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Nucleon Tomography and Generalized Parton Distribution at Physical Pion Mass from Lattice QCD

Huey-Wen Lin [email protected] Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 Department of Computational Mathematics, Science and Engineering, Michigan State University, East Lansing, MI 48824
Abstract

We present the first lattice calculation of the nucleon isovector unpolarized generalized parton distribution (GPD) at the physical pion mass using a lattice ensemble with 2+1+1 flavors of highly improved staggered quarks (HISQ) generated by MILC Collaboration, with lattice spacing a0.09a\approx 0.09 fm and volume 643×9664^{3}\times 96. We use momentum-smeared sources to improve the signal at nucleon boost momentum Pz2.2P_{z}\approx 2.2 GeV, and report results at nonzero momentum transfers in [0.2,1.0] GeV2[0.2,1.0]\text{ GeV}^{2}. Nonperturbative renormalization in RI/MOM scheme is used to obtain the quasi-distribution before matching to the lightcone GPDs. The three-dimensional distributions H(x,Q2)H(x,Q^{2}) and E(x,Q2)E(x,Q^{2}) at ξ=0\xi=0 are presented, along with the three-dimensional nucleon tomography and impact-parameter–dependent distribution for selected Bjorken xx at μ=3\mu=3 GeV in MS¯\overline{\text{MS}} scheme.

pacs:
12.38.-t, 11.15.Ha, 12.38.Gc
preprint: MSUHEP-20-014

Nucleons (that is, protons and neutrons) are the building blocks of all ordinary matter, and the study of nucleon structure is a central goal of many worldwide experimental efforts. Gluons and quarks are the underlying degrees of freedom that explain the properties of nucleons, and fully understanding how they contribute to the properties of nucleons (such as their mass or spin structure) helps to decode the Standard Model. In quantum chromodynamics (QCD), gluons strongly interact with themselves and with quarks, binding both nucleons and nuclei. However, due to their confinement within these bound states, we cannot single out individual constituents to study them. More than half a century since the discovery of nucleon structure, our understanding has improved greatly; however, there is still a long way to go in unveiling the nucleon’s detailed structure, which is characterized by functions such as the generalized parton distributions (GPDs) Müller et al. (1994); Ji (1997a); Radyushkin (1996). GPDs can be viewed as a hybrid of parton distributions (PDFs), form factors and distribution amplitudes. They play an important role in providing a three-dimensional spatial picture of the nucleon Burkardt (2000) and in revealing its spin structure Ji (1997a). Experimentally, GPDs can be accessed in exclusive processes such as deeply virtual Compton scattering Ji (1997b) or meson production Kriesten et al. (2020). Experimental collaborations and facilities worldwide have been devoted to searching for these last unknowns of the nucleon, including HERMES at DESY, COMPASS at CERN, GSI in Europe, BELLE and JPAC in Japan, Halls A, B and C at Jefferson Laboratory, and PHENIX and STAR at RHIC at Brookhaven National Laboratory in the US. There are also plans for future facilities: a US electron-ion collider (EIC) National Academies of Sciences and Medicine (2018) at Brookhaven National Laboratory, an EIC in China (EicC) Chen (2018); Chen et al. (2020), and the Large Hadron-Electron Collider (LHeC) in Europe Abelleira Fernandez et al. (2012); Agostini et al. (2020).

Although interest in GPDs has grown enormously, we still need fresh theoretical and phenomenological ideas, including reliable model-independent techniques. Most QCD models have issues associated with three-dimensional structure that are not yet fully understood, so a reliable framework for extracting three-dimensional parton distributions and fragmentation functions from experimental observables does not yet exist. Theoretically, there are factorization issues in hadron production from hadronic reactions, and theoretical efforts are striving to answer key questions that lie along the path to a precise mapping of three-dimensional nucleon structure from experiment. It has become common understanding that we need to develop a program in both theory and experiment that will allow an accurate flavor decomposition of the nucleon GPDs, including flavor differences in the quark structure, the gluon structure and the nucleon sea-quark GPDs. Most current theoretical issues are associated with nonperturbative features of QCD, that is, where the strong coupling is too large for analytic perturbative methods to be valid. Using a nonperturbative theoretical method that starts from the quark and gluon degrees of freedom, lattice QCD (LQCD), allows us to compute these properties on supercomputers.

