delta-baryon electromagnetic form factors in lattice QCD The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Alexandrou, C. et al. "delta-baryon electromagnetic form factors in lattice QCD." Physical Review D 79.1 (2009): 014507. As Published http://dx.doi.org/10.1103/PhysRevD.79.014507 Publisher American Physical Society Version Final published version Accessed Thu May 26 23:24:26 EDT 2016 Citable Link http://hdl.handle.net/1721.1/52708 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. Detailed Terms PHYSICAL REVIEW D 79, 014507 (2009) -baryon electromagnetic form factors in lattice QCD C. Alexandrou,1 T. Korzec,1 G. Koutsou,1 Th. Leontiou,1 C. Lorcé,2 J. W. Negele,3 V. Pascalutsa,2 A. Tsapalis,4 and M. Vanderhaeghen2 1 Department of Physics, University of Cyprus, P.O. Box 20537, 1678 Nicosia, Cyprus Institut für Kernphysik, Johannes Gutenberg-Universität, D-55099 Mainz, Germany 3 Center for Theoretical Physics, Laboratory for Nuclear Science and Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 4 Institute of Accelerating Systems and Applications, University of Athens P.O. Box 17214, GR-10024, Athens, Greece (Received 22 October 2008; published 21 January 2009) 2 We develop techniques to calculate the four electromagnetic form factors using lattice QCD, with particular emphasis on the subdominant electric quadrupole form factor that probes deformation of the . Results are presented for pion masses down to approximately 350 MeV for three cases: quenched QCD, two flavors of dynamical Wilson quarks, and three flavors of quarks described by a mixed action combining domain-wall valence quarks and dynamical staggered sea quarks. The magnetic moment of the is compared with chiral effective field theory calculations and the charge density distributions are discussed. DOI: 10.1103/PhysRevD.79.014507 PACS numbers: 11.15.Ha, 12.38.Aw, 12.38.Gc I. INTRODUCTION Lattice quantum chromodynamics (QCD) provides a well-defined framework to directly calculate hadron form factors from the fundamental theory of strong interactions. Form factors characterize the internal structure of hadrons, including their magnetic moment, their size, and their charge density distribution. Since the ð1232Þ decays strongly, experiments [1,2] to measure its form factors are harder and yield less precise results than for nucleons [3,4]. In this work, we compute form factors using lattice QCD more accurately than can be currently obtained from experiment. A primary motivation for this work is to understand the role of deformation in baryon structure: whether any of the low-lying baryons have deformed intrinsic states and if so, why. Thus, a major achievement of this work is the development of lattice methods with sufficient precision to show, for the first time, that the electric quadrupole form factor is nonzero and hence the has a nonvanishing quadrupole moment and an associated deformed shape. Unlike the , the spin-1=2 nucleon cannot have a quadrupole moment, so the experiment of choice to explore its deformation has been measurement of the nucleon to electric and Coulomb quadrupole transition form factors. Major experiments [5–7] have shown that these transition form factors are indeed nonzero, confirming the presence of deformation in either the nucleon , or both [8,9], and lattice QCD yields comparable nonzero results [10,11]. Our new calculation of the quadrupole form factor, coupled with the nucleon to transition form factors, should in turn shed light on the deformation of the nucleon. In order to evaluate the electromagnetic (EM) form factors to the required accuracy, we isolate the two dominant form factors and the subdominant electric quadrupole form factor. This is particularly crucial for the latter since 1550-7998= 2009=79(1)=014507(5) without the construction of an optimized source for the sequential propagator it can not be extracted with the required precision. We note that this increases the computational cost since additional inversions are needed. Our techniques are first tested in quenched QCD [12]. We then calculate form factors using two degenerate flavors of dynamical Wilson fermions, denoted by NF ¼ 2, with pion masses in the range of 700 MeV to 380 MeV [13,14]. Finally, we use a mixed action with chirally symmetric domain-wall valence quarks and staggered sea quarks with two degenerate light flavors and one strange flavor [15], denoted by NF ¼ 2 þ 1, at a pion mass of 353 MeV. Using the results obtained with dynamical quarks, we extrapolate the magnetic moment to the physical point. We extract the quark charge distributions in the , and discuss their quadrupole moment. II. LATTICE EVALUATION The matrix element of the EM current j EM , hðpf ; sf Þjj jðp ; s Þi, can be parametrized in terms of i i EM four multipole form factors that depend only on the momentum