$\bf{
824 \pm30}$
|
OUR AVERAGE
|
$826$ $\pm49$ ${}^{+49}_{-34}$ |
1.3k |
1 |
|
BES2 |
$810$ $\pm68$ ${}^{+15}_{-24}$ |
1.4k |
2 |
|
BES2 |
$878$ $\pm23$ ${}^{+64}_{-55}$ |
25k |
3 |
|
BES2 |
$797$ $\pm19$ $\pm43$ |
15k |
4, 5 |
|
E791 |
• • • We do not use the following data for averages, fits, limits, etc. • • • |
$888.0$ $\pm1.9$ |
141k |
6 |
|
CLEO |
$856$ $\pm17$ $\pm13$ |
54k |
7 |
|
FOCS |
$855$ $\pm15$ |
0.6k |
8 |
|
CLEO |
$905$ ${}^{+65}_{-30}$ |
|
9 |
|
RVUE |
1
The Breit-Wigner parameters from a fit with seven intermediate resonances. The S-matrix pole position is ($764$ $\pm63$ ${}^{+71}_{-54}$) $−$ ${\mit i}$ ($306$ $\pm149$ ${}^{+143}_{-85}$) MeV.
|
2
From a fit including ten additional resonances and energy-independent Breit-Wigner width.
|
3
A fit in the ${{\mathit K}_{{0}}^{*}{(700)}}$ + ${{\mathit K}^{*}{(892)}}$ + ${{\mathit K}^{*}{(1410)}}$ model with mass and width of the ${{\mathit K}_{{0}}^{*}{(700)}}$ from ABLIKIM 2006C well describes the left slope of the ${{\mathit K}_S^0}$ ${{\mathit \pi}^{-}}$ invariant mass spectrum in ${{\mathit \tau}^{-}}$ $\rightarrow$ ${{\mathit K}_S^0}$ ${{\mathit \pi}^{-}}{{\mathit \nu}_{{\tau}}}$ decay studied by EPIFANOV 2007 . Averaged value from different parameterizations.
|
4
Not seen by KOPP 2001 using 7070 events of ${{\mathit D}^{0}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{0}}$ . LINK 2002E and LINK 2005I show clear evidence for a constant non-resonant scalar amplitude rather than ${{\mathit K}_{{0}}^{*}{(700)}}$ in their high statistics analysis of ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \mu}^{+}}{{\mathit \nu}_{{\mu}}}$ .
|
5
AUBERT 2007T does not find evidence for the charged ${{\mathit K}_{{0}}^{*}{(700)}}$ using 11k events of ${{\mathit D}^{0}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit K}^{+}}{{\mathit \pi}^{0}}$ .
|
6
Using parameters from the model that fits data best.
|
7
A Breit-Wigner mass and width.
|
8
Breit-Wigner parameters. A significant ${\mathit S}{\mathrm -wave}$ can be also modeled as a non-resonant contribution.
|
9
Reanalysis of ASTON 1988 using interfering Breit-Wigner amplitudes.
|