Probing hadron structure with lattice QCD was for many years limited to the first few moments, due to complications arising from the breaking of rotational symmetry by the discretized Euclidean spacetime. The breakthrough for LQCD came in 2013, when a technique was proposed to connect quantities calculable on the lattice to those on the lightcone. Large-momentum effective theory (LaMET), also known as the “quasi-PDF method” Ji (2013, 2014); Ji et al. (2017), allows us to calculate the full Bjorken-xx dependence of distributions for the first time. Much progress has been made since the first LaMET paper  Lin (2014a); Lin et al. (2015); Chen et al. (2016); Lin et al. (2018a); Alexandrou et al. (2015, 2017a, 2017b); Chen et al. (2018a); Alexandrou et al. (2018a); Chen et al. (2018b); Zhang et al. (2019a); Alexandrou et al. (2018b); Lin et al. (2018b); Fan et al. (2018); Liu et al. (2018a); Wang et al. (2019); Lin and Zhang (2019); Chen et al. (2019); Xiong et al. (2014); Ji and Zhang (2015); Ji et al. (2015a); Xiong and Zhang (2015); Ji et al. (2015b); Lin (2014b); Monahan (2018); Ji et al. (2018a); Stewart and Zhao (2018); Constantinou and Panagopoulos (2017); Green et al. (2018); Izubuchi et al. (2018); Xiong et al. (2017); Wang et al. (2018); Wang and Zhao (2018); Xu et al. (2018a); Zhang et al. (2017); Ishikawa et al. (2016); Chen et al. (2017); Ji et al. (2018b); Ishikawa et al. (2017, 2019); Li (2016); Monahan and Orginos (2017); Radyushkin (2017a); Rossi and Testa (2017); Carlson and Freid (2017); Ji et al. (2017); Briceño et al. (2018); Hobbs (2018); Jia et al. (2017); Xu et al. (2018b); Jia et al. (2018); Spanoudes and Panagopoulos (2018); Rossi and Testa (2018); Liu et al. (2018b); Ji et al. (2019a); Bhattacharya et al. (2019); Radyushkin (2019); Zhang et al. (2019b); Li et al. (2019); Braun et al. (2019); Detmold et al. (2019); Ebert et al. (2020a); Ji et al. (2019b); Bali et al. (2018a, b); Sufian et al. (2019); Bali et al. (2019a); Orginos et al. (2017); Karpie et al. (2018a, b, 2019); Joó et al. (2019a, b); Radyushkin (2018); Zhang et al. (2018); Lin et al. (2020); Zhang et al. (2020a); Fan et al. (2020a); Sufian et al. (2020); Shugert et al. (2020); Green et al. (2020); Chai et al. (2020); Shanahan et al. (2020); Braun et al. (2020); Bhattacharya et al. (2020); Ji et al. (2020a); Ebert et al. (2020b); Lin (2020a); Joó et al. (2020); Bhat et al. (2020); Fan et al. (2020b). Most work has been done using only one lattice ensemble, but there has been some progress in determining the size of lattice systematic uncertainties. For example, finite-volume systematics were studied in Refs. Joó et al. (2019b); Lin and Zhang (2019). Machine-learning algorithms have been applied to the inverse problem Karpie et al. (2019); Zhang et al. (2020b) and to making predictions for larger boost momentum and larger Wilson-displacement Zhang et al. (2020c). On the lattice discretization errors, a Nf=2+1+1N_{f}=2+1+1 superfine (a0.042a\approx 0.042 fm) lattice at 310-MeV pion mass was used to study nucleon PDFs in Ref. Fan et al. (2020a), and results using multiple lattice spacings were reported in Refs. Zhang et al. (2020b); Lin et al. (2020); Sufian et al. (2020). The first attempt to obtain strange and charm distributions of the nucleon was recently reported Zhang et al. (2020a). However, beyond one-dimensional hadron structure, there is little work available. Last spring, the first lattice study of GPDs was made for pions Chen et al. (2019). During the completion of this work, ETM Collaboration reported their findings on both unpolarized and polarized nucleon GPDs with largest boost momentum 1.67 GeV at pion mass Mπ260M_{\pi}\approx 260 MeV Alexandrou et al. (2019a, 2020a). In this work, we present the first lattice-QCD calculation of the nucleon GPD at the physical pion mass using the LaMET method and study the three-dimensional structure of the unpolarized nucleon GPDs.

The unpolarized GPDs H(x,ξ,t)H(x,\xi,t) and E(x,ξ,t)E(x,\xi,t) are defined in terms of the matrix elements

F(x,ξ,t)\displaystyle F(x,\xi,t) =dz4πeixp+zp′′|ψ¯(z2)γ+L(z2,z2)ψ(z2)|pz+=0,z=0\displaystyle=\int\frac{dz^{-}}{4\pi}e^{ixp^{+}z^{-}}\left\langle p^{\prime\prime}\left|\bar{\psi}\left(-\frac{z}{2}\right)\gamma^{+}L\left(-\frac{z}{2},\frac{z}{2}\right)\psi\left(\frac{z}{2}\right)\right|p^{\prime}\right\rangle_{z^{+}=0,\vec{z}_{\perp}=0}
=12p+[H(x,ξ,t)u¯(p′′)γ+u(p)+E(x,ξ,t)u¯(p′′)iσ+νΔν2mu(p)],\displaystyle=\frac{1}{2p^{+}}\left[H(x,\xi,t)\bar{u}(p^{\prime\prime})\gamma^{+}u(p^{\prime})+E(x,\xi,t)\bar{u}(p^{\prime\prime})\frac{i\sigma^{+\nu}\Delta_{\nu}}{2m}u(p^{\prime})\right], (1)

where L(z/2,z/2)L(-z/2,z/2) is the gauge link along the lightcone and

Δμ=p′′μpμ,t=Δ2,ξ=p′′+p+p′′++p+.\Delta^{\mu}=p^{\prime\prime\mu}-p^{\prime\mu},\qquad t=\Delta^{2},\qquad\xi=\frac{p^{\prime\prime+}-p^{\prime+}}{p^{\prime\prime+}+p^{\prime+}}. (2)

In the limit ξ,t0\xi,t\to 0, HH reduces to the usual unpolarized parton distributions while the information encoded in EE cannot be accessed, since they are multiplied by the four-momentum transfer Δ\Delta. Only in exclusive processes with a nonzero momentum transfer can EE be probed. The one-loop matching Ji et al. (2015a); Liu et al. (2019) for the GPD HH and EE turns out to be similar to that for the parton distribution.

