Search results for "Nuclear Structure"
showing 10 items of 401 documents
From nuclear halos to superheavy nuclei—Perspectives for nuclear structure research at GSI
1998
Of fundamental interest is the investigation of nuclear matter at the limits of its existence in the vicinity of the driplines and in the region of the superheavy elements. The availability of unstable nuclei over large energy ranges and new experimental developments gave new impulse to nuclear structure research. Examples are the investigations of halo nuclei by nuclear decay studies combined with reactions at low and high energies, the mapping of the mass surface in large-scale direct mass measurements, and the production of heavy and superheavy nuclei. New developments such as high-current accelerators or the next generation of radioactive beam facilities will lead to further progress in…
Nuclear structure theory for the astrophysical rp-process and r-process
2003
Abstract The astrophysical processes of rapid-proton capture and rapid-neutron capture require the knowledge of many nuclear properties which are not known from experiment. I will describe two examples of how theoretical models are used to provide this input. The first of these uses the Hartree-Fock method for displacement energies to obtain the masses of proton-rich nuclei needed for the rp-process. The second uses a model for configuration mixing near 132 Sn to provide Q values and beta-decay lifetimes for the r-process.
Facilities and Methods: Heavy Element Spectroscopy at JYFL
2007
A central theme throughout the history of experimental nuclear physics has been the pursuit of nuclei at the extremes. These extremes, be they in terms of mass, proton-to-neutron ratio, or spin and excitation energy, provide the most stringent tests for our current nuclear structure theories. The pursuit of these extremes also provides impetus to develop and exploit new techniques and instrumentation. At the Department of Physics of the University of Jyvaskyla (JYFL), a major part of the experimental program is devoted to the study of heavy nuclei along the proton dripline and superheavy nuclei in the transfermium region. This program was initiated in the mid-1990s when a small array of TES…
Nuclear structure of97Y in the interacting boson-fermion model
1988
Unique-parity states of97Y are studied in the framework of the interacting boson-fermion model (IBFM). Spin assignments for the levels of the unique-parity yrast band are proposed on the basis of nuclear systematics and the IBFM band pattern associated with coupling of a particle-type quasiparticle (g9/2) to the SU(5) core3896Sr58. The good fit of the experimental data with the IBFM calculations confirms the single particle character of this immediate neighbour of the doubly sub-magic nucleus96Zr.
Level scheme ofZr101and structure of theN=61 Sr, Zr, and Mo isotones
1995
The neutron-rich nucleus $_{40}^{101}\mathrm{Zr}_{61}$ has been studied at the isotope separator ISOLDE via the \ensuremath{\beta} decay of $^{101}\mathrm{Y}$. A detailed level scheme has been obtained from \ensuremath{\gamma}-ray singles, \ensuremath{\gamma}-\ensuremath{\gamma}-t and \ensuremath{\beta}-\ensuremath{\gamma}-t coincidence measurements. The level structure of $^{101}\mathrm{Zr}$ is similar to that of its isotone $^{103}\mathrm{Mo}$ showing that, in contrast to their Sr neighbors, the Zr isotopes do not reach maximum of deformation immediately at its onset. This result is rather well reproduced by particle-rotor coupling calculations. A level systematics for the deformed N=61 i…
Frontiers of nuclear structure research and the GSI experimental program
2004
Structure and decay properties of the heaviest elements
2005
Recent results from the study of elements with proton number Z ⩾ 100 are reviewed with emphasis on nuclear structure data from both decay and in-beam studies. Selected data, in particular concerning confirmation experiments, from the study of new elements with Z = 110-112, 114-116 and 118 are also discussed. The experimental equipment used in this work is described and some future possibilities are discussed.
Attempt to calculation of delayed neutron emission probabilities using simple statistical model considerations
1977
Delayed neutron emission probabilities,P n , have been calculated using usual nuclear statistical model considerations. The influence of the incident parameters on the calculatedP n -values is discussed. The observed systematic deviation from the experimental neutron emission probabilities may be explained by the persistence of nuclear structure effects not contained in a simple statistical model.
Nuclear-structure input to r-process calculations
1998
Abstract By comparing results from r-process parameter studies within the classical waiting-point approximation with the observed solar-system r-abundance distribution N r ,⊙ , in-formation on nuclear-structure phenomena on neutron-rich isotopes far off the stability line can be obtained. Such information is — to a large extent — experimentally not accessible. Investigations in the early 1990's, making use of QRPA β-decay properties and nuclear masses from the macroscopic-microscopic FRDM and ETFSI-1 models, showed r-abundance deficiencies around A ⋍115 and 180 , indicating overly strong N=82 and 126 shell strengths far from stability. Recent experiments in the A ⋍110–130 region as well as …