $\mathrm{Lu}$ nuclei. Since the two highly deformed bands in $^{175}\mathrm{Hf}$ are associated with different deformations, this work also identifies the role of the intruder orbits in polarizing the nuclear shape.

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