In this work, we focus on the nucleon isovector unpolarized GPDs and their quasi-GPD counterparts defined in terms of spacelike correlations calculated in Breit frame. We use clover valence fermions on an ensemble with lattice spacing a0.09a\approx 0.09 fm, spatial (temporal) extent around 5.8 (8.6) fm, and with the physical pion mass Mπ135M_{\pi}\approx 135 MeV and Nf=2+1+1N_{f}=2+1+1 (degenerate up/down, strange and charm) flavors of highly improved staggered dynamical quarks (HISQ) Follana et al. (2007) generated by MILC Collaboration Bazavov et al. (2013). The gauge links are one-step hypercubic (HYP) smeared Hasenfratz and Knechtli (2001) to suppress discretization effects. The clover parameters are tuned to recover the lowest sea pion mass of the HISQ quarks. The “mixed-action” approach is commonly used, and there has been promising agreement between the calculated lattice nucleon charges, moments and form factors and the experimental data when applicable Mondal et al. (2020); Jang et al. (2020); Gupta et al. (2018a); Lin et al. (2018c); Gupta et al. (2018b, 2017); Yoon et al. (2017); Bhattacharya et al. (2016, 2015, 2014); Briceno et al. (2012); Bhattacharya et al. (2012); Lin (2020b). Gaussian momentum smearing Bali et al. (2016) is used on the quark field to improve the overlap with ground-state nucleons of the desired boost momentum, allowing us to reach higher boost momentum for the nucleon states. We calculate the matrix elements of the form Pf|ψ¯(z2)ΓL(z2,z2)ψ(z2)|Pi\left\langle P_{f}\left|\bar{\psi}\left(-\frac{z}{2}\right)\Gamma L\left(-\frac{z}{2},\frac{z}{2}\right)\psi\left(\frac{z}{2}\right)\right|P_{i}\right\rangle with projection operators 1+γt2(1+iγ5γx,y,z)\frac{1+\gamma_{t}}{2}(1+i\gamma_{5}\gamma_{x,y,z}). We also use high-statistics measurements, 501,760 total over 1960 configurations, to drive down the increased statistical noise at high boost momenta, Pz=|Pi+Pf2|=|2πL{0,0,10}a1|P_{z}=|\frac{\vec{P_{i}}+\vec{P_{f}}}{2}|=|\frac{2\pi}{L}\{0,0,10\}a^{-1}|, and vary spatial momentum transfer q=PfPi=2πL{nx,ny,0}a1\vec{q}=\vec{P_{f}}-\vec{P_{i}}=\frac{2\pi}{L}\{n_{x},n_{y},0\}a^{-1} with integer nx,yn_{x,y} and nx2+ny2{0,4,8,16,20}n_{x}^{2}+n_{y}^{2}\in\{0,4,8,16,20\} with four-momentum transfer squared Q2=qμqμ={0,0.19,0.39,0.77,0.97}Q^{2}=-q_{\mu}q^{\mu}=\{{0,0.19,0.39,0.77,0.97}\} GeV2. We solve a set of linear equations to obtain HH and EE (similar to form-factor extraction) with all |q||q| at fixed Q2Q^{2}. Technical details (such as renormalization) and more information on how the matrix elements are extracted can be found in the supplement and our previous work Yoon et al. (2016); Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a).

The nonperturbatively renormalized matrix elements are then Fourier transformed into quasi-GPDs through two different approaches. Following the recent work Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a), we take the matrix elements z[12,12]z\in[-12,12] and apply the simple but effective “derivative” method, Q~=izmax+zmax𝑑zeixPzzh~R/x\tilde{Q}=i\int_{-z_{\text{max}}}^{+z_{\text{max}}}\!\!dz\,e^{ixP_{z}z}\tilde{h}^{\prime}_{R}/x, to obtain the quasi-GPDs. Alternatively, we adopt the extrapolation formulation suggested by Ref. Ji et al. (2020b) by fitting |z|{10,15}|z|\in\{10,15\} using the formula c1(izPz)d1+c2eizPz(izPz)d2c_{1}(-izP_{z})^{-d_{1}}+c_{2}e^{izP_{z}}(izP_{z})^{-d_{2}}, inspired by the Regge behavior, to extrapolate the matrix elements into the region beyond the lattice calculation and suppress Fourier-transformation artifacts. Then, both quasi-GPDs are matched to the physical GPDs by applying the matching condition Stewart and Zhao (2018); Liu et al. (2018b); Chen et al. (2018b); Lin et al. (2018b). Examples of the GPDs at momentum transfer Q20.4 GeV2Q^{2}\approx 0.4\text{ GeV}^{2} are shown in Fig. 1. Figure 1 compares the HH and EE GPDs at Q20.4 GeV2Q^{2}\approx 0.4\text{ GeV}^{2} with the quasi-distribution and matched distribution using Pz2.2P_{z}\approx 2.2 GeV. The matching lowers the positive mid-xx to large-xx distribution, as expected; as one approaches lightcone limit, the probability of a parton carrying a larger fraction of its parent nucleon’s momentum should become smaller. We also find that the derivative and Regge-inspired extrapolation agree in the mid- to large-xx regions, but their difference grows as xx approaches zero in both the quark and antiquark distribution. This is expected, since they differ mainly in the treatment of the large-zz matrix elements in the quasi-GPD Fourier transformation, which contributes more significantly to the small-xx distribution. By repeating a similar analysis for each available Q2Q^{2} in this calculation, we can construct the full three-dimensional shape of HH and EE as functions of xx and Q2Q^{2}, as shown in Fig. 2. Due to the limited reliable zPzzP_{z} reach of the lattice calculation, we find that the small-xx region is unreliable, due to lack of precision lattice data to constrain it. Thus, due to charge conservation, the antiquark (negative-xx) distribution can also be sensitive to PzP_{z}. It has been found in past work Lin et al. (2018a); Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a) that higher boost momenta are needed to improve the antiquark region. Therefore, for the rest of the work, we will mainly focus on the x>0.05x>0.05 region. For convenience, we will focus on showing the GPD results from derivative method, and use the Regge-inspired extrapolation to estimate the uncertainties in the small-xx region by reconstructing GPD moments from our xx-dependent GPD functions.

