21,960 research outputs found

    Shell and isospin effects in nuclear charge radii

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    The shell effect and isospin effect in nuclear charge radii are systematically investigated and a four-parameter formula is proposed for the description of the root-mean-square (rms) charge radii by combining the shell corrections and deformations of nuclei obtained from the Weizs\"acker-Skyrme mass model. The rms deviation with respect to the 885 measured charge radii falls to 0.022 fm. The proposed formula is also applied for the study of the charge radii of super-heavy nuclei and nuclear symmetry energy. The linear relationship between the slope parameter L of the nuclear symmetry energy and the rms charge radius difference of 30S - 30Si mirror pair is clearly observed. The estimated slope parameter is about L=54±19L=54 \pm 19 MeV from the coefficient of the isospin term in the proposed charge radius formula.Comment: 7 figures, 1 table, accepted for publication as a Rapid Communication in Physical Review

    GPU-based Efficient Join Algorithms on Hadoop

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    The growing data has brought tremendous pressure for query processing and storage, so there are many studies that focus on using GPU to accelerate join operation, which is one of the most important operations in modern database systems. However, existing GPU acceleration join operation researches are not very suitable for the join operation on big data. Based on this, this paper speeds up nested loop join, hash join and theta join, combining Hadoop with GPU, which is also the first to use GPU to accelerate theta join. At the same time, after the data pre-filtering and pre-processing, using Map-Reduce and HDFS in Hadoop proposed in this paper, the larger data table can be handled, compared to existing GPU acceleration methods. Also with Map-Reduce in Hadoop, the algorithm proposed in this paper can estimate the number of results more accurately and allocate the appropriate storage space without unnecessary costs, making it more efficient. The rigorous experiments show that the proposed method can obtain 1.5 to 2 times the speedup, compared to the traditional GPU acceleration equi join algorithm. And in the synthetic data set, the GPU version of the proposed method can get 1.3 to 2 times the speedup, compared to CPU version.Comment: 39 page

    Impurity effects and ferromagnetism in excitonic insulators

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    Both nonmagnetic and magnetic impurity effects in spin singlet and triplet excitonic insulators were investigated. The bound state energies caused by single impurity were given. The different compositions of the bound states can be used to detect the symmetry of the excitonic insulators. In finite concentration problems, nonmagnetic impurities showed same pair-breaking effect in singlet and triplet excitonic insulators while magnetic impurities showed weaker pair-breaking effect in triplet excitonic insulators than in singlet ones. The pair-breaking effects suppressed the ferromagnetic range via doping and gave a natural explaination for experimental results.Comment: 7 pages, 4 figure

    Mechanism of production of light complex particles in nucleon-induced reactions

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    The Improved Quantum Molecular Dynamics (ImQMD) model incorporated with the statistical decay model is successful in describing emission of nucleons in the intermediate energy spallation reactions, but not good enough in describing productions of light complex particles, i.e. dd, tt, 3^3He and 4^4He. To improve the description on emission of light complex particles, a phenomenological mechanism called surface coalescence and emission is introduced into ImQMD model: nucleon ready to escape from the compound nuclei can coalesce with the other nucleon(s) to form light complex particle and be emitted. With updated ImQMD model, the description on the experimental data of light complex particles produced in nucleon-induced reactions are great improved.Comment: 17 pages, 6 figures. arXiv admin note: text overlap with arXiv:nucl-th/0606004 by other author

    Microscopic dynamics simulations of heavy-ion fusion reactions induced by neutron-rich nuclei

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    The heavy-ion fusion reactions induced by neutron-rich nuclei are investigated with the improved quantum molecular dynamics (ImQMD) model. With a subtle consideration of the neutron skin thickness of nuclei and the symmetry potential, the stability of nuclei and the fusion excitation functions of heavy-ion fusion reactions 16^{16}O+76^{76}Ge, 16^{16}O+154^{154}Sm, 40^{40}Ca+96^{96}Zr and 132^{132}Sn+40^{40}Ca are systematically studied. The fusion cross sections of these reactions at energies around the Coulomb barrier can be well reproduced by using the ImQMD model. The corresponding slope parameter of the symmetry energy adopted in the calculations is L≈78L \approx 78 MeV and the surface energy coefficient is gsur=18±1.5g_{\rm sur}=18\pm 1.5 MeVfm2^2. In addition, it is found that the surface-symmetry term significantly influences the fusion cross sections of neutron-rich fusion systems. For sub-barrier fusion, the dynamical fluctuations in the densities of the reaction partners and the enhanced surface diffuseness at neck side result in the lowering of the fusion barrier.Comment: 10 figures, the version published in PR

