${{\mathit a}_{{{1}}}{(1260)}}$ MASS

INSPIRE   PDGID:
M010M
VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT
$\bf{ 1230 \pm40}$ OUR ESTIMATE
$1299$ ${}^{+12}_{-28}$ 46M 1
AGHASYAN
2018B
COMP 190 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit p}}$
• • We do not use the following data for averages, fits, limits, etc. • •
$1195.05$ $\pm1.05$ $\pm6.33$ 894k
AAIJ
2018AI
LHCB ${{\mathit D}^{0}}$ $\rightarrow$ ${{\mathit K}^{\mp}}{{\mathit \pi}^{\pm}}{{\mathit \pi}^{\pm}}{{\mathit \pi}^{\mp}}$
$1225$ $\pm9$ $\pm20$ 7k 2
DARGENT
2017
RVUE ${{\mathit D}^{0}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{+}}$
$1255$ $\pm6$ ${}^{+7}_{-17}$ 420k 3
ALEKSEEV
2010
COMP 190 ${{\mathit \pi}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit P}}{{\mathit b}^{\,'}}$
$1243$ $\pm12$ $\pm20$ 4
AUBERT
2007AU
BABR 10.6 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \rho}^{0}}{{\mathit \rho}^{\pm}}{{\mathit \pi}^{\mp}}{{\mathit \gamma}}$
$\text{1230 - 1270}$ 6360 5
LINK
2007A
FOCS ${{\mathit D}^{0}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{+}}$
$1203$ $\pm3$ 6
GOMEZ-DUMM
2004
RVUE ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}_{{{\tau}}}}$
$1330$ $\pm24$ 90k
SALVINI
2004
OBLX ${{\overline{\mathit p}}}$ ${{\mathit p}}$ $\rightarrow$ 2 ${{\mathit \pi}^{+}}$2 ${{\mathit \pi}^{-}}$
$1331$ $\pm10$ $\pm3$ 37k 7
ASNER
2000
CLE2 $10.6$ ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$, ${{\mathit \tau}^{-}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \nu}_{{{\tau}}}}$
$1255$ $\pm7$ $\pm6$ 5904 8
ABREU
1998G
DLPH ${{\mathit e}^{+}}{{\mathit e}^{-}}$
$1207$ $\pm5$ $\pm8$ 5904 9
ABREU
1998G
DLPH ${{\mathit e}^{+}}{{\mathit e}^{-}}$
$1196$ $\pm4$ $\pm5$ 5904 10, 11
ABREU
1998G
DLPH ${{\mathit e}^{+}}{{\mathit e}^{-}}$
$1240$ $\pm10$
BARBERIS
1998B
450 ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit p}_{{{f}}}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}{{\mathit p}_{{{s}}}}$
$1262$ $\pm9$ $\pm7$ 8, 12
ACKERSTAFF
1997R
OPAL ${\it{}E}^{\it{}ee}_{\rm{}cm}$= $88 - 94$, ${{\mathit \tau}}$ $\rightarrow$ 3 ${{\mathit \pi}}{{\mathit \nu}}$
$1210$ $\pm7$ $\pm2$ 9, 12
ACKERSTAFF
1997R
OPAL ${\it{}E}^{\it{}ee}_{\rm{}cm}$= $88 - 94$, ${{\mathit \tau}}$ $\rightarrow$ 3 ${{\mathit \pi}}{{\mathit \nu}}$
$1211$ $\pm7$ ${}^{+50}_{-0}$ 9
ALBRECHT
1993C
ARG ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1121$ $\pm8$ 13
ANDO
1992
SPEC 8 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}{{\mathit n}}$
$1242$ $\pm37$ 14
IVANOV
1991
RVUE ${{\mathit \tau}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1260$ $\pm14$ 15
IVANOV
1991
RVUE ${{\mathit \tau}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1250$ $\pm9$ 16
IVANOV
1991
RVUE ${{\mathit \tau}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1208$ $\pm15$
ARMSTRONG
1990
OMEG 300.0 ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit p}}{{\mathit p}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \pi}^{0}}$
$1220$ $\pm15$ 17
ISGUR
1989
RVUE ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1260$ $\pm25$ 18
BOWLER
1988
RVUE
$1166$ $\pm18$ $\pm11$
BAND
1987
MAC ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1164$ $\pm41$ $\pm23$
BAND
1987
MAC ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{0}}{{\mathit \pi}^{0}}{{\mathit \nu}}$
$1250$ $\pm40$ 17
TORNQVIST
1987
RVUE
$1046$ $\pm11$
ALBRECHT
1986B
ARG ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1056$ $\pm20$ $\pm15$
RUCKSTUHL
1986
DLCO ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1194$ $\pm14$ $\pm10$
SCHMIDKE
1986
MRK2 ${{\mathit \tau}^{+}}$ $\rightarrow$ ${{\mathit \pi}^{+}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit \nu}}$
$1255$ $\pm23$
BELLINI
1985
SPEC 40 ${{\mathit \pi}^{-}}$ ${{\mathit A}}$ $\rightarrow$ ${{\mathit \pi}^{-}}{{\mathit \pi}^{+}}{{\mathit \pi}^{-}}{{\mathit A}}$
$1240$ $\pm80$ 19
DANKOWYCH
1981
SPEC 8.45 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit n}}$3 ${{\mathit \pi}}$
$1280$ $\pm30$ 19
DAUM
1981B
CNTR 63,94 ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit p}}$3 ${{\mathit \pi}}$
$1041$ $\pm13$ 20
GAVILLET
1977
HBC 4.2 ${{\mathit K}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit \Sigma}}$3 ${{\mathit \pi}}$
1  Statistical error negligible.
2  Reanalysis of CLEO data using Breit-Wigner parameterization.
3  Superseded by AGHASYAN 2018B.
4  The ${{\mathit \rho}^{\pm}}{{\mathit \pi}^{\mp}}$ state can be also due to the ${{\mathit \pi}{(1300)}}$.
5  Using the Breit-Wigner parameterization; strong correlation between mass and width.
6  Using the data of BARATE 1998R.
7  From a fit to the 3${{\mathit \pi}}$ mass spectrum including the ${{\mathit K}}{{\overline{\mathit K}}^{*}{(892)}}$ threshold.
8  Uses the model of KUHN 1990.
9  Uses the model of ISGUR 1989.
10  Includes the effect of a possible ${{\mathit a}_{{{1}}}^{\,'}}$ state.
11  Uses the model of FEINDT 1990.
12  Supersedes AKERS 1995P.
13  Average and spread of values using 2 variants of the model of BOWLER 1975.
14  Reanalysis of RUCKSTUHL 1986.
15  Reanalysis of SCHMIDKE 1986.
16  Reanalysis of ALBRECHT 1986B.
17  From a combined reanalysis of ALBRECHT 1986B, SCHMIDKE 1986, and RUCKSTUHL 1986.
18  From a combined reanalysis of ALBRECHT 1986B and DAUM 1981B.
19  Uses the model of BOWLER 1975.
20  Produced in ${{\mathit K}^{-}}$ backward scattering.
References