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Figure 1: Nucleon isovector HH and EE quasi-GPDs and matched GPDs at momentum transfer Q2=0.39 GeV2Q^{2}=0.39\text{ GeV}^{2}. The orange and green bands are the quasi-GPD and matched GPDs from derivative method Lin et al. (2018a), while the pink band corresponds to the matched GPD using quasi-GPD from the extrapolation formulation suggested by Ref. Ji et al. (2020b). We find both methods give reasonable agreement in the xx-dependent behavior, except in the small-xx region, which is dominated by the large-zz matrix elements that rely on the extrapolation.
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Figure 2: Nucleon isovector HH and EE GPDs at ξ=0\xi=0 as functions of xx and momentum transfer Q2Q^{2}.

Since this is the first lattice calculation with full three-dimensional xx and Q2Q^{2} dependence of the HH and EE GPD functions, we would like to check how the new results using LaMET approach compare with the previous moment approaches to the generalized form factors. In the ξ0\xi\to 0 limit, the HH and EE GPDs decrease monotonically as xx or Q2Q^{2} increases. We take Mellin moments of the GPDs to compare with previous lattice calculations done using local matrix elements through the operator product expansion (OPE). Taking the xx-moments of HH and EE Ji (1998); Hagler (2010):

1+1𝑑xxn1H(x,ξ,Q2)\displaystyle\int_{-1}^{+1}\!\!dx\,x^{n-1}\,H(x,\xi,Q^{2}) =\displaystyle=
i=0, evenn1(2ξ)iAni(Q2)\displaystyle\sum\limits_{i=0,\text{ even}}^{n-1}(-2\xi)^{i}A_{ni}(Q^{2}) +(2ξ)nCn0(Q2)|n even,\displaystyle+(-2\xi)^{n}\,C_{n0}(Q^{2})|_{n\text{ even}}, (3a)
1+1𝑑xxn1E(x,ξ,Q2)\displaystyle\int_{-1}^{+1}\!\!dx\,x^{n-1}\,E(x,\xi,Q^{2}) =\displaystyle=
i=0, evenn1(2ξ)iBni(Q2)\displaystyle\sum\limits_{i=0,\text{ even}}^{n-1}(-2\xi)^{i}B_{ni}(Q^{2}) (2ξ)nCn0(Q2)|n even,\displaystyle-(-2\xi)^{n}\,C_{n0}(Q^{2})|_{n\text{ even}}\,, (3b)

where the generalized form factors (GFFs) Ani(Q2)A_{ni}(Q^{2}), Bni(Q2)B_{ni}(Q^{2}) and Cni(Q2)C_{ni}(Q^{2}) in the ξ\xi-expansion on the right-hand side are real functions. When n=1n=1, we get the Dirac and Pauli electromagnetic form factors F1(Q2)=A10(Q2)F_{1}(Q^{2})=A_{10}(Q^{2}) and F2(Q2)=B10(Q2)F_{2}(Q^{2})=B_{10}(Q^{2}). To compare with other lattice results, we plot the Sachs electric and magnetic form factors using F1,2F_{1,2} as GE(Q2)=F1(Q2)+q2F2(Q2)/(2MN)2G_{E}(Q^{2})=F_{1}(Q^{2})+q^{2}F_{2}(Q^{2})/(2M_{N})^{2} and GM(Q2)=F1(Q2)+F2(Q2)G_{M}(Q^{2})=F_{1}(Q^{2})+F_{2}(Q^{2}) in Fig. 3 with selected results from near-physical pion masses. PACS has the largest volume among these calculations and is able to probe the smallest Q2Q^{2}. Overall, our results are not only consistent within errors with the earlier PNDME study using the same ensemble (but which used local operators) but are also in good agreement with other lattice collaborations. When n=2n=2, we obtained GFFs of A20(Q2)A_{20}(Q^{2}) and B20(Q2)B_{20}(Q^{2}) so that we can compare our moment results with past lattice calculations using the OPE, as shown in Fig. 3. We compare our moment results with those obtained from simulations at the physical point by ETMC using three ensembles Alexandrou et al. (2020b) and the near-physical calculation of RQCD Bali et al. (2019b). We note that even with the same OPE approach by the same collaboration, the two data sets for A20A_{20} in the ETMC calculation exhibit some tension. This is an indication that the systematic uncertainties are more complicated for these GFFs. Given that the blue points correspond to finer lattice spacing, larger volume and larger mπLm_{\pi}L, we expect that the blue points have suppressed systematic uncertainties. Our moment result A20(Q2)A_{20}(Q^{2}) is in better agreement with those obtained using the OPE approach at small momentum transfer Q2Q^{2}, while B20(Q2)B_{20}(Q^{2}) is in better agreement with OPE approaches at large Q2Q^{2}. The comparison between the Nf=2N_{f}=2 ETMC data and Nf=2N_{f}=2 RQCD data reveals agreement for A20A_{20} and B20B_{20}. However, the RQCD data have a different slope than the ETMC data, which is attributed to the different analysis methods and systematic uncertainties. Both our results and ETMC’s are done using a single ensemble; future studies to include other lattice artifacts, such as lattice-spacing dependence, are important to account for the difference in the results.

