${{\mathit \rho}{(1450)}}$ MASS

${{\mathit \omega}}{{\mathit \pi}}$ MODE

INSPIRE   PDGID:
M105M3
VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$1510$ $\pm7$ 10.2k 1
ACHASOV
2016D
 SND $1.05 - 2.00$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \gamma}}$
$1544$ $\pm22$ ${}^{+11}_{-46}$ 821 2
MATVIENKO
2015
BELL ${{\overline{\mathit B}}^{0}}$ $\rightarrow$ ${{\mathit D}^{*+}}{{\mathit \omega}}{{\mathit \pi}^{-}}$
$1491$ $\pm19$ 7815 3
ACHASOV
2013
SND $1.05 - 2.00$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \gamma}}$
$1582$ $\pm17$ $\pm25$ 2382 4
AKHMETSHIN
2003B
 CMD2 ${{\mathit e}^{+}}$ ${{\mathit e}}$ $\rightarrow$ ${{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \gamma}}$
$1349$ $\pm25$ ${}^{+10}_{-5}$ 341 5
ALEXANDER
2001B
 CLE2 ${{\mathit B}}$ $\rightarrow$ ${{\mathit D}}{}^{(*)}$ ${{\mathit \omega}}{{\mathit \pi}^{-}}$
$1523$ $\pm10$ 6
EDWARDS
2000A
 CLE2 ${{\mathit \tau}^{-}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{-}}{{\mathit \nu}_{{{\tau}}}}$
$1463$ $\pm25$ 7
CLEGG
1994
RVUE
$1250$ 8
ASTON
1980C
 OMEG 20$-$70 ${{\mathit \gamma}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{0}}{{\mathit p}}$
$1290$ $\pm40$ 8
BARBER
1980C
 SPEC 3$-$5 ${{\mathit \gamma}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{0}}{{\mathit p}}$
1  From a phenomenological model based on vector meson dominance with interfering ${{\mathit \rho}{(770)}}$, ${{\mathit \rho}{(1450)}}$, and ${{\mathit \rho}{(1700)}}$. The ${{\mathit \rho}{(1700)}}$ mass and width are fixed at 1720 MeV and 250 MeV, respectively. Systematic uncertainties not estimated. Supersedes ACHASOV 2013.
2  Using Breit-Wigner parameterization of the ${{\mathit \rho}{(1450)}}$ and assuming equal probabilities of the ${{\mathit \rho}{(1450)}}$ $\rightarrow$ ${{\mathit \pi}}{{\mathit \pi}}$ and ${{\mathit \rho}{(1450)}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}}$ decays.
3  From a phenomenological model based on vector meson dominance with the interfering ${{\mathit \rho}{(1450)}}$ and ${{\mathit \rho}{(1700)}}$ and their widths fixed at 400 and 250 MeV, respectively. Systematic uncertainty not estimated.
4  Using the data of AKHMETSHIN 2003B and BISELLO 1991B assuming the ${{\mathit \omega}}{{\mathit \pi}^{0}}$ and ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ mass dependence of the total width. ${{\mathit \rho}{(1700)}}$ mass and width fixed at 1700 MeV and 240 MeV, respectively.
5  Using Breit-Wigner parameterization of the ${{\mathit \rho}{(1450)}}$ and assuming the ${{\mathit \omega}}{{\mathit \pi}^{-}}$ mass dependence for the total width.
6  Mass-independent width parameterization. ${{\mathit \rho}{(1700)}}$ mass and width fixed at 1700 MeV and 235 MeV respectively.
7  Using data from BISELLO 1991B, DOLINSKY 1986 and ALBRECHT 1987L.
8  Not separated from ${{\mathit b}_{{{1}}}{(1235)}}$, not pure $\mathit J{}^{P} = 1{}^{-}$ effect.
References