1,864 research outputs found

    Production of proton-rich nuclei around Z=84-90 in fusion-evaporation reactions

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    Within the framework of the dinuclear system model, production cross sections of proton-rich nuclei with charged numbers of Z=84-90 are investigated systematically. Possible combinations with the 28^{28}Si, 32^{32}S, 40^{40}Ar bombarding the target nuclides 165^{165}Ho, 169^{169}Tm, 170−174^{170-174}Yb, 175,176^{175,176}Lu, 174,176−180^{174,176-180}Hf and 181^{181}Ta are analyzed thoroughly. The optimal excitation energies and evaporation channels are proposed to produce the proton-rich nuclei. The systems are feasible to be constructed in experiments. It is found that the neutron shell closure of N=126 is of importance during the evaporation of neutrons. The experimental excitation functions in the 40^{40}Ar induced reactions can be nicely reproduced. The charged particle evaporation is comparable with neutrons in cooling the excited proton-rich nuclei, in particular for the channels with α\alpha and proton evaporation. The production cross section increases with the mass asymmetry of colliding systems because of the decrease of the inner fusion barrier. The channels with pure neutron evaporation depend on the isotopic targets. But it is different for the channels with charged particles and more sensitive to the odd-even effect.Comment: 15 pages, 10 figures. arXiv admin note: text overlap with arXiv:0803.1117, arXiv:0707.258

    Network nonlocality sharing via weak measurements in the generalized star network configuration

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    Network nonlocality exhibits completely novel quantum correlations compared to standard quantum nonlocality. It has been shown that network nonlocality can be shared in a generalized bilocal scenario via weak measurements [Phys. Rev. A. 105, 042436 (2022)]. In this paper, we investigate network nonlocality sharing via weak measurements in a generalized star-shaped network configuration with arbitrary numbers of unbiased dichotomic input kk, which includes nn branches and adds (mm-1) more parties in each branch to the original star network (n,m=1,k=2)(n, m=1, k=2) scenario. It is shown that network nonlocality sharing among all observers can be revealed from simultaneous violation of 2n2^n inequalities in the (n,m=2,k=2n, m=2, k=2) and (n,m=2,k=3n, m=2, k=3) scenarios for any nn branches. The noise resistance of network nonlocality sharing with a precise noise model is also analyzed.Comment: 8 pages, 3 figures. update new result
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