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Figure 3: (top) The nucleon isovector electric and magnetic form factor results obtained from this work (labeled as “MSULat20 2+1+1”) as functions of transferred momentum Q2Q^{2}, and comparison with other lattice works calculated near physical pion mass: Nf=2N_{f}=2 ETMC18 Alexandrou et al. (2017c) Nf=2+1N_{f}=2+1 LHPC14 Green et al. (2014), LHPC17 Hasan et al. (2018), PACS18 Shintani et al. (2019); Nf=2+1+1N_{f}=2+1+1 ETMC18 Alexandrou et al. (2019b), PNDME19 Jang et al. (2018) with 2 lattice spacings of 0.06 and 0.09 fm. (bottom) The unpolarized nucleon isovector GFFs obtained from this work, compared with other lattice results calculated near physical pion mass as functions of transfer momentum Q2Q^{2}: ETMC19 Alexandrou et al. (2020b), and RQCD19 Bali et al. (2019b).

Note that the error bands in Fig. 3 include the systematics from the following: 1) The systematics due to the negative- and small-xx regions of the current GPD extraction. We create pseudo-lattice data using input of CT18NNLO PDF Hou et al. (2019) with the same lattice parameters (such as zz and PzP_{z}) used in this calculation and apply the same analysis procedure described above. We take the upper limit of the reconstructed and original CT18 moments as an estimate of the systematics introduced by the analysis procedure (e.g. by Fourier truncation); 2) We vary the maximum Wilson-line length zz within 2 lattice units and take half the difference as an estimate of the systematic due to finite zz; 3) We estimate 1/Pz1/P_{z} systematics due to higher-twist effects by comparing our Q2=0Q^{2}=0 PDFs and to those in the previous works with 3 boost momenta Chen et al. (2018b); Lin et al. (2018b). The final errors are summed in quadrature to create the final error bands shown in Fig. 3.

The Fourier transform of the non–spin-flip GPD H(x,ξ=0,Q2)H(x,\xi=0,Q^{2}) gives the impact-parameter–dependent distribution 𝗊(x,b)\mathsf{q}(x,b) Burkardt (2003)

𝗊(x,b)=d𝐪(2π)2H(x,ξ=0,t=𝐪2)ei𝐪𝐛,\mathsf{q}(x,b)=\int\frac{d\mathbf{q}}{(2\pi)^{2}}H(x,\xi=0,t=-\mathbf{q}^{2})e^{i\mathbf{q}\,\cdot\,\mathbf{b}}, (4)

where bb is the transverse distance from the center of momentum. Figure 4 shows the first results of impact-parameter–dependent distribution from lattice QCD: a three-dimensional distribution as function of xx and bb, and two-dimensional distributions at x=0.3x=0.3, 0.5 and 0.7. The impact-parameter–dependent distribution describes the probability density for a parton with momentum fraction xx at distance bb in the transverse plane. Figure 4 shows that the probability decreases quickly as xx increases. Using Eq. 4 and the H(x,ξ=0,t=𝐪2)H(x,\xi=0,t=-\mathbf{q}^{2}) obtained from the lattice calculation at the physical pion mass, we can take a snapshot of the nucleon in the transverse plane to perform xx-dependent nucleon tomography using lattice QCD for the first time.

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Figure 4: (Left) Nucleon tomography: three-dimensional impact parameter–dependent parton distribution as a function of xx and bb using lattice HH at physical pion mass. (Right) The two-dimensional impact-parameter–dependent distribution for x=0.3x=0.3, 0.5 and 0.7.

In this work, we compute the isovector nucleon unpolarized GPDs at physical pion mass using boost momentum 2.22.2 GeV with nonzero momentum transfers in [0.2,1.0] GeV2[0.2,1.0]\text{ GeV}^{2}. We are able to map out the first three-dimensional GPD structures using lattice QCD in the special limit ξ=0\xi=0. There are residual lattice systematics are not yet included in the current calculation: In our past studies, we found the finite-volume effects to be negligible for isovector nucleon quasi-distributions calculated within the range MπvalL{3.3,5.5}M_{\pi}^{\text{val}}L\in\{3.3,5.5\}. We anticipate such systematics should be small compared to the statistical errors. The lattice discretization has been studied by MSULat collaboration in Refs. Zhang et al. (2020b); Lin et al. (2020) with multiple lattice spacings in the LaMET study of pion and kaon distribution amplitudes and PDFs; similarly, a comparison of nucleon isovector PDFs with 0.045 and 0.12 fm lattice spacing is shown in supplementary materials. There was mild lattice-spacing dependence for a majority of the Wilson-link displacements studied with similar largest boost momenta with same valence/sea lattice setup. EMTC also report LaMET isovector nucleon PDFs in Ref. Alexandrou et al. (2020c) using twisted-mass fermion actions and reports different findings. Future work will investigate ensembles with smaller lattice spacing to reach even higher boost momentum (either directly or with the aid of machine learning Zhang et al. (2020c)) so that we can push toward reliable determination of the smaller-xx and antiquark regions.

Acknowledgements.
We thank the MILC Collaboration for sharing the lattices used to perform this study. The LQCD calculations were performed using the Chroma software suite Edwards and Joo (2005). This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 through ERCAP; facilities of the USQCD Collaboration, which are funded by the Office of Science of the U.S. Department of Energy, and supported in part by Michigan State University through computational resources provided by the Institute for Cyber-Enabled Research (iCER). The work of HL is partially supported by the US National Science Foundation under grant PHY 1653405 “CAREER: Constraining Parton Distribution Functions for New-Physics Searches” and by the Research Corporation for Science Advancement through the Cottrell Scholar Award “Unveiling the Three-Dimensional Structure of Nucleons”.

