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Charmed Baryon Weak Decays with SU(3) Flavor Symmetry

机译:具有sU(3)风味对称性的迷人重子弱衰变

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摘要

We study the semileptonic and non-leptonic charmed baryon decays with $SU(3)$flavor symmetry, where the charmed baryons can be ${\bfB}_{c}=(\Xi_c^0,\Xi_c^+,\Lambda_c^+)$, ${\bfB}'_{c}=(\Sigma_c^{(++,+,0)},\Xi_{c}^{\prime(+,0)},\Omega_c^0)$, ${\bfB}_{cc}=(\Xi_{cc}^{++},\Xi_{cc}^+,\Omega_{cc}^+)$, or ${\bfB}_{ccc}=\Omega^{++}_{ccc}$. With ${\bf B}_n^{(\prime)}$ denoted as the baryonoctet (decuplet), we find that the ${\bf B}_{c}\to {\bf B}'_n\ell^+\nu_\ell$decays are forbidden, while the $\Omega_c^0\to \Omega^-\ell^+\nu_\ell$,$\Omega_{cc}^+\to\Omega_c^0\ell^+\nu_\ell$, and $\Omega_{ccc}^{++}\to\Omega_{cc}^+\ell^+\nu_\ell$ decays are the only existing Cabibbo-allowed modesfor ${\bf B}'_{c}\to {\bf B}'_n\ell^+\nu_\ell$, ${\bf B}_{cc}\to {\bfB}'_c\ell^+\nu_\ell$, and ${\bf B}_{ccc}\to {\bfB}_{cc}^{(\prime)}\ell^+\nu_\ell$, respectively. We predict the rarely studied${\bf B}_{c}\to {\bf B}_n^{(\prime)}M$ decays, such as ${\calB}(\Xi_c^0\to\Lambda^0\bar K^0,\,\Xi_c^+\to\Xi^0\pi^+)=(8.3\pm 0.9,8.0\pm4.1)\times 10^{-3}$ and ${\cal B}(\Lambda_c^+\to\Delta^{++}\pi^-,\,\Xi_c^0\to\Omega^- K^+)=(5.5\pm 1.3,4.8\pm 0.5)\times10^{-3}$. For the observation, the doubly and triply charmed baryon decays of$\Omega_{cc}^{+}\to \Xi_c^+\bar K^0$, $\Xi_{cc}^{++}\to (\Xi_c^+\pi^+$,$\Sigma_c^{++}\bar K^0)$, and $\Omega_{ccc}^{++}\to (\Xi_{cc}^{++}\barK^0,\Omega_{cc}^+\pi^+,\Xi_c^+ D^+)$ are the favored Cabibbo-allowed decays,which are accessible to the BESIII and LHCb experiments.
机译:我们研究具有$ SU(3)$ flavor对称性的半轻子和非轻子有魅力的重子衰变,其中有魅力的重子可以是$ {\ bfB} _ {c} =(\ Xi_c ^ 0,\ Xi_c ^ +,\ Lambda_c ^ +)$,$ {\ bfB}'_ {c} =(\ Sigma_c ^ {(++,+,0)},\ Xi_ {c} ^ {\ prime(+,0)},\ Omega_c ^ 0)$,$ {\ bfB} _ {cc} =(\ Xi_ {cc} ^ {++},\ Xi_ {cc} ^ +,\ Omega_ {cc} ^ +)$或$ {\ bfB} _ {ccc} = \ Omega ^ {++} _ {ccc} $。将$ {\ bf B} _n ^ {(\ prime)} $表示为重音八位字节(十进制),我们发现$ {\ bf B} _ {c} \ to {\ bf B}'_ n \ ell ^ + \ nu_ \ ell $禁止衰减,而$ \ Omega_c ^ 0 \至\ Omega ^-\ ell ^ + \ nu_ \ ell $,$ \ Omega_ {cc} ^ + \至\ Omega_c ^ 0 \ ell ^ + \ nu_ \ ell $和$ \ Omega_ {ccc} ^ {++} \ to \ Omega_ {cc} ^ + \ ell ^ + \ nu_ \ ell $衰减是$ {\ bf仅有的Cabibbo允许模式B}'_ {c} \ to {\ bf B}'_ n \ ell ^ + \ nu_ \ ell $,$ {\ bf B} _ {cc} \ to {\ bfB}'_ c \ ell ^ + \ nu_ \ ell $和$ {\ bf B} _ {ccc} \至{\ bfB} _ {cc} ^ {(\ prime)} \ ell ^ + \ nu_ \ ell $。我们预测很少研究的$ {\ bf B} _ {c} \至{\ bf B} _n ^ {(\ prime)} M $衰减,例如$ {\ calB}(\ Xi_c ^ 0 \ to \ Lambda ^ 0 \ bar K ^ 0,\,\ Xi_c ^ + \到\ Xi ^ 0 \ pi ^ +)=(8.3 \ pm 0.9,8.0 \ pm4.1)\乘以10 ^ {-3} $和$ { \ cal B}(\ Lambda_c ^ + \ to \ Delta ^ {++} \ pi ^-,\,\ Xi_c ^ 0 \ to \ Omega ^-K ^ +)=(5.5 \ pm 1.3,4.8 \ pm 0.5 )\ times10 ^ {-3} $。为了进行观察,$ \ Omega_ {cc} ^ {+} \到\ Xi_c ^ + \ bar K ^ 0 $,$ \ Xi_ {cc} ^ {++} \ to(\\ Xi_c ^ + \ pi ^ + $,$ \ Sigma_c ^ {++} \ bar K ^ 0)$和$ \ Omega_ {ccc} ^ {++} \ to(\ Xi_ {cc} ^ {++} \ barK ^ 0,\ Omega_ {cc} ^ + \ pi ^ +,\ Xi_c ^ + D ^ +)$是最受Cabibbo允许的衰变,可通过BESIII和LHCb实验获得。

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