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- W2950809315 abstract "We extend recently developed methods used for determining the electromagnetic charge radius and ${a}_{ensuremath{mu}}^{ensuremath{pi}ensuremath{pi}}$ to obtain a determination of the electromagnetic form factor of the pion, ${F}_{ensuremath{pi}}^{V}(t)$, in several significant kinematical regions, using a parametrization-free formalism based on analyticity and unitarity, with the inclusion of precise inputs from both timelike and spacelike regions. On the unitarity cut, below the first inelastic threshold, we use the precisely known phase of the form factor, known from $ensuremath{pi}ensuremath{pi}$ elastic scattering via the Fermi-Watson theorem, and above the inelastic threshold, a conservative integral condition on the modulus. We also use as input the experimental values of the modulus at several energies in the elastic region, where the data from ${e}^{+}{e}^{ensuremath{-}}ensuremath{rightarrow}{ensuremath{pi}}^{+}{ensuremath{pi}}^{ensuremath{-}}$ and $ensuremath{tau}$ hadronic decays are mutually consistent, as well as the most recent measurements at spacelike momenta. The experimental uncertainties are implemented by Monte Carlo simulations. At spacelike values ${Q}^{2}=ensuremath{-}t>0$ near the origin, our predictions are consistent and significantly more precise than the recent QCD lattice calculations. The determinations at larger ${Q}^{2}$ confirm the late onset of perturbative QCD for exclusive quantities. From the predictions of $|{F}_{ensuremath{pi}}^{V}(t){|}^{2}$ on the timelike axis below 0.63 GeV, we obtain the hadronic vacuum polarization (HPV) contribution to the muon anomaly, ${a}_{ensuremath{mu}}^{ensuremath{pi}ensuremath{pi}}{|}_{ensuremath{le}0.63text{ }text{ }mathrm{GeV}}=(132.97ifmmodepmelsetextpmfi{}0.70)ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}10}$, using input from both ${e}^{+}{e}^{ensuremath{-}}$ annihilation and $ensuremath{tau}$ decay, and ${a}_{ensuremath{mu}}^{ensuremath{pi}ensuremath{pi}}{|}_{ensuremath{le}0.63text{ }text{ }mathrm{GeV}}=(132.91ifmmodepmelsetextpmfi{}0.76)ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}10}$ using only ${e}^{+}{e}^{ensuremath{-}}$ input. Our determinations can be readily extended to obtain such contributions in any interval of interest lying between $2{m}_{ensuremath{pi}}$ and 0.63 GeV." @default.
- W2950809315 created "2019-06-27" @default.
- W2950809315 creator A5000080854 @default.
- W2950809315 creator A5013835407 @default.
- W2950809315 creator A5040294120 @default.
- W2950809315 date "2018-12-17" @default.
- W2950809315 modified "2023-09-24" @default.
- W2950809315 title "Pion electromagnetic form factor at high precision with implications to <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msubsup><mml:mi>a</mml:mi><mml:mi>μ</mml:mi><mml:mrow><mml:mi>π</mml:mi><mml:mi>π</mml:mi></mml:mrow></mml:msubsup></mml:math> and the onset of perturbative QCD" @default.
- W2950809315 cites W1484711978 @default.
- W2950809315 cites W1510620661 @default.
- W2950809315 cites W1532872899 @default.
- W2950809315 cites W1547048877 @default.
- W2950809315 cites W1600576976 @default.
- W2950809315 cites W1638111448 @default.
- W2950809315 cites W1651605877 @default.
- W2950809315 cites W1867453671 @default.
- W2950809315 cites W1927035392 @default.
- W2950809315 cites W1970010556 @default.
- W2950809315 cites W1973080198 @default.
- W2950809315 cites W1973441513 @default.
- W2950809315 cites W1974697555 @default.
- W2950809315 cites W1978968729 @default.
- W2950809315 cites W1979081013 @default.
- W2950809315 cites W1980416430 @default.
- W2950809315 cites W1984449794 @default.
- W2950809315 cites W1995164980 @default.
- W2950809315 cites W1997841560 @default.
- W2950809315 cites W1998390781 @default.
- W2950809315 cites W2001000366 @default.
- W2950809315 cites W2002164351 @default.
- W2950809315 cites W2004773248 @default.
- W2950809315 cites W2005909293 @default.
- W2950809315 cites W2014632813 @default.
- W2950809315 cites W2018702222 @default.
- W2950809315 cites W2021542324 @default.
- W2950809315 cites W2021870515 @default.
- W2950809315 cites W2022382755 @default.
- W2950809315 cites W2022667651 @default.
- W2950809315 cites W2026456202 @default.
- W2950809315 cites W2028883660 @default.
- W2950809315 cites W2029915370 @default.
- W2950809315 cites W2029969274 @default.
- W2950809315 cites W2032829857 @default.
- W2950809315 cites W2033198217 @default.
- W2950809315 cites W2035692763 @default.
- W2950809315 cites W2043879367 @default.
- W2950809315 cites W2051436471 @default.
- W2950809315 cites W2052652719 @default.
- W2950809315 cites W2056701546 @default.
- W2950809315 cites W2057962040 @default.
- W2950809315 cites W2058393264 @default.
- W2950809315 cites W2058511210 @default.
- W2950809315 cites W2059048223 @default.
- W2950809315 cites W2066711625 @default.
- W2950809315 cites W2071606511 @default.
- W2950809315 cites W2081122760 @default.
- W2950809315 cites W2081546224 @default.
- W2950809315 cites W2088806215 @default.
- W2950809315 cites W2093708650 @default.
- W2950809315 cites W2094644248 @default.
- W2950809315 cites W2100097417 @default.
- W2950809315 cites W2111511395 @default.
- W2950809315 cites W2116109970 @default.
- W2950809315 cites W2121140421 @default.
- W2950809315 cites W2121160050 @default.
- W2950809315 cites W2123198607 @default.
- W2950809315 cites W2132162721 @default.
- W2950809315 cites W2134179461 @default.
- W2950809315 cites W2134777028 @default.
- W2950809315 cites W2137941090 @default.
- W2950809315 cites W2155763512 @default.
- W2950809315 cites W2157531843 @default.
- W2950809315 cites W2158401454 @default.
- W2950809315 cites W2222790990 @default.
- W2950809315 cites W2321763666 @default.
- W2950809315 cites W2333321650 @default.
- W2950809315 cites W2333954931 @default.
- W2950809315 cites W2345375968 @default.
- W2950809315 cites W2588268857 @default.
- W2950809315 cites W2588986264 @default.
- W2950809315 cites W2598251527 @default.
- W2950809315 cites W2598750649 @default.
- W2950809315 cites W2626597518 @default.
- W2950809315 cites W2765628869 @default.
- W2950809315 cites W2784714858 @default.
- W2950809315 cites W2785694820 @default.
- W2950809315 cites W2899140785 @default.
- W2950809315 cites W2963120226 @default.
- W2950809315 cites W2963276111 @default.
- W2950809315 cites W2987121807 @default.
- W2950809315 cites W3098674065 @default.
- W2950809315 cites W3099464552 @default.
- W2950809315 cites W3103827222 @default.
- W2950809315 cites W3104168600 @default.
- W2950809315 cites W3105147765 @default.
- W2950809315 cites W3105445257 @default.
- W2950809315 cites W3106198992 @default.
- W2950809315 cites W3202860274 @default.
- W2950809315 cites W4232639452 @default.
- W2950809315 doi "https://doi.org/10.1103/physrevd.98.114015" @default.