References

Supplemental materials

Details of the lattice calculations

In the LaMET (or “quasi-PDF”) approach, we calculate time-independent spatially displaced matrix elements that can be connected to the parton distributions. The operator choice is not unique at finite nucleon momentum; a convenient choice for leading-twist PDFs is to take the average of the hadron momentum (0,0,Pz)(0,0,P_{z}) and the quark-antiquark separation to be along the zz direction

hΓ(z,Pz)=N(Pf,s)|ψ¯(λz^)W(λz^,0)Γψ(0)|N(Pi,s)),h_{\Gamma}(z,P_{z})=\langle N(P_{f},s^{\prime})\left|\bar{\psi}(\lambda\hat{z})W(\lambda\hat{z},0)\Gamma\psi(0)\right|N(P_{i},s))\rangle, (5)

where |N(Pi,f)|N(P_{i,f})\rangle denotes a nucleon state with momenta Piμ=(Ei,qx/2,qy/2,Pz)P_{i}^{\mu}=(E_{i},-q_{x}/2,-q_{y}/2,P_{z}) and Pfμ=(Ef,qx/2,qy/2,Pz)P_{f}^{\mu}=(E_{f},q_{x}/2,q_{y}/2,P_{z}), ψ\psi (ψ¯\bar{\psi}) are the (anti-)quark fields, nμn^{\mu} is a unit vector and W(λz^,0)W(\lambda\hat{z},0) is the Wilson link along the zz direction. See Fig. 5 for an illustration. There are multiple choices of operator in this framework that will recover the same lightcone PDFs when the large-momentum limit is taken. For example, Γ\Gamma can be γz\gamma_{z} or γt\gamma_{t} Xiong et al. (2014); Radyushkin (2017a, b); Orginos et al. (2017); both will give the unpolarized PDFs in the infinite-momentum frame. In this work, we use Γ=γt\Gamma=\gamma_{t} for the unpolarized GPDs calculations. Since the systematics of the LaMET methods, such as the higher-twist effects at O(ΛQCD2Pz2)O\left(\frac{\Lambda_{\text{QCD}}^{2}}{P_{z}^{2}}\right), decrease as the momentum increases, we use Pz2.2P_{z}\approx 2.2 GeV in this calculation. (A study of the PzP_{z} convergence of the LaMET approach on the same ensembles can be found in Refs. Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a).) This also allows us to reach smaller-xx regions of the GPDs functions.

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Figure 5: Illustration of the lattice matrix-element calculation on top of the QCD vacuum.

We use Gaussian momentum smearing Bali et al. (2016) ψ(x)+αjUj(x)eike^jψ(x+e^j)\psi(x)+\alpha\sum_{j}U_{j}(x)e^{ik\hat{e}_{j}}\psi(x+\hat{e}_{j}), where kk is the input momentum-smearing parameter, Uj(x)U_{j}(x) are the gauge links in the jj direction, and α\alpha is a tunable parameter as in traditional Gaussian smearing. We vary the α\alpha values in this study so that we can have multiple ways of removing the excited-state contributions from matrix elements later on. To better extract the boosted-momentum ground-state nucleon, we apply the variational method Luscher and Wolff (1990) to extract the principal correlators corresponding to pure energy eigenstates from a matrix of correlators. We use a 3×33\times 3 smeared-smeared two-point correlation matrix, which can be decomposed as

C2ptij(t)=n=0vnivnjetEnC^{ij}_{\text{2pt}}(t)=\sum_{n=0}v^{i}_{n*}v^{j}_{n}e^{-tE_{n}} (6)

with eigenvalues λn(t,tr)=e(ttr)En\lambda_{n}(t,t_{r})=e^{-(t-t_{r})E_{n}} by solving the generalized eigensystem problem C2ptij(t)V=λ(t,tr)C2ptij(tr)VC^{ij}_{\text{2pt}}(t)V=\lambda(t,t_{r})C^{ij}_{\text{2pt}}(t_{r})V, where VV is the matrix of eigenvectors and trt_{r} is a reference time slice. The resulting 3 eigenvalues (principal correlators) λn(t,tr)\lambda_{n}(t,t_{r}) are then further analyzed to extract the energy levels EnE_{n}. Since they have been projected onto pure eigenstates of the Hamiltonian, the principal correlator should be fit well by a single exponential and double checked for the consistency of the obtained energies. The leading contamination due to higher-lying states is another exponential having higher energy; we use a two-exponential fit to help remove this contamination. The overlap factors (AnA_{n}) between the interpolating operators and the nthn^{\text{th}} state are derived from the eigenvectors obtained in the variational method.

To calculate the GPD matrix elements at nonzero momentum transfer, first calculate the matrix element χN(Pf)|Oμ|χN(Pi)\langle\chi_{N}(\vec{P}_{f})|O^{\mu}|\chi_{N}(\vec{P}_{i})\rangle, where χN\chi_{N} is the nucleon spin-1/2 interpolating field, ϵabc[qa(x)Cγ5qb(x)]qc(x)\epsilon^{abc}[q^{a\top}(x)C\gamma_{5}q^{b}(x)]q^{c}(x). Oμ=ψ¯γμW(z)ψO_{\mu}=\overline{\psi}\gamma_{\mu}W(z)\psi is the LaMET Wilson-line displacement operator with ψ\psi being either an up or down quark field, and P{i,f}\vec{P}_{\{i,f\}} are the initial and final nucleon momenta. We integrate out the spatial dependence and project the baryonic spin, using projection operators ρ=1+γt2(1+iγ5γρ)\mathbb{P}_{\rho}=\frac{1+\gamma_{t}}{2}(1+i\gamma_{5}\gamma_{\rho}) with ρ{x,y,z}\rho\in\{x,y,z\}, leaving a time-dependent three-point correlator, C3ptC_{\text{3pt}}.

