# Nucleon Electromagnetic Form Factors in the Continuum Limit from   2+1+1-flavor Lattice QCD

**Authors:** Yong-Chull Jang, Rajan Gupta, Huey-Wen Lin, Boram Yoon, Tanmoy, Bhattacharya

arXiv: 1906.07217 · 2020-01-29

## TL;DR

This study uses high-statistics lattice QCD simulations to accurately determine nucleon electromagnetic form factors, extrapolating to the continuum limit and analyzing their $Q^2$ dependence with various methods, providing precise radius and magnetic moment estimates.

## Contribution

First comprehensive lattice QCD analysis of nucleon electromagnetic form factors across multiple lattice spacings and quark masses with continuum extrapolation.

## Key findings

- Form factors consistent with experimental data within uncertainties.
- $z$-expansion and dipole form yield compatible radii and magnetic moments.
- Data plotted versus $Q^2/M_N^2$ reduces discretization errors.

## Abstract

Results are presented for the nucleon isovector electromagnetic form factors using 11 ensembles generated by the MILC collaboration using the 2+1+1-flavors HISQ action. They span 4 lattice spacings $a \sim$ 0.06, 0.09, 0.12 and 0.15~fm and 3 values of $M_\pi \sim 135, 225$ and 315 MeV. High-statistics estimates are used to perform a simultaneous extrapolation in the lattice spacing, lattice volume and light-quark masses. The $Q^2$ dependence over the range 0.05-1.4 ${\rm GeV}^2$ is investigated using both the $z$-expansion and the dipole form. Final $z$-expansion estimates for the isovector r.m.s. radius are $r_E = 0.769(27)(30)$ fm $r_M = 0.671(48)(76)$ fm and $\mu^{p-n} = 3.939(86)(138)$ Bohr magneton. The first error is the combined uncertainty from the leading-order analysis, and the second is an estimate of the additional uncertainty due to using the leading order chiral-continuum-finite-volume fits. The dipole estimates, $r_E = 0.765(11)(8)$ fm, $r_M = 0.704(21)(29)$ fm and $\mu^{p-n} = 3.975(84)(125)$, are consistent with those from the $z$-expansion but with smaller errors. Our analysis highlights three points. First, all data from the eleven ensembles and existing lattice data on, or close to, physical mass ensembles from other collaborations collapses more clearly onto a single curve when plotted versus $Q^2/M_N^2$ as compared to $Q^2$ with the scale set by quantities other than $M_N$. The difference between these two analyses is indicative of discretization errors, some of which presumably cancel when the data are plotted versus $Q^2/M_N^2$. Second, the size of the remaining deviation of this common curve from the Kelly curve is small and can be accounted for by statistical and possible systematic uncertainties. Third, to improve lattice estimates, high statistics data for $Q^2 < 0.1$ ${\rm GeV}^2$ are needed.

## Full text

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## Figures

330 figures with captions in the complete paper: https://tomesphere.com/paper/1906.07217/full.md

## References

92 references — full list in the complete paper: https://tomesphere.com/paper/1906.07217/full.md

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Source: https://tomesphere.com/paper/1906.07217