46,341 research outputs found

    Reprocessed emission from warped accretion discs induced by the Bardeen-Petterson effect

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    The broad Balmer emission-line profiles resulting from the reprocessing of UV/X-ray radiation from a warped accretion disc induced by the Bardeen-Petterson effect are studied. We adopt a thin warped disc geometry and a central ring-like illuminating source in our model. We compute the steady-state shape of the warped disc numerically, and then use it in the calculation of the line profile. We find that, from the outer radius to the inner radius of the disc, the warp is twisted by an angle of ∼π\sim\pi before being flattened efficiently into the equatorial plane. The profiles obtained depend weakly on the illuminating source radius in the range from 3rg3r_{g} to 10rg10r_g, but depend strongly on this radius when it approaches the marginally stable orbit of an extreme Kerr black hole. Double- or triplet-peaked line profiles are present in most cases when the illuminating source radius is low. The triplet-peaked line profiles observed from the Sloan Digital Sky Survey may be a {"}signature" of a warped disc.Comment: 8 pages, 6 figures, typos corrected, matches version to appear in MNRA

    Study of Minor Actinides Transmutation in PWR MOX fuel

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    The management of long-lived radionuclides in spent fuel is a key issue to achieve the closed nuclear fuel cycle and the sustainable development of nuclear energy. Partitioning-Transmutation is supposed to be an efficient method to treat the long-lived radionuclides in spent fuel. Some Minor Actinides (MAs) have very long half-lives among the radionuclides in the spent fuel. Accordingly, the study of MAs transmutation is a significant work for the post-processing of spent fuel. In the present work, the transmutations in Pressurized Water Reactor (PWR) mixed oxide (MOX) fuel are investigated through the Monte Carlo based code RMC. Two kinds of MAs, 237^{237}Np and five MAs (237^{237}Np, 241^{241}Am, 243^{243}Am, 244^{244}Cm and 245^{245}Cm) are incorporated homogeneously into the MOX fuel assembly. The transmutation of MAs is simulated with different initial MOX concentrations. The results indicate an overall nice efficiency of transmutation in both initial MOX concentrations, especially for the two kinds of MAs primarily generated in the UOX fuel, 237^{237}Np and 241^{241}Am. In addition, the inclusion of 237^{237}Np in MOX has no large influence for other MAs, while the transmutation efficiency of 237^{237}Np is excellent. The transmutation of MAs in MOX fuel depletion is expected to be a new, efficient nuclear spent fuel management method for the future nuclear power generation

    A study of turbulent flows about oscillating airfoils

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    Issued as Progress reports [1-6], and Technical report, Project no. E-16-66
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