868 research outputs found
Stellar weak-interaction rates for -process waiting-point nuclei from projected shell model
We propose a projected shell model (PSM) for description of stellar
weak-interaction rates between even-even and odd-odd nuclei with extended
configuration space where up to six-quasiparticle (qp) configurations are
included, and the stellar weak-interaction rates for eight -process
waiting-point (WP) nuclei, Ge, Se, Kr, Sr,
Zr, Mo, Ru and Pd, are calculated and analyzed for
the first time within the model. Higher-order qp configurations are found to
affect the underlying Gamow-Teller strength distributions and the corresponding
stellar weak-interaction rates. Under -process environments with high
temperatures and densities, on one hand, thermal population of excited states
of parent nuclei tends to decrease the stellar decay rates. On the
other hand, the possibility of electron capture (EC) tends to provide
increasing contribution to the rates with temperature and density. The
effective half-lives of WP nuclei under the -process peak condition are
predicted to be reduced as compared with the terrestrial case, especially for
Ge and Se
Possible singlet and triplet superconductivity on honeycomb lattice
We study the possible superconducting pairing symmetry mediated by spin and
charge fluctuations on the honeycomb lattice using the extended Hubbard model
and the random-phase-approximation method. From to doping levels,
a spin-singlet -wave is shown to be the leading
superconducting pairing symmetry when only the on-site Coulomb interaction
is considered, with the gap function being a mixture of the nearest-neighbor
and next-nearest-neighbor pairings. When the offset of the energy level between
the two sublattices exceeds a critical value, the most favorable pairing is a
spin-triplet -wave which is mainly composed of the next-nearest-neighbor
pairing. We show that the next-nearest-neighbor Coulomb interaction is also
in favor of the spin-triplet -wave pairing.Comment: 6 pages, 4 figure
Nuclear spectrum from projected shell model (I): allowed one-to-one transition
Nuclear spectrum and the corresponding (anti-)neutrino spectrum play
important roles in many aspects of nuclear astrophysics, particle physics,
nuclear industry and nuclear data. In this work we propose a projected shell
model (PSM) to calculate the level energies as well as the reduced one-body
transition density (ROBTD) by the Pfaffian algorithm for nuclear
decays. The calculated level energies and ROBTD are inputed to the Beta
Spectrum Generator (BSG) code to study the high precision spectrum of
allowed one-to-one transitions. When experimental level energies are adopted,
the calculated spectrum by ROBTD of the PSM deviates from the one by
the extreme simple particle evaluation of the BSG by up to , reflecting
the importance of nuclear many-body correlations. When calculated level
energies are adopted, the calculated spectrum shows sensitive
dependence on the reliability of calculated level energies. The developed
method for ROBTD by the PSM will also be useful for study of the
first-forbidden transitions, the isovector spin monopole resonance etc. in a
straightforward way
Caste-biased Expression of fem and Amdsx Genes in Apis mellifera ligustica (Hymenoptera: Apidae)
Sex determination and caste differentiation are two crucial processes for morphology building in honeybees. It is unclear whether there is an interaction between these two processes. Here, we investigated the expression of fem and Amdsx genes between female castes of honeybees. We found that the expression of fem and Amdsx is significantly higher in queens than in workers, and this expression was positively regulated by juvenile hormone (JH). Our results suggest that sex-determining genes fem and Amdsx are also involved in honeybee caste differentiation
Ceria–terbia solid solution nanobelts with high catalytic activities for CO oxidation
Ceria–terbia solid solution nanobelts were prepared by an electrochemical route and tested as catalysts of high activity for CO oxidation
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