transfer q2 Q2 ¼ ðpf pi Þ2 [16] The decomposition for the on shell matrix element is given by ðpf ; sf ÞO u ðpi ; si Þ hðpf ; sf Þjj EM jðpi ; si Þi ¼ Au a ðq2 Þ ðpf þ p Þ O ¼ g a1 ðq2 Þ þ 2 i 2m 2 q q 2 Þ þ c2 ðq Þ ðp þ p Þ ; ðq (1) c 1 i f 2m 4m2 where a1 ðq2 Þ, a2 ðq2 Þ, c1 ðq2 Þ, and c2 ðq2 Þ are known linear combinations of the electric charge form factor GE0 ðq2 Þ, the magnetic dipole form factor GM1 ðq2 Þ, the electric 014507-1 Ó 2009 The American Physical Society PHYSICAL REVIEW D 79, 014507 (2009) C. ALEXANDROU et al. 2 quadrupole form factor GE2 ðq Þ, and the magnetic octupole form factor GM3 ðq2 Þ [17], and A is a known factor depending on the normalization of hadron states. These form factors can be extracted from correlation functions calculated in lattice QCD [17]. We calculate in Euclidean time the two- and three-point correlation functions in a frame where the final state is at rest: ~ ¼ Gðt; qÞ 3 XX eix~f q~ 4 hJj ðxf ÞJj ð0Þi x~ f j¼1 X ~ ¼ eix~ q~ hJ ðxf Þj ðxÞJ ð0Þi; G ð ; t; qÞ (2) x~ f x~ where j is the electromagnetic current on the lattice, J and J are the þ interpolating fields constructed from smeared quarks [12], 4 ¼ 14 ð1 þ 4 Þ, and k ¼ i4 5 k . The form factors can then be extracted from ratios of three- and two-point functions in which unknown normalization constants and the leading time dependence cancel v ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi u u ð; t; qÞ ~ ~ Gðtf t; p~ i ÞGðt; 0ÞGðt ~ G u f ; 0Þ t : R ¼ ~ ~ Gðtf t; 0ÞGðt; p~ i ÞGðtf ; p~ i Þ Gðtf ; 0Þ (3) For sufficiently large tf t and t ti , this ratio exhibits a ~ ! ð; qÞ, ~ from which the form factors plateau Rð; t; qÞ are extracted, and we use the particular combinations 3 X ~ ¼ K1 GE0 ðQ2 Þ þ K2 GE2 ðQ2 Þ; k k ð4 ; qÞ The connected part of each combination of three-point functions can be calculated efficiently using the method of sequential inversions [18]. These yield the isovector form factors. At present, it is not yet computationally feasible to calculate the contributions arising from disconnected diagrams. A calculation of disconnected contributions in the case of the electromagnetic form factors have shown that these are consistent with zero [19]. We note that these disconnected contributions are particularly hard to calculate not just because they require the all-to-all propagators but also because they are noise dominated [20]. We expect that, like in the case of nucleon electromagnetic form factors, the disconnected contributions to the electromagnetic form factors are small. The known kinematical coefficients K1 , K2 , K3 , K4 are functions of the mass and ~ The combinations above are energy as well as of and q. chosen such that all possible directions of and q~ contribute symmetrically to the form factors at a given Q2 [21]. The over-constrained system of Eqs. (4)–(6) is solved by a least-squares analysis, and GE2 ðQ2 Þ can also be isolated separately from Eq. (6). The details of the simulations are summarized in Table I. In each case, the separation between the final and initial time is tf ti * 1 fm and Gaussian smearing is applied to both source and sink to produce adequate plateaus by suppressing contamination from higher states having the quantum numbers of the ð1232Þ. For the mixed-action calculation, the domain-wall valence quark mass was chosen to reproduce the lightest pion mass obtained using NF ¼ 2 þ 1 improved staggered quarks [21,23]. (4) III. RESULTS k¼1 3 X jkl j k ð 4 2 ~ ¼ K3 GM1 ðQ Þ; ; qÞ (5) ~ ¼ K4 GE2 ðQ2 Þ: jkl j 4 k ðj ; qÞ (6) j;k;l¼1 3 X j;k;l¼1 The results for GE0 ðQ2 Þ are shown in Fig. 1 as a function of Q2 at the lightest pion mass for each of the three actions. For Wilson fermions, we use the conserved lattice current requiring no renormalization. The local current is used for the mixed action, and the renormalization constant ZV ¼ 1:0992ð32Þ is determined by the condition that GE0 ð0Þ equals the charge of the in units of e. As can be seen, pffiffiffiffiffiffiffiffi TABLE I. Lattice parameters and results. Nconf denotes the number of lattice configurations, hr2 i gives the charge radius, þ is þ the þ magnetic moment in nuclear magnetons and Q 3=2 is the quadrupole moment. pffiffiffiffiffiffiffiffi Nconf m [GeV] m [GeV] hr2 i [fm] þ [N ] Q 3=2 200 200 200 0.563(4) 0.490(4) 0.411(4) 185 157 200 0.691(8) 0.509(8) 0.384(8) 300 0.353(2) Quenched Wilson, 323 64, a ¼ 0:092 fm 1.470(15) 0.6147(66) 1.720(42) 1.425(16) 0.6329(76) 1.763(51) 1.382(19) 0.6516(87) 1.811(69) NF ¼ 2 Wilson, 243 40 (32 for lightest pion), a ¼ 0:077 fm 1.687(15) 0.5279(61) 1.462(45) 1.559(19) 0.594(10) 1.642(81) 1.395(18) 0.611(17) 1.58(11) NF ¼ 2 þ 1, Mixed action, 283 64, a ¼ 0:124 fm [22] 1.533(27) 0.641(22) 1.91(16) 014507-2 0.96(12) 0.91(15) 0.83(21) 0.80(21) 0.41(45) 0.46(35) 0.74(68) -BARYON ELECTROMAGNETIC FORM FACTORS IN . . . quenched