${{\mathit \omega}{(782)}}$ MASS

INSPIRE   PDGID:
M001M
VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT
$\bf{ 782.66 \pm0.13}$ OUR AVERAGE  Error includes scale factor of 2.0.  See the ideogram below.
$777.9$ $\pm2.2$ ${}^{+4.3}_{-2.2}$ 900k
ANDREEV
2020
H1 ${{\mathit e}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
$783.20$ $\pm0.13$ $\pm0.16$ 18680
AKHMETSHIN
2005
CMD2 0.60-1.38 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{0}}{{\mathit \gamma}}$
$782.68$ $\pm0.09$ $\pm0.04$ 11200 1
AKHMETSHIN
2004
CMD2 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$782.79$ $\pm0.08$ $\pm0.09$ 1.2M 2
ACHASOV
2003D
RVUE $0.44 - 2.00$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$781.96$ $\pm0.17$ $\pm0.80$ 11k 3
AMSLER
1994C
CBAR $0.0$ ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \eta}}{{\mathit \pi}^{0}}$
$782.08$ $\pm0.36$ $\pm0.82$ 3463 4
AMSLER
1994C
CBAR $0.0$ ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \eta}}{{\mathit \pi}^{0}}$
$781.96$ $\pm0.13$ $\pm0.17$ 15k
AMSLER
1993B
CBAR $0.0$ ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit \pi}^{0}}{{\mathit \pi}^{0}}$
$782.4$ $\pm0.2$ 270k
WEIDENAUER
1993
ASTE ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$782.4$ $\pm0.5$ 7000 5
KEYNE
1976
CNTR ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit n}}$
• • We do not use the following data for averages, fits, limits, etc. • •
$782.58$ $\pm0.03$ $\pm0.01$ 6
HOID
2020
RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{0}}{{\mathit \gamma}}$
$781.68$ $\pm0.09$ $\pm0.03$ 7
COLANGELO
2019
RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$
$782.63$ $\pm0.03$ $\pm0.01$ 8
HOFERICHTER
2019
RVUE ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$781.91$ $\pm0.24$ 9
LEES
2012G
BABR ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \gamma}}$
$782.7$ $\pm0.1$ $\pm1.5$ 19500 10
WURZINGER
1995
SPEC 1.33 ${{\mathit p}}$ ${{\mathit d}}$ $\rightarrow$ ${}^{3}\mathrm {He}$ ${{\mathit \omega}}$
$781.78$ $\pm0.10$ 10
BARKOV
1987
CMD ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$782.2$ $\pm0.4$ 1488 11
KURDADZE
1983B
OLYA ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$783.3$ $\pm0.4$ 433
CORDIER
1980
DM1 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$782.5$ $\pm0.8$ 33260
ROOS
1980
RVUE 0.0$-$3.6 ${{\overline{\mathit p}}}{{\mathit p}}$
$782.6$ $\pm0.8$ 3000
BENKHEIRI
1979
OMEG 9$-$12 ${{\mathit \pi}^{\pm}}{{\mathit p}}$
$781.8$ $\pm0.6$ 1430
COOPER
1978B
HBC 0.7$-$0.8 ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ 5 ${{\mathit \pi}}$
$782.7$ $\pm0.9$ 535
VANAPELDOORN
1978
HBC 7.2 ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ ${{\overline{\mathit p}}}{{\mathit p}}{{\mathit \omega}}$
$783.5$ $\pm0.8$ 2100
GESSAROLI
1977
HBC 11 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \omega}}{{\mathit n}}$
$782.5$ $\pm0.8$ 418
AGUILAR-BENIT..
1972B
HBC 3.9,4.6 ${{\mathit K}^{-}}{{\mathit p}}$
$783.4$ $\pm1.0$ 248
BIZZARRI
1971
HBC 0.0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \omega}}$
$781.0$ $\pm0.6$ 510
BIZZARRI
1971
HBC 0.0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit K}_{{{1}}}}{{\mathit K}_{{{1}}}}{{\mathit \omega}}$
$783.7$ $\pm1.0$ 3583 12
COYNE
1971
HBC 3.7 ${{\mathit \pi}^{+}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$784.1$ $\pm1.2$ 750
ABRAMOVICH
1970
HBC 3.9 ${{\mathit \pi}^{-}}{{\mathit p}}$
$783.2$ $\pm1.6$ 13
BIGGS
1970B
CNTR $<$4.1 ${{\mathit \gamma}}$ ${}^{}\mathrm {C}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{}^{}\mathrm {C}$
$782.4$ $\pm0.5$ 2400
BIZZARRI
1969
HBC 0.0 ${{\overline{\mathit p}}}{{\mathit p}}$
1  Update of AKHMETSHIN 2000C.
2  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.
3  From the ${{\mathit \eta}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ decay.
4  From the ${{\mathit \eta}}$ $\rightarrow$ 3 ${{\mathit \pi}^{0}}$ decay.
5  Observed by threshold-crossing technique. Mass resolution = 4.8 MeV FWHM.
6  The values were extracted from a dispersively improved Breit-Wigner parameterization and do not include vacuum polarization. Inclusion of vacuum polarization gives $782.736$ $\pm0.024$ MeV.
7  The ${{\mathit \omega}}$ mass was extracted from a dispersively improved Breit-Wigner parameterization, the ${{\mathit \omega}}$ width fixed at $8.49$ $\pm0.08$ MeV. The value does not include vacuum polarization which would shift the mass to $781.81$ $\pm0.09$ $\pm0.03$ MeV. The mixing parameter is assumed real valued.
8  The values were extracted from a dispersively improved Breit-Wigner parameterization and do not include vacuum polarization.
9  From the ${{\mathit \rho}}−{{\mathit \omega}}$ interference in the ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ mass spectrum using the Breit-Wigner for the ${{\mathit \omega}}$ and leaving its mass and width as free parameters of the fit.
10  Systematic uncertainties underestimated.
11  Systematic uncertainties not estimated.
12  From best-resolution sample of COYNE 1971.
13  From ${{\mathit \omega}}-{{\mathit \rho}}$ interference in the ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}$ mass spectrum assuming ${{\mathit \omega}}$ width 12.6 MeV.

           ${{\mathit \omega}{(782)}}$ mass (MeV)
References