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${{\mathit N}{(1710)}}$ POLE POSITION

$-2{\times }$IMAGINARY PART

INSPIRE   PDGID:

B014IM

VALUE (MeV) DOCUMENT ID TECN  COMMENT $\bf{ 80\text{ to }160\text{ }(\approx120) }$ OUR ESTIMATE $115$ $\pm5$ ROENCHEN 2022 DPWA Multichannel $155$ $\pm25$ ANISOVICH 2017 A DPWA Multichannel $84$ $\pm34$ 1 ANISOVICH 2017 A L+P ${{\mathit \gamma}}{{\mathit p}}$, ${{\mathit \pi}^{-}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit K}}{{\mathit \Lambda}}$ $98$ $\pm8$ $\pm5$ 2 SVARC 2014 L+P ${{\mathit \pi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \pi}}{{\mathit N}}$ $80$ $\pm20$ CUTKOSKY 1980 IPWA ${{\mathit \pi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \pi}}{{\mathit N}}$ • • We do not use the following data for averages, fits, limits, etc. • • $169$ HUNT 2019 DPWA Multichannel $121$ ROENCHEN 2015 A DPWA Multichannel $170$ $\pm20$ SOKHOYAN 2015 A DPWA Multichannel $170$ $\pm20$ GUTZ 2014 DPWA Multichannel $159$ SHKLYAR 2013 DPWA Multichannel $200$ $\pm25$ ANISOVICH 2012 A DPWA Multichannel $174$ $\pm16$ 3 BATINIC 2010 DPWA ${{\mathit \pi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \pi}}$, ${{\mathit N}}{{\mathit \eta}}$ $132$ VRANA 2000 DPWA Multichannel $200$ HOEHLER 1993 SPED ${{\mathit \pi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \pi}}{{\mathit N}}$ $88$ CUTKOSKY 1990 IPWA ${{\mathit \pi}}$ ${{\mathit N}}$ $\rightarrow$ ${{\mathit \pi}}{{\mathit N}}$ 1  Statistical error only. 2  Fit to the amplitudes of HOEHLER 1979. 3  BATINIC 2010 finds evidence for a second ${\mathit P}_{\mathrm 11}$ state with all parameters except for the phase of the pole residue very similar to the parameters we give here.

References

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