Γμ,AB(3),ρ(ti,t,tf,pi,Pf)\displaystyle\Gamma^{(3),\mathbb{P}_{\rho}}_{\mu,AB}(t_{i},t,t_{f},\vec{p}_{i},\vec{P}_{f}) =\displaystyle= ZOnnfn,n(Pf,Pi,En,En,t,ti,tf)\displaystyle Z_{O}\sum_{n}\sum_{n^{\prime}}f_{n,n^{\prime}}(P_{f},P_{i},E_{n}^{\prime},E_{n},t,t_{i},t_{f}) (7)
×\displaystyle\times s,s(ρ)αβun(Pf,s)βNn(Pf,s)|Oμ|Nn(Pi,s)u¯n(Pi,s)α,\displaystyle\sum_{s,s^{\prime}}(\mathbb{P}_{\rho})_{\alpha\beta}u_{n^{\prime}}(\vec{P}_{f},s^{\prime})_{\beta}\langle N_{n^{\prime}}(\vec{P}_{f},s^{\prime})\left|O_{\mu}\right|N_{n}(\vec{P}_{i},s)\rangle\overline{u}_{n}(\vec{P}_{i},s)_{\alpha},

where fn,n(Pf,Pi,En,En,t,ti,tf)f_{n,n^{\prime}}(P_{f},P_{i},E_{n}^{\prime},E_{n},t,t_{i},t_{f}) contains kinematic factors involving the energies EnE_{n} and overlap factors AnA_{n} obtained in the two-point variational method, nn and nn^{\prime} are the indices of different energy states and ZOZ_{O} is the operator renormalization constant (which is determined nonperturbatively). We also use high-statistics measurements, 501,760 total over 1960 configurations, to drive down the increased statistical noise at high boost momenta, Pz=|Pi+Pf2|=|2πL{0,0,10}a1|P_{z}=\left|\frac{\vec{P_{i}}+\vec{P_{f}}}{2}\right|=|\frac{2\pi}{L}\{0,0,10\}a^{-1}|, and vary spatial momentum transfer q=PfPi=2πL{nx,ny,0}a1\vec{q}=\vec{P_{f}}-\vec{P_{i}}=\frac{2\pi}{L}\{n_{x},n_{y},0\}a^{-1} with all possible integer nx,yn_{x,y} and nx2+ny2{0,4,8,16,20}n_{x}^{2}+n_{y}^{2}\in\{0,4,8,16,20\} with transfer four-momentum squared Q2=qμqμ={0,0.19,0.39,0.77,0.97}Q^{2}=-q_{\mu}q^{\mu}=\{{0,0.19,0.39,0.77,0.97}\} GeV2. Figure 6 shows an example of the ground-state matrix elements (shown as the gray band) from the variational analysis along with the two-state fitted results with Pf={1,0,10}2πL\vec{P_{f}}=\{1,0,10\}\frac{2\pi}{L} and Pi={1,0,10}2πL\vec{P_{i}}=\{-1,0,10\}\frac{2\pi}{L} with projection operator 1+γt2(1+iγ5γz)\frac{1+\gamma_{t}}{2}(1+i\gamma_{5}\gamma_{z}). The ground-state matrix elements can be extracted from v0TC3ptij(t)v0v_{0}^{T}C_{\text{3pt}}^{ij}(t)v_{0} using the eigenvectors from the two-point variational-method analysis (shown in the left panel of Fig. 6), simultaneous two-state fitted results using source-sink separation of tsep=[8,12]t_{\text{sep}}=[8,12] lattice units, two-state fitted results as functions of tsepmint_{\text{sep}}^{\text{min}}. The consistency of these methods demonstrates that our extracted ground-state matrix elements are stably determined. For more details on the lattice study of nucleon matrix elements comparing the variational and two-state fit methods, we refer readers to Ref. Yoon et al. (2016), which contains a very detailed discussion.

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Figure 6: An example of the ground-state matrix element determination using variational method using rotated two- and three-point correlators (left), two-state fit to multiple source-sink separation (middle), along with the ratio plots data and reconstructed fit to the ratio points. The rightmost plot shows how much the ground-state matrix elements change as we reduce the inputs to the fits; we see some fluctuations and increase of errors due to the reduction of the available data but overall steady determination of the ground-state matrix element. The example used here is from Pf={1,0,10}2πL\vec{P_{f}}=\{1,0,10\}\frac{2\pi}{L} and Pi={1,0,10}2πL\vec{P_{i}}=\{-1,0,10\}\frac{2\pi}{L} with projection operator 1+γt2(1+iγ5γz)\frac{1+\gamma_{t}}{2}(1+i\gamma_{5}\gamma_{z}).