    Improved Kelson-Garvey mass relations for proton-rich nuclei

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    The improved Kelson-Garvey (ImKG) mass relations are proposed from the mass differences of mirror nuclei. The masses of 31 measured proton-rich nuclei with 7≤A≤417\leq A\leq41 and −5≤(N−Z)≤−3-5\leq (N-Z)\leq-3 can be remarkably well reproduced by using the proposed relations, with a root-mean-square deviation of 0.398 MeV, which is much smaller than the results of Kelson-Garvey (0.502 MeV) and Isobar-Mirror mass relations (0.647 MeV). This is because many more masses of participating nuclei are involved in the ImKG mass relations for predicting the masses of unknown proton-rich nuclei. The masses for 144 unknown proton-rich nuclei with 6≤A≤746\leq A\leq74 are predicted by using the ImKG mass relations. The one- and two-proton separation energies for these proton-rich nuclei and the diproton emission are investigated simultaneously.Comment: 23 Pages,7figures,to be published in Phys. Rev.

    Dynamical and statistical description of multifragmentation in heavy-ion collisions

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    To explore the roles of dynamical model and statistical model in the description of multifragmentation in heavy-ion collisions at intermediate energies, the fragments charge distributions of 197^{197}Au+197^{197}Au at 35 MeV/u are analyzed by using the hybrid model of improved quantum molecular dynamics (ImQMD) model plus the statistical model GEMINI. We find that, the ImQMD model can well describe the charge distributions of fragments produced in central and semi-central collisions. But for the peripheral collisions of Au+Au at 35 MeV/u, the statistical model is required at the end of the ImQMD simulations for the better description of the charge distribution of fragments. By using the hybrid model of ImQMD+GEMINI, the fragment charge distribution of Au+Au at 35 MeV/u can be reproduced reasonably well. The time evolution of the excitation energies of primary fragments is simultaneously investigated.Comment: 6 pages, 3 figure

    Fusion and quasi-fission dynamics in nearly-symmetric reactions

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    Some nearly-symmetric fusion reactions are systematically investigated with the improved quantum molecular dynamics (ImQMD) model. By introducing two-body inelastic scattering in the Fermi constraint procedure, the stability of an individual nucleus and the description of fusion cross sections at energies near the Coulomb barrier can be further improved. Simultaneously, the quasi-fission process in 154^{154}Sm+160^{160}Gd is also investigated with the microscopic dynamics model for the first time. We find that at energies above the Bass barrier, the fusion probability is smaller than 10−510^{-5} for this reaction, and the nuclear contact-time is generally smaller than 15001500 fm/c. From the central collisions of Sm+Gd, the neutron-rich fragments such as 164,165^{164,165}Gd, 192^{192}W can be produced in the ImQMD simulations, which implies that the quasi-fission reaction could be an alternative way to synthesize new neutron-rich heavy nuclei.Comment: 11 figure

    Search for possible way of producing super-heavy elements-Dynamic study on damped reactions of 244Pu+244Pu,238U+238U+238U and 197Au+197Au

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    By using the improved Quantum Molecular Dynamics model, the 244^{244}Pu+244^{244}Pu, 238^{238}U+238^{238}U and 197^{197}Au+197^{197}Au reactions at the energy range of Ec.m.E_{c.m.}=800 MeVMeV to 2000 MeVMeV are studied. We find that the production probability of superheavy fragments(SHF) with Z≥Z \geq 114 is much higher for 244^{244}Pu+244^{244}Pu reaction compared with that of 238^{238}U+238^{238}U reaction and no product of SHF is found for 197^{197}Au+197^{197}Au. The production probability of SHF is narrowly peaked in incident energy dependence. The decay mechanism of the composite system of projectile and target and the time scale of decay process are explored. The binding energies of superheavy fragments are found to be broadly distributed and their shapes turn out to be exotic form.Comment: 6 pages, 5 figures, 1 tabl

    Determination of the nucleon-nucleon interaction in the ImQMD model by nuclear reaction at the Fermi energy region

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    The nucleon-nucleon interaction is investigated by using the ImQMD model with the three sets of parameters IQ1, IQ2 and IQ3 in which the corresponding incompressibility coefficients of nuclear matter are different. The charge distribution of fragments for various reaction systems are calculated at different incident energies. The parameters strongly affect the charge distribution below the threshold energy of nuclear multifragmentation. The fragment multiplicity spectrum for 238^{238}U+197^{197}Au at 15 AMeV and the charge distribution for 129^{129}Xe+120^{120}Sn at 32 and 45 AMeV, and 197^{197}Au+197^{197}Au at 35 AMeV are reproduced by the ImQMD model with the set of parameter IQ3. It is concluded that charge distribution of the fragments and the fragment multiplicity spectrum are good observables for studying N-N interaction, the Fermi energy region is a sensitive energy region to explore the N-N interaction, and IQ3 is a suitable set of parameters for the ImQMD model.Comment: 10pages,6figure
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