${{\mathit K}^{*}{(892)}}$ WIDTH

NEUTRAL ONLY

INSPIRE   JSON  (beta) PDGID:
M018W2
VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT
$\bf{ 47.3 \pm0.5}$ OUR FIT  Error includes scale factor of 2.0.
$\bf{ 47.3 \pm0.5}$ OUR AVERAGE  Error includes scale factor of 2.0.  See the ideogram below.
$46.53$ $\pm0.56$ $\pm0.31$ 1
ABLIKIM
01F
 
BES3 ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit e}^{+}}{{\mathit \nu}_{{{e}}}}$
$46.5$ $\pm0.3$ $\pm0.2$ 243k 2
DEL-AMO-SANCH..
01I
 
BABR ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit e}^{+}}{{\mathit \nu}_{{{e}}}}$
$45.3$ $\pm0.5$ $\pm0.6$ 141k 3
BONVICINI
00A
 
CLEO ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{+}}$
$47.79$ $\pm0.86$ ${}^{+1.32}_{-1.06}$ 18k 4
LINK
00I
 
FOCS ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \mu}^{+}}{{\mathit \nu}_{{{\mu}}}}$
$54$ $\pm3$
BARBERIS
99E
 
OMEG 450 ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit p}_{{{f}}}}{{\mathit p}_{{{s}}}}{{\mathit K}^{*}}{{\overline{\mathit K}}^{*}}$
$50.8$ $\pm0.8$ $\pm0.9$
ASTON
98
 
LASS 11 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit n}}$
$46.5$ $\pm4.3$ 5900
BARTH
98
 
HBC 70 ${{\mathit K}^{+}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}$ X
$54$ $\pm2$ 28k
EVANGELISTA
98
 
OMEG 10 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}$( ${{\mathit \Lambda}}$ ,${{\mathit \Sigma}}$)
$45.9$ $\pm4.8$ 1180
AGUILAR-BENIT..
97B
 
HBC 0.76 ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{\mp}}{{\mathit K}_S^0}$ ${{\mathit \pi}^{\pm}}$
$51.2$ $\pm1.7$
WICKLUND
97
 
ASPK 3,4,6 ${{\mathit K}^{\pm}}$ ${{\mathit N}}$ $\rightarrow$ ( ${{\mathit K}}{{\mathit \pi}}$) ${}^{0}$ ${{\mathit N}}$
$48.9$ $\pm2.5$
BOWLER
97
 
DBC 5.4 ${{\mathit K}^{+}}$ ${{\mathit d}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}{{\mathit p}}$
$48$ ${}^{+3}_{-2}$ 3600
MCCUBBIN
97
 
HBC 3.6 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit n}}$
$50.6$ $\pm2.5$ 22k 5
PALER
97
 
HBC 14.3 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ( ${{\mathit K}}{{\mathit \pi}}$) ${}^{0}$ X
$47$ $\pm2$ 10k
FOX
97
 
RVUE 2 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit n}}$
$51$ $\pm2$
FOX
97
 
RVUE 2 ${{\mathit K}^{+}}$ ${{\mathit n}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
$46.0$ $\pm3.3$ 3186 6
LEWIS
97
 
HBC 2.1$-$2.7 ${{\mathit K}^{+}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}}{{\mathit \pi}}{{\mathit \pi}}{{\mathit p}}$
$51.4$ $\pm5.0$ 1700 6
BUCHNER
97
 
DBC 4.6 ${{\mathit K}^{+}}$ ${{\mathit n}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
$55.8$ ${}^{+4.2}_{-3.4}$ 2934 6
AGUILAR-BENIT..
97B
 
HBC 3.9,4.6 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit n}}$
$48.5$ $\pm2.7$ 5362
AGUILAR-BENIT..
97B
 
HBC 3.9,4.6 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
$54.0$ $\pm3.3$ 4300 6, 7
HABER
97
 
DBC 3 ${{\mathit K}^{-}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}$ X
$53.2$ $\pm2.1$ 10k 6
DAVIS
96
 
HBC 12 ${{\mathit K}^{+}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit p}}$
$44$ $\pm5.5$ 1040 6
DAUBER
96B
 
HBC 2.0 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
• • We do not use the following data for averages, fits, limits, etc. • •
$48.8$ $\pm1.8$ $\pm2.0$ 8
ADUSZKIEWICZ
02A
 
NA61 158 ${{\mathit p}}{{\mathit p}}$
$52.6$ $\pm1.7$ 4k 9
LEES
01C
 
BABR ${{\mathit J / \psi}}$ $\rightarrow$ ${{\mathit K}_S^0}$ ${{\mathit K}^{\pm}}{{\mathit \pi}^{\mp}}$
$44.90$ $\pm0.30$
LEES
01F
 
BABR ${{\mathit D}^{+}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \pi}^{+}}$
$45.7$ $\pm1.1$ $\pm0.5$ 14.4k 10
MITCHELL
00A
 
CLEO ${{\mathit D}_{{{s}}}^{+}}$ $\rightarrow$ ${{\mathit K}^{+}}{{\mathit K}^{-}}{{\mathit \pi}^{+}}$
$50.6$ $\pm0.9$ 20k 11
AUBERT
00AK
 
BABR 10.6 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit K}^{*0}}{{\mathit K}^{\pm}}{{\mathit \pi}^{\mp}}{{\mathit \gamma}}$
1  Taking also into account the ${{\mathit K}^{*}_{\mathrm 0}{(1430)}^{0}}$ and ${{\mathit K}^{*}_{\mathrm 2}{(1430)}^{0}}$.
2  Taking into account the ${{\mathit K}^{*}{(892)}^{0}}$, ${\mathit S}{\mathrm -wave}$ and ${\mathit P}{\mathrm -wave}$ (${{\mathit K}^{*}{(1410)}^{0}}$).
3  From the isobar model with a complex pole for the ${{\mathit \kappa}}$.
4  Fit to ${{\mathit K}}{{\mathit \pi}}$ mass spectrum includes a non-resonant scalar component.
5  Inclusive reaction. Complicated background and phase-space effects.
6  Width errors enlarged by us to 4${\times }\Gamma /\sqrt {\mathit N }$; see note.
7  Number of events in peak reevaluated by us.
8  For transverse momenta between 0.6 and 0.8 GeV/c and rapidity 0 $<$ y $<$ 0.5.
9  From a Dalitz plot analysis in an isobar model with charged and neutral ${{\mathit K}^{*}{(892)}}$ masses and widths floating.
10  This value comes from a fit with $\chi {}^{2}$ of 178/117.
11  Systematic uncertainties not estimated.

           NEUTRAL ONLY (MeV)
References
see fit info