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Recent Progress on Three-Body Nonmesonic Weak Decay of A Hypernuclei

机译:超核三体非中子弱衰变的最新进展

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摘要

One important recent developement of nonmesonic weak decay (NMWD) study of hypernuclei is the experimentatl confirmation of three-body NMWD and the finding of its big branching ratio, which is comparable to those of two-body NMWD channels. The implication is that the current values of Γ_n and Γ_p, which are fundamentally important for the study of baryon-baryon weak interaction but have been determined without taking accounts of the three-body NMWD, should be significanly modified. We have recently obtained the branching ratio of the three-body NMWD attributing the quenching of nucleon yields in the NMWD due to the presence of the three-body NMWD. In order to disentangle the effects of the final state interaction (FSI), which occupies the same three-body phase space as the three-body NMWD, we adopted a novel renormalization method of INC (Intranuclear Cascade) calculation. We obtained the branching ratios, Γ_(2N)/Γ_(nm), 0.29±0.13 for _Λ~(12)C and 0.26±0.13 (preliminary) for _Λ~(11)B. This big branching ratio, Γ_(2n)/Γ~(nm), has also been confirmed by the recent reports from FINUDA experiment. These results are quite consistent with those of the theoretical calculations. It seems that the strong contribution of the three-body NMWD is not accidental, but a universal characteristics of NMWD, though the current error bars of the measured values are quite large. The accurate measurement of its branching ratio becomes one of the most urgent issues. Such a big contribution of three-body effect is quite unique so that it provides an excellent means for the numerical studies of three-body interaction models.
机译:超核的非中子弱衰减(NMWD)研究的一项最新重要进展是对三体NMWD的实验确认和发现其大分支比,这与两体NMWD通道的可比性相当。这意味着对于重子-重子弱相互作用的研究至关重要的,但在未考虑三体NMWD的情况下确定的Γ_n和Γ_p的当前值应该进行显着修改。我们最近获得了三体NMWD的分支比,归因于三体NMWD的存在,其归因于NMWD中核子产量的淬灭。为了消除最终状态相互作用(FSI)的影响,该状态占据了与三体NMWD相同的三体相空间,我们采用了一种新颖的INC(核级联)计算方法。得到支化比Γ_(2N)/Γ_(nm),对于_Λ〜(12)C为0.29±0.13,对于_Λ〜(11)B为0.26±0.13(初步)。 FINUDA实验的最新报道也证实了这种大的分支比Γ_(2n)/Γ〜(nm)。这些结果与理论计算非常一致。似乎三体NMWD的强大贡献不是偶然的,而是NMWD的普遍特性,尽管测量值的当前误差线很大。准确测量其分支比例成为最紧迫的问题之一。三体效应的如此巨大的贡献是非常独特的,从而为三体相互作用模型的数值研究提供了极好的手段。

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  • 来源
    《原子核研究》 |2013年第3期|166-172|共7页
  • 作者单位

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea;

    Department of Physics, Osaka University, Toyonaga 560-0043, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan;

    Gesellschaft fur Schwerionenforschung mbH (GSI), Darmstadt 64291 Germany;

    Lab. of Physics, Osaka Electro Communication University, Neyagawa 572-8530, Japan;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Department of Physics, Ewha Womans University, Seoul 120-750, Korea;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea,Institute of Basic Science, Daejeon 305-811, Korea;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea,Korea Research Institute of Standards and Science (KRISS), Daejeon 305-600, Korea;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea,Institute of Basic Science, Daejeon 305-811, Korea;

    Department of Physics, University of Tokyo, Hongo 113-0033, Japan;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Department of Physics, Osaka University, Toyonaga 560-0043, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan,Department of Physics, Kyoto University, Kyoto 606-8502, Japan;

    Department of Physics, University of Tokyo, Hongo 113-0033, Japan;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan,Department of Physics, Osaka University, Toyonaga 560-0043, Japan;

    Department of Physics, Tokyo Institute of Technology, Ookayama 152-8551, Japan,INFN-LNF, Frascati 00044, Italy;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan,Riken Nishina Center, Riken, Wako 351-0198, Japan;

    Korea Research Institute of Standards and Science (KRISS), Daejeon 305-600, Korea;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan,Japan Atomic Energy Research Institute, Tokai 319-1195, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Riken Nishina Center, Riken, Wako 351-0198, Japan,Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea;

    High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801, Japan;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea,Institute of Basic Science, Daejeon 305-811, Korea;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Department of Physics, Tohoku University, Sendai 980-8578, Japan;

    Department of Physics and Astronomy, Seoul National University, Seoul 151-747, Korea,Korea Institute of Radiological and Medical Science, Seoul 139-706, Korea;

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