$\bf{
-0.11958 \pm0.00021}$
|
OUR AVERAGE
Error includes scale factor of 1.2.
|
$-0.11985$ $\pm0.00017$ $\pm0.00012$ |
1 |
|
SPEC |
$-0.12015$ $\pm0.00034$ $\pm0.00063$ |
2 |
|
UCNA |
$-0.11926$ $\pm0.00031$ ${}^{+0.00036}_{-0.00042}$ |
3 |
|
SPEC |
$-0.1160$ $\pm0.0009$ $\pm0.0012$ |
|
|
TPC |
$-0.1135$ $\pm0.0014$ |
4 |
|
CNTR |
$-0.1146$ $\pm0.0019$ |
|
|
SPEC |
• • • We do not use the following data for averages, fits, limits, etc. • • • |
$-0.11972$ $\pm0.00025$ |
5 |
|
SPEC |
$-0.11952$ $\pm0.00110$ |
6 |
|
UCNA |
$-0.11966$ $\pm0.00089$ ${}^{+0.00123}_{-0.00140}$ |
7 |
|
UCNA |
$-0.11966$ $\pm0.00089$ ${}^{+0.00123}_{-0.00140}$ |
|
|
UCNA |
$-0.1138$ $\pm0.0046$ $\pm0.0021$ |
|
|
SPEC |
$-0.1189$ $\pm0.0007$ |
8 |
|
SPEC |
$-0.1168$ $\pm0.0017$ |
9 |
|
CNTR |
$-0.1189$ $\pm0.0012$ |
|
|
SPEC |
$-0.1160$ $\pm0.0009$ $\pm0.0011$ |
|
|
TPC |
$-0.1116$ $\pm0.0014$ |
|
|
CNTR |
$-0.114$ $\pm0.005$ |
10 |
|
CNTR |
$-0.113$ $\pm0.006$ |
10 |
|
CNTR |
1
MAERKISCH 2019 further derive a value for the CKM-element $\vert {{\mathit V}_{{{ud}}}}\vert $ = $0.97351$ $\pm0.00060$, using ${\mathit \tau}_{{{\mathit n}}}$ = 879.7(8) sec and the relation from CZARNECKI 2018.
|
2
BROWN 2018 gets $\mathit A$ = $-0.12054$ $\pm0.00044$ $\pm0.00068$ and $\lambda $ = $-1.2783$ $\pm0.0022$. We quote the combined values that include the earlier UCNA measurements (MENDENHALL 2013).
|
3
This MUND 2013 value includes earlier PERKEO II measurements (ABELE 2002 and ABELE 1997D), with a correction to those results.
|
4
YEROZOLIMSKY 1997 makes a correction to the EROZOLIMSKII 1991 value.
|
5
Under the SM assumption that the Fierz term ${{\mathit b}}$ = 0, SAUL 2020 obtain the quoted asymmetry parameter ${{\mathit A}}$ and $\lambda $ = $-1.27607$ $\pm0.00068$. In a combined fit authors extract the values ${{\mathit A}}$ = $-0.1209$ $\pm0.0015$, $\lambda $ = $-1.2792$ $\pm0.0060$, and ${{\mathit b}}$ = $0.017$ $\pm0.021$.
|
6
MENDENHALL 2013 gets $\mathit A$ = $-0.11954$ $\pm0.00055$ $\pm0.00098$ and $\lambda $ = $-1.2756$ $\pm0.0030$. We quote the nearly identical values that include the earlier UCNA measurement (PLASTER 2012), with a correction to that result.
|
7
This PLASTER 2012 value is identical with that given in LIU 2010, but the experiment is now described in detail.
|
8
This is the combined result of ABELE 2002 and ABELE 1997D.
|
9
MOSTOVOI 2001 calculates this from its measurement of $\lambda =\mathit g_{\mathit A}/\mathit g_{\mathit V}$ above.
|
10
These results are not corrected for radiative effects and weak magnetism, but the corrections are small compared to the errors.
|