$\mathbf {B( {{\boldsymbol a}_{{3}}{(1875)}} \rightarrow {{\boldsymbol \rho}_{{3}}{(1690)}} {{\boldsymbol \pi}} )/B( {{\boldsymbol a}_{{3}}{(1875)}} \rightarrow {{\boldsymbol \rho}} {{\boldsymbol \pi}} )}$ INSPIRE search

VALUE DOCUMENT ID TECN  COMMENT
$0.9$ $\pm0.3$ 1
CHUNG
2002
B852 18.3 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{-}}{{\mathit p}}$
1  Using the observable fractions of 50.0$\%$ ${{\mathit \rho}}{{\mathit \pi}}$ , 56.5$\%$ ${{\mathit f}_{{2}}}{{\mathit \pi}}$ , and 11.8$\%$ ${{\mathit \rho}_{{3}}}{{\mathit \pi}}$ .
  References:
CHUNG 2002
PR D65 072001 Exotic and ${\mathit {\mathit q}}{\mathit {\overline{\mathit q}}}$ Resonances in the ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{-}}$ System Produced in ${{\mathit \pi}^{-}}{{\mathit p}}$ Collisions at 18-GeV/$\mathit c$