The overdetermined system of linear equations (using multiple q\vec{q} and projection operators) allows for solution of hH(Pz,Q2,z)h_{H}(P_{z},Q^{2},z) and hE(Pz,Q2,z)h_{E}(P_{z},Q^{2},z), similar to vector form factor calculations with our chosen projection operator and momentum configuration: The ground-state matrix elements are proportional to

Tr{ρ[if+mN][hH(Pz,Q2,z)γt+hE(Pz,Q2,z)iσtνqν2MN][ii+mN]}4EN(Pf)EN(Pi)\frac{\operatorname{Tr}\left\{\mathbb{P}_{\rho}\,[-i\not{P_{f}}+m_{N}]\>[h_{H}(P_{z},Q^{2},z)\gamma_{t}+h_{E}(P_{z},Q^{2},z)\frac{i\sigma^{t\nu}q_{\nu}}{2M_{N}}]\,[-i\not{P_{i}}+m_{N}]\,\right\}}{4\,E_{N}(\vec{P_{f}})E_{N}(\vec{P_{i}}\,)} (8)

with =iEN(p)γ4+pγ\not{p}=iE_{N}(\vec{p}\,)\gamma_{4}+\vec{p}\cdot\vec{\gamma}. We obtain a linear system of equations by using different projection operators ρ\mathbb{P}_{\rho}, momenta PfP_{f} and PiP_{i} to solve for HH and EE in coordinate space, h{H,E}(Pz,Q2,z)h_{\{H,E\}}(P_{z},Q^{2},z). Selected Q2Q^{2} values of h{H,E}(Pz,Q2,z)h_{\{H,E\}}(P_{z},Q^{2},z) normalized by h{H,E}(Pz,Q2=0,z=0)h_{\{H,E\}}(P_{z},Q^{2}=0,z=0) are shown in Fig. 7. The real matrix elements decrease quickly to zero due to the large boost momentum used in this calculation. This helps us to use smaller-displacement data to avoid large contributions from higher-twist effects in the larger-zz region.

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Figure 7: The Wilson-line length displacement zz-dependence of normalized matrix elements hH(Pz,Q2,z)h_{H}(P_{z},Q^{2},z) (top) and hE(Pz,Q2,z)h_{E}(P_{z},Q^{2},z) (bottom) at selected Q2{0.19,0.39,0.77} GeV2Q^{2}\in\{0.19,0.39,0.77\}\text{ GeV}^{2}.

To obtain the quasi-GPDs, we first apply nonperturbative renormalization (NPR) in RI/MOM scheme to the bare matrix elements, using the NPR done in previous work using the same lattice ensembles Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a), itself following the same strategy described in Refs. Stewart and Zhao (2018); Chen et al. (2018a). The RI/MOM renormalization constant Z{Z} is calculated nonperturbatively on the lattice by imposing the following momentum-subtraction condition on the matrix element:

Z(pzR,μR)=Tr[𝒫sps|ψ¯f(λz^)γtW(λz^,0)ψf(0)|ps]Tr[𝒫sps|ψ¯f(λz^)γtW(λz^,0)ψf(0)|pstree]|p2=μR2pz=pzR,Z(p^{R}_{z},\mu_{R})=\\ \left.\frac{\operatorname{Tr}[\mathcal{P}\sum_{s}\langle ps|\bar{\psi}_{f}(\lambda\hat{z})\gamma_{t}W(\lambda\hat{z},0)\psi_{f}(0)|ps\rangle]}{\operatorname{Tr}[\mathcal{P}\sum_{s}\langle ps|\bar{\psi}_{f}(\lambda\hat{z})\gamma_{t}W(\lambda\hat{z},0)\psi_{f}(0)|ps\rangle_{\text{tree}}]}\right|_{\tiny\begin{matrix}p^{2}=-\mu_{R}^{2}\\ \!\!\!\!p_{z}=p^{R}_{z}\end{matrix}}, (9)

where 𝒫=γtpxptγx+pyptγypx2+py2\mathcal{P}=\gamma_{t}-\frac{p_{x}p_{t}\gamma_{x}+p_{y}p_{t}\gamma_{y}}{p_{x}^{2}+p_{y}^{2}}. On the lattice, ps|Ot(z)|ps\langle ps|O_{t}(z)|ps\rangle is calculated from the amputated Green function of OtO_{t} with Euclidean external momentum. In this work, we use the same renormalization scales as used in the previous work Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a): μR=3.8\mu_{R}=3.8 GeV, pzR=2.2p_{z}^{R}=2.2 GeV, μMS¯=3\mu^{\overline{\text{MS}}}=3 GeV. The renormalization-scale dependence was studied in Ref. Liu et al. (2018b). We also vary the values of PzRP_{z}^{R}, and the results are shown in Fig. 8, focusing on the ξ=0\xi=0 GPDs, where the matching formula is the same as that in the PDFs, as discussed in Ref. Liu et al. (2019). We normalize all matrix elements by hH(Pz,Q2=0,z=0)h_{H}(P_{z},Q^{2}=0,z=0), as in our previous PDF work Chen et al. (2018b); Lin et al. (2018b); Liu et al. (2018a). Using matrix-element ratios reduces the lattice systematic error, since in the continuum limit hH(Pz,Q2=0,z=0)h_{H}(P_{z},Q^{2}=0,z=0), the vector charge, goes to 1.

We also perform checks of the zmaxz_{\text{max}} input in the Fourier transformation and lattice-spacing dependence. The effects are documented in Fig. 8.

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Figure 8: Examples of the systematics being considered in this calculation. The left and middle show examples of post-matching HH-GPD at Q2=0.39Q^{2}=0.39 GeV2 with varying choices of pzRp_{z}^{R} and zmaxz_{\text{max}} in the NPR and maximum Wilson-line displacement zmaxz_{\text{max}} used in quasi-GPD. We found the effects to be mild except in the small-xx region. The right-hand side shows a comparison of 310-MeV nucleon isovector matrix elements for PDF at lattice spacings of 0.12 and 0.042 fm for around 2.2 GeV nucleon boost momentum.