78 research outputs found
Two-proton radioactivity and three-body decay. IV. Connection to quasiclassical formulation
We derive quasiclassical expressions for the three-body decay width and
define the ``preexponential'' coefficients for them. The derivation is based on
the integral formulae for the three-body width obtained in the semianalytical
approach with simplified three-body Hamiltonian [L.V. Grigorenko and M.V.\
Zhukov, arXiv:0704.0920v1]. The model is applied to the decays of the first
excited state of Ne and ground state of Fe.
Various qualitative aspects of the model and relations with the other
simplified approaches to the three-body decays are discussed.Comment: 9 Pages, 2 figure
Two-proton radioactivity and three-body decay. III. Integral formulae for decay widths in a simplified semianalytical approach
Three-body decays of resonant states are studied using integral formulae for
decay widths. Theoretical approach with a simplified Hamiltonian allows
semianalytical treatment of the problem. The model is applied to decays of the
first excited state of Ne and the ground state of
Fe. The convergence of three-body hyperspherical model calculations to
the exact result for widths and energy distributions are studied. The
theoretical results for Ne and Fe decays are updated and
uncertainties of the derived values are discussed in detail. Correlations for
the decay of Ne state are also studied.Comment: 19 pages, 20 figure
Evidence for the pair-breaking process in 116,117Sn
The nuclear level densities of 116,117Sn below the neutron separation energy
have been determined experimentally from the (3He,alpha gamma) and (3He,3He
gamma') reactions, respectively. The level densities show a characteristic
exponential increase and a difference in magnitude due to the odd-even effect
of the nuclear systems. In addition, the level densities display pronounced
step-like structures that are interpreted as signatures of subsequent breaking
of nucleon pairs.Comment: 7 pages, 5 figures, accepted for publication in Phys. Rev. C, 22
December 200
Nuclear level densities and gamma-ray strength functions in 44,45Sc
The scandium isotopes 44,45Sc have been studied with the 45Sc(3He,alpha
gamma)44Sc and 45Sc(3He,3He' gamma)45Sc reactions, respectively. The nuclear
level densities and gamma-ray strength functions have been extracted using the
Oslo method. The experimental level densities are compared to calculated level
densities obtained from a microscopic model based on BCS quasiparticles within
the Nilsson level scheme. This model also gives information about the parity
distribution and the number of broken Cooper pairs as a function of excitation
energy. The experimental gamma-ray strength functions are compared to
theoretical models of the E1, M1, and E2 strength, and to data from (gamma,n)
and (gamma,p) experiments. The strength functions show an enhancement at low
gamma energies that cannot be explained by the present, standard models.Comment: 21 pages, 13 figures. Published versio
Alpha-nucleus potential for alpha-decay and sub-barrier fusion
The set of parameters for alpha-nucleus potential is derived by using the
data for both the alpha-decay half-lives and the fusion cross-sections around
the barrier for reactions alpha+40Ca, alpha+59Co, alpha+208Pb. The alpha-decay
half-lives are obtained in the framework of a cluster model using the WKB
approximation. The evaluated alpha-decay half-lives and the fusion
cross-sections agreed well with the data. Fusion reactions between
alpha-particle and heavy nuclei can be used for both the formation of very
heavy nuclei and spectroscopic studies of the formed compound nuclei.Comment: 10 pages, 5 figure
Microcanonical entropies and radiative strength functions of V
The level densities and radiative strength functions (RSFs) of V
have been extracted using the (He,) and
(He,He) reactions, respectively. From the level
densities, microcanonical entropies are deduced. The high -energy part
of the RSF is described by the giant electric dipole resonance. A significant
enhancement over the predicted strength in the region of MeV is seen, which at present has no theoretical explanation.Comment: 16 pages including 9 figure
Level density of Fe and low-energy enhancement of -strength function
The MnFe differential cross section is measured at
MeV\@. The Fe level density obtained from neutron evaporation spectra is
compared to the level density extracted from the
FeHe,Fe reaction by the Oslo-type technique.
Good agreement is found between the level densities determined by the two
methods. With the level density function obtained from the neutron evaporation
spectra, the Fe -strength function is also determined from the
first-generation matrix of the Oslo experiment. The good agreement
between the past and present results for the -strength function
supports the validity of both methods and is consistent with the low-energy
enhancement of the strength below MeV first discovered by the
Oslo method in iron and molybdenum isotopes.Comment: 7 pages, 5 figure
Proton Decay from Excited States in Spherical Nuclei
Based on a single particle model which describes the time evolution of the
wave function during tunneling across a one dimensional potential barrier we
study the proton decay of Pb from excited states with non-vanishing
angular momentum . Several quantities of interest in this process like
the decay rate , the period of oscillation , the transient
time , the tunneling time and the average value of the proton
packet position are computed and compared with the WKB results.Comment: 12 pages, 4 figure
Instantaneous Shape Sampling - a model for the -absorption cross section of transitional nuclei
The influence of the quadrupole shape fluctuations on the dipole vibrations
in transitional nuclei is investigated in the framework of the Instantaneous
Shape Sampling Model, which combines the Interacting Boson Model for the slow
collective quadrupole motion with the Random Phase Approximation for the rapid
dipole vibrations. Coupling to the complex background configurations is taken
into account by folding the results with a Lorentzian with an energy dependent
width. The low-energy energy portion of the - absorption cross section,
which is important for photo-nuclear processes, is studied for the isotopic
series of Kr, Xe, Ba, and Sm. The experimental cross sections are well
reproduced. The low-energy cross section is determined by the Landau
fragmentation of the dipole strength and its redistribution caused by the shape
fluctuations. Collisional damping only wipes out fluctuations of the absorption
cross section, generating the smooth energy dependence observed in experiment.
In the case of semi-magic nuclei, shallow pygmy resonances are found in
agreement with experiment
Pygmy dipole strength close to particle-separation energies - the case of the Mo isotopes
The distribution of electromagnetic dipole strength in 92, 98, 100 Mo has
been investigated by photon scattering using bremsstrahlung from the new ELBE
facility. The experimental data for well separated nuclear resonances indicate
a transition from a regular to a chaotic behaviour above 4 MeV of excitation
energy. As the strength distributions follow a Porter-Thomas distribution much
of the dipole strength is found in weak and in unresolved resonances appearing
as fluctuating cross section. An analysis of this quasi-continuum - here
applied to nuclear resonance fluorescence in a novel way - delivers dipole
strength functions, which are combining smoothly to those obtained from
(g,n)-data. Enhancements at 6.5 MeV and at ~9 MeV are linked to the pygmy
dipole resonances postulated to occur in heavy nuclei.Comment: 6 pages, 5 figures, proceedings Nuclear Physics in Astrophysics II,
May 16-20, Debrecen, Hungary. The original publication is available at
www.eurphysj.or
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