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- W939294503 abstract "鉴于目前DS1（2536）粒子的性质存在争议,利用组分夸克模型（CQM）,研究辐射衰变过程DS1（2536）→DS（1968）＋γ.认为DS1（2536）是由c和s-组成的激发态,它的自旋宇称为1＋,属于T类型的双重态（1＋,2＋）.理论计算得到了合理的数值结果,其分支比为1.1%～4.5%,表明所采用的CQM模型及对DS1（2536）的假设是合理的,并希望在将来的实验中能探测到该过程." @default.
- W939294503 created "2016-06-24" @default.
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- W939294503 date "2010-01-01" @default.
- W939294503 modified "2023-09-24" @default.
- W939294503 title "在CQM模型下研究D_（S1）（2536）→D_S（1968）＋γ的过程" @default.
- W939294503 hasPublicationYear "2010" @default.
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