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${{\mathit \omega}{(1420)}}$ MASS

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M125M

M125M VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT $\bf{ 1410 \pm60}$ OUR ESTIMATE • • We do not use the following data for averages, fits, limits, etc. • • $1350$ $\pm43$ 1 DIMOVA 2025   SND ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ $1350$ $\pm43$ 2 ACHASOV 2024 A   SND ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ $1418$ $\pm30$ $\pm10$ 824 3 AKHMETSHIN 2017 A   CMD3 $1.4 - 2.0$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \eta}}$ $1470$ $\pm50$ 13.1k 4 AULCHENKO 2015 A   SND $1.05 - 1.80$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ $1382$ $\pm23$ $\pm70$ AUBERT 2007 AU   BABR 10.6 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \gamma}}$ $1350$ $\pm20$ $\pm20$ AUBERT,B 2004 N   BABR 10.6 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}{{\mathit \gamma}}$ $1400$ $\pm50$ $\pm130$ 1.2M 5 ACHASOV 2003 D   RVUE $0.44 - 2.00$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ $1450$ $\pm10$ 6 HENNER 2002   RVUE $1.2 - 2.0$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \rho}}{{\mathit \pi}}$, ${{\mathit \omega}}{{\mathit \pi}}{{\mathit \pi}}$ $1373$ $\pm70$ 177 7 AKHMETSHIN 2000 D   CMD2 $1.2 - 1.38$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ $1370$ $\pm25$ 5095 ANISOVICH 2000 H   SPEC 0.0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \pi}^{0}}$ $1400$ ${}^{+100}_{-200}$ 8 ACHASOV 1998 H   RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ $\sim$$1400$ 9 ACHASOV 1998 H   RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ $\sim$$1460$ 10 ACHASOV 1998 H   RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit K}^{-}}$ $1440$ $\pm70$ 11 CLEGG 1994   RVUE $1419$ $\pm31$ 315 12 ANTONELLI 1992   DM2 1.34$-2.4{{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \rho}}{{\mathit \pi}}$ 1  From a fit to the cross section with contributions from ${{\mathit \omega}{(782)}}$, ${{\mathit \phi}{(1020)}}$, ${{\mathit \omega}{(1420)}}$, and ${{\mathit \omega}{(1650)}}$. An alternative fit which also includes ${{\mathit \phi}{(1680)}}$ gives $1374$ $\pm27$ MeV with a worse ${{\mathit \chi}^{2}}$. Supersedes ACHASOV 2024A. 2  From a fit to the cross section including contribution from ${{\mathit \omega}{(782)}}$, ${{\mathit \phi}{(1020)}}$, ${{\mathit \omega}{(1420)}}$, and ${{\mathit \omega}{(1650)}}$. Supersedes ACHASOV 2020A. 3  From a fit of the interfering ${{\mathit \omega}{(1420)}}$ and ${{\mathit \omega}{(1650)}}$ with a relative phase of ${{\mathit \pi}}$ and other parameters floating. 4  From a fit with contributions from ${{\mathit \omega}{(782)}}$, ${{\mathit \phi}{(1020)}}$, ${{\mathit \omega}{(1420)}}$, and ${{\mathit \omega}{(1650)}}$. See ACHASOV 2020A for a further analysis of the ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ data. 5  From the combined fit of ANTONELLI 1992, ACHASOV 2001E, ACHASOV 2002E, and ACHASOV 2003D data on the ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$ and ANTONELLI 1992 on the ${{\mathit \omega}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ final states. Supersedes ACHASOV 1999E and ACHASOV 2002E. 6  Using results of CORDIER 1981 and preliminary data of DOLINSKY 1991 and ANTONELLI 1992. 7  Using the data of AKHMETSHIN 2000D and ANTONELLI 1992. The ${{\mathit \rho}}{{\mathit \pi}}$ dominance for the energy dependence of the ${{\mathit \omega}{(1420)}}$ and ${{\mathit \omega}{(1650)}}$ width assumed. 8  Using data from BARKOV 1987, DOLINSKY 1991, and ANTONELLI 1992. 9  Using the data from ANTONELLI 1992. 10  Using the data from IVANOV 1981 and BISELLO 1988B. 11  From a fit to two Breit-Wigner functions and using the data of DOLINSKY 1991 and ANTONELLI 1992. 12  From a fit to two Breit-Wigner functions interfering between them and with the $\omega ,\phi $ tails with fixed ($+,–,+$) phases.

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