28 research outputs found
Level densities and -strength functions in Sm
The level densities and -strength functions of the weakly deformed
Sm and Sm nuclei have been extracted. The temperature versus
excitation energy curve, derived within the framework of the micro canonical
ensemble, shows structures, which we associate with the break up of Cooper
pairs. The nuclear heat capacity is deduced within the framework of both the
micro canonical and the canonical ensemble. We observe negative heat capacity
in the micro canonical ensemble whereas the canonical heat capacity exhibits an
S-shape as function of temperature, both signals of a phase transition. The
structures in the -strength functions are discussed in terms of the
pygmy resonance and the scissors mode built on exited states. The samarium
results are compared with data for the well deformed Dy,
Er and Yb isotopes and with data from
(n,)-experiments and giant dipole resonance studies.Comment: 12 figure
Statistical properties of the well deformed Sm nuclei and the scissors resonance
The Nuclear Level Densities (NLDs) and the -ray Strength Functions
(SFs) of Sm have been extracted from (d,p)
coincidences using the Oslo method. The experimental NLD of Sm is
higher than the NLD of Sm, in accordance with microscopic calculations.
The SFs of Sm are in fair agreement with QRPA calculations
based on the D1M Gogny interaction. An enhancement is observed in the
SF for both Sm nuclei around 3 MeV in excitation energy and
is attributed to the M1 Scissors Resonance (SR). Their integrated strengths
were found to be in the range 1.3 - 2.1 and 4.4 - 6.4 for
Sm and Sm, respectively. The strength of the SR for Sm
is comparable to those for deformed even-even Sm isotopes from nuclear
resonance fluorescence measurements, while that of Sm is lower than
expected
Evolution of the -ray strength function in neodymium isotopes
The experimental gamma-ray strength functions (gamma-SFs) of 142,144-151Nd
have been studied for gamma-ray energies up to the neutron separation energy.
The results represent a unique set of gamma-SFs for an isotopic chain with
increasing nuclear deformation. The data reveal how the low-energy enhancement,
the scissors mode and the pygmy dipole resonance evolve with nuclear
deformation and mass number. The data indicate that the mechanisms behind the
low-energy enhancement and the scissors mode are decoupled from each other.Comment: 14 pages and 10 figure
Nuclear Level Density and -ray Strength Function of and the impact on the i-process
Proton- coincidences from reactions between
a beam and a deuterated polyethylene target have been
analyzed with the inverse Oslo method to find the nuclear level density (NLD)
and -ray strength function (SF) of . The
capture cross section has been calculated
using the Hauser-Feshbach model in TALYS using the measured NLD and SF
as constraints. We confirm that acts as a
bottleneck when relying on one-zone nucleosynthesis calculations. However, we
find that the impact of this reaction is strongly damped in multi-zone
low-metallicity AGB stellar models experiencing i-process nucleosynthesis.Comment: Submitted to Phys. Rev.
New experimental constraint on the W()W cross section
In this work, we present new data on the W() cross
sections, utilizing a quasi-monochromatic photon beam produced at the NewSUBARU
synchrotron radiation facility. Further, we have extracted the nuclear level
density and -ray strength function of W from data on the
W()W reaction measured at the Oslo
Cyclotron Laboratory. Combining previous measurements on the
W() cross section with our new W()
and ()W data sets, we have deduced the
W -ray strength function in the range of MeV
and MeV.
Our data are used to extract the level density and -ray strength
functions needed as input to the nuclear-reaction code \textsf{TALYS},
providing an indirect, experimental constraint for the
W()W cross section and reaction rate. Compared to the
recommended Maxwellian-averaged cross section (MACS) in the KADoNiS-1.0 data
base, our results are on average lower for the relevant energy range keV, and we provide a smaller uncertainty for the MACS. The
theoretical values of Bao \textit{et al.} and the cross section experimentally
constrained on photoneutron data of Sonnabend \textit{et al.} are significantly
higher than our result. The lower value by Mohr \textit{et al.} is in very good
agreement with our deduced MACS. Our new results could have implications for
the -process and in particular the predicted -process production of
Os nuclei.Comment: 17 pages, 15 figures; to be submitted to Phys. Rev.
Anomalies in the Charge Yields of Fission Fragments from the U(n,f)238 Reaction
Fast-neutron-induced fission of 238U at an energy just above the fission threshold is studied with a novel technique which involves the coupling of a high-efficiency γ-ray spectrometer (MINIBALL) to an inverse-kinematics neutron source (LICORNE) to extract charge yields of fission fragments via γ−γ coincidence spectroscopy. Experimental data and fission models are compared and found to be in reasonable agreement for many nuclei; however, significant discrepancies of up to 600% are observed, particularly for isotopes of Sn and Mo. This indicates that these models significantly overestimate the standard 1 fission mode and suggests that spherical shell effects in the nascent fission fragments are less important for low-energy fast-neutron-induced fission than for thermal neutron-induced fission. This has consequences for understanding and modeling the fission process, for experimental nuclear structure studies of the most neutron-rich nuclei, for future energy applications (e.g., Generation IV reactors which use fast-neutron spectra), and for the reactor antineutrino anomaly
Nuclear level densities and γ -ray strength functions of 180,181Ta and neutron capture cross sections
Abstract: Please refer to full text to view abstract
Resonances in odd-odd 182Ta
Abstract: Enhanced γ -decay on the tail of the giant electric dipole resonance, such as the scissors or pygmy resonances, can have significant impact on (n,γ ) reaction rates. These rates are important input for modeling processes that take place in astrophysical environments and nuclear reactors. Recent results from the University of Oslo indicate the existence of a significant enhancement in the photon strength function for nuclei in the actinide region due to the scissors resonance. Further, the M1 strength distribution of the scissors resonances in rare earth nuclei has been studied extensively over the years. To investigate the evolution and persistence of the scissor resonance in other mass regions, an experiment was performed utilizing the NaI(Tl) γ -ray detector array (CACTUS) and silicon particle telescopes (SiRi) at the University of Oslo Cyclotron laboratory. Particle-γ coincidences from the 181Ta(d,p)182Ta and 181Ta(d,d’)181Ta reactions were used to measure the nuclear level density and photon strength function of the well-deformed 181Ta and 182Ta systems, to investigate the existence of resonances below the neutron separation energy