5,093 research outputs found

    Sheldon Hsiao-peng Lu. Transnational Chinese cinemas : identity, nationhood, gender

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    This article reviews the book Transnational Chinese Cinemas: Identity, Nationhood, Gender edited by Sheldon Hsiao-peng Lu

    Anomalous Higgs-top Coupling Pollution on Triple Higgs Coupling Extraction at Future High-Luminosity Electron-Positron Collider

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    One of the most challenging tasks for future high-luminosity electron-positron colliders is to extract Higgs triple coupling. It was proposed that this can be carried out via the precisely measuring the cross section of ZH associated production up to 0.4%0.4\%. In this paper, we example the possible heavy pollution from Higgs-top anomalous coupling. Our numerical results show that the pollution is small for se+eβˆ’=240GeV\sqrt{s}_{e^+e^-}= 240 GeV. However for the higher energy collider, pollution is sizable, which should be taken into account. We further explored the possibility to measure CP-violated Higgs top coupling, via the forward-backward asymmetry AFBA_{FB} for the process e+eβˆ’β†’ZHe^+e^- \rightarrow ZH. The asymmetry can reach 0.7%0.7\% which is comparable to the precision of cross section measurement.Comment: 10 pages, 6 figures, discussions and references added, published in Phys. Rev.

    Proton fraction in neutron stars

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    The proton fraction in {\sl \beta}-stable neutron stars is investigated within the framework of the Skyrme-Hartree-Fock theory using the extended Skyrme effective interaction for the first time. The calculated results show that the proton fraction disappears at high density, which implies that the pure neutron matter may exist in the interior of neutron stars. The incompressibility of the nuclear equation of state is shown to be more important to determine the proton fraction. Meanwhile, it is indicated that the addition of muons in neutron stars will change the proton fraction. It is also found that the higher-order terms of the nuclear symmetry energy have obvious effects on the proton fraction and the parabolic law of the nuclear symmetry energy is not enough to determine the proton fraction.Comment: 4 Pgaes in REVTex, 2 Figures, 1 Tabl

    Relativistic effect of spin and pseudospin symmetries

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    Dirac Hamiltonian is scaled in the atomic units ℏ=m=1\hbar =m=1, which allows us to take the non-relativistic limit by setting the Compton wavelength β†’0% \lambda \rightarrow 0 . The evolutions of the spin and pseudospin symmetries towards the non-relativistic limit are investigated by solving the Dirac equation with the parameter Ξ»\lambda. With Ξ»\lambda transformation from the original Compton wavelength to 0, the spin splittings decrease monotonously in all spin doublets, and the pseudospin splittings increase in several pseudospin doublets, no change, or even reduce in several other pseudospin doublets. The various energy splitting behaviors of both the spin and pseudospin doublets with Ξ»\lambda are well explained by the perturbation calculations of Dirac Hamiltonian in the present units. It indicates that the origin of spin symmetry is entirely due to the relativistic effect, while the origin of pseudospin symmetry cannot be uniquely attributed to the relativistic effect.Comment: 15 pages, 7 figures, accepted by PR
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