${\mathit {\mathit b}}$ ${\mathit {\overline{\mathit b}}}$ MESONS
(including possibly non-${\mathit {\mathit q}}$ ${\mathit {\overline{\mathit q}}}$ states)
INSPIRE   JSON PDGID:
M079

${{\mathit \chi}_{{{b0}}}{(2P)}}$

$I^G(J^{PC})$ = $0^+(0^{+ +})$ J need confirmation.
Observed in radiative decay of the ${{\mathit \Upsilon}{(3S)}}$, therefore ${}^{C} = +$. Branching ratio requires E1 transition, M1 is strongly disfavored, therefore ${}^{P} = +$.
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${{\mathit \chi}_{{{b0}}}{(2P)}}$ MASS $10232.5$ $\pm0.4$ $\pm0.5$ MeV 
 
${\mathit m}_{{{\mathit \chi}_{{{b1}}}{(2P)}}}-{\mathit m}_{{{\mathit \chi}_{{{b0}}}{(2P)}}}$ $23.8$ $\pm1.7$ MeV 
 
${{\mathit \gamma}}$ ENERGY IN ${{\mathit \Upsilon}{(3S)}}$ DECAY $121.9$ $\pm0.4$ MeV 
 
▸  ${{\mathit \chi}_{{{b0}}}{(2P)}}$ BRANCHING RATIOS
Mode  
Fraction ($\Gamma_i$ / $\Gamma$) Scale Factor/
Conf. Level
P(MeV/c)  
$\Gamma_{1}$ ${{\mathit \gamma}}{{\mathit \Upsilon}{(2S)}}$ ($1.38$ $\pm0.30$ ) $\%$ 207
 
$\Gamma_{2}$ ${{\mathit \gamma}}{{\mathit \Upsilon}{(1S)}}$ ($3.8$ $\pm1.7$) $ \times 10^{-3}$ 743
 
$\Gamma_{3}$ ${{\mathit D}^{0}}{{\mathit X}}$ <8.2 $\%$ CL=90%  
 
$\Gamma_{4}$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \pi}^{0}}$ $<3.4$ $\times 10^{-5}$ CL=90% 5064
 
$\Gamma_{5}$ 2 ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit K}^{-}}{{\mathit K}_S^0}$ $<5$ $\times 10^{-5}$ CL=90% 5063
 
$\Gamma_{6}$ 2 ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit K}^{-}}{{\mathit K}_S^0}$ 2 ${{\mathit \pi}^{0}}$ $<2.2$ $\times 10^{-4}$ CL=90% 5036
 
$\Gamma_{7}$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}$2 ${{\mathit \pi}^{0}}$ $<2.4$ $\times 10^{-4}$ CL=90% 5092
 
$\Gamma_{8}$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}$ $<1.5$ $\times 10^{-4}$ CL=90% 5050
 
$\Gamma_{9}$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \pi}^{0}}$ $<2.2$ $\times 10^{-4}$ CL=90% 5035
 
$\Gamma_{10}$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}$2 ${{\mathit \pi}^{0}}$ $<1.1$ $\times 10^{-3}$ CL=90% 5019
 
$\Gamma_{11}$ 3 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}{{\mathit K}^{-}}{{\mathit K}_S^0}$ ${{\mathit \pi}^{0}}$ $<7$ $\times 10^{-4}$ CL=90% 5018
 
$\Gamma_{12}$ 3 ${{\mathit \pi}^{+}}$3 ${{\mathit \pi}^{-}}$ $<7$ $\times 10^{-5}$ CL=90% 5091
 
$\Gamma_{13}$ 3 ${{\mathit \pi}^{+}}$3 ${{\mathit \pi}^{-}}$2 ${{\mathit \pi}^{0}}$ $<1.2$ $\times 10^{-3}$ CL=90% 5070
 
$\Gamma_{14}$ 3 ${{\mathit \pi}^{+}}$3 ${{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}$ $<1.5$ $\times 10^{-4}$ CL=90% 5017
 
$\Gamma_{15}$ 3 ${{\mathit \pi}^{+}}$3 ${{\mathit \pi}^{-}}{{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \pi}^{0}}$ $<7$ $\times 10^{-4}$ CL=90% 4999
 
$\Gamma_{16}$ 4 ${{\mathit \pi}^{+}}$4 ${{\mathit \pi}^{-}}$ $<1.7$ $\times 10^{-4}$ CL=90% 5069
 
$\Gamma_{17}$ 4 ${{\mathit \pi}^{+}}$4 ${{\mathit \pi}^{-}}$2 ${{\mathit \pi}^{0}}$ $<6$ $\times 10^{-4}$ CL=90% 5039