Wilson, mπ = 410 MeV hybrid, m = 353 MeV π 1 dynamical Wilson, mπ = 384 MeV GE0 0.8 0.6 0.4 0.2 0 0 0.5 1 1.5 2 2 2.5 2 Q in GeV FIG. 1 (color online). The electric charge form factor versus Q2 . The green (red) line and error band show a dipole fit to the mixed-action (quenched) results. all three calculations yield consistent results. The momentum dependence of the charge form factor is described well 2 by a dipole form GE0 ðQ2 Þ ¼ 1=ð1 þ Q2 Þ2 . To compare the E0 slopes at Q2 ¼ 0, we follow convention and show in Table I the so-called ‘‘rms radius’’ hr2 i ¼ d 2 6 dQ 2 GE0 ðQ ÞjQ2 ¼0 [17]. The momentum dependence of GM1 ðQ2 Þ is displayed in Fig. 2. In order to extract the magnetic moment an extrapolation to zero momentum transfer is necessary. Both an 2 2 exponential form, GM1 eQ =M1 , and a dipole describe the 4 PHYSICAL REVIEW D 79, 014507 (2009) 2 Q dependence well, and we adopt the exponential form because of its faster decay at large Q2 , in accord with perturbative arguments. The larger spatial volume for the quenched and mixed-action cases yields smaller and more densely spaced values of the lattice momenta and correspondingly more precise determination of the form factor than for the smaller volume used with dynamical Wilson fermions. In Fig. 2, we show the best exponential fit and error band for the mixed action and quenched results. As can be seen, results in the quenched theory and for NF ¼ 2 Wilson fermions are within the error band. The magnetic moment in natural units is given by ¼ GM1 ð0Þe=ð2m Þ, where m is the mass measured on the lattice and GM1 ð0Þ is from the exponential fits. In Table I, we give the values of the þ magnetic moment in nuclear magnetons e=ð2mN Þ, with mN the physical nucleon mass. The magnetic moments of the þ and þþ are accessible to experiments [1,2], which presently suffer from large uncertainties. The magnetic moment as function of m2 is shown in Fig. 3, together with a comparison to a chiral effective field theory (ChEFT) result [24]. The ChEFT result has one free parameter (a low-energy constant) that has been fitted to lattice data, shown by the central line. We also estimate the uncertainty of the ChEFT expansion (expansion in pion mass) by the error band in Fig. 3. The uncertainty of the ChEFT calculation vanishes in the chiral limit because in this limit one simply has the value of the low-energy constant, which lies within the broad experimental error band þ ¼ 2:7þ1:0 1:3 ðstatÞ 1:5ðsystÞ 3:0ðtheoryÞN [1]. In this work, we do not consider the uncertainty in the fit value of the low-energy constant due to the lattice errors, as the calculations are still performed for pion masses where the is stable (on the right side of the kink). A calculation for pion mass values where the quenched Wilson, m = 410 MeV π 3.5 hybrid, m = 353 MeV π dynamical Wilson, mπ = 384 MeV 3 GM1 2.5 2 1.5 1 0.5 0 0 0.5 1 2 1.5 2 2.5 2 Q in GeV FIG. 2 (color online). The magnetic dipole form factor. The green (red) line and error band show an exponential fit to the mixed-action (quenched) results. FIG. 3 (color online). The magnetic dipole moment in nuclear magnetons. The value at the physical pion mass (filled square) is shown with statistical and systematic errors [1]. The solid and dashed curves show the results of ChEFT with the theoretical error estimate [24]. 014507-3 PHYSICAL REVIEW D 79, 014507 (2009) C. ALEXANDROU et al. becomes unstable will be a challenge for future calculations. The moments using an approach similar to ours are calculated only in the quenched approximation [17,25,26]. Our magnetic moment results agree with recent background field calculations using dynamical improved Wilson fermions [27], which supersede previous quenched background field results [28]. The spatial length Ls of our lattices satisfies Ls m > 4 in all cases except at the lightest pion mass with NF ¼ 2 Wilson fermions, for which Ls m ¼ 3:6. For that point, the magnetic moment falls slightly below the error band, consistent with the fact that Ref. [27] shows that finite volume effects decrease the magnetic moment. The electric quadrupole form factor is particularly interesting because it can be related to the shape of a hadron, and lattice calculations for each of the three actions are shown in Fig. 4 with exponential fits for the quenched and mixed-action cases. Just as the electric form factor for a spin-1=2 nucleon can be expressed precisely as the transverse Fourier transform of the transverse quark charge density in the infinite momentum frame [29], a proper field-theoretic interpretation of the shape of the ð1232Þ can be obtained by considering the quark transverse charge densities in this frame [30–32]. With respect to the direction of the average baryon momentum P, the transverse charge density in a spin-3=2 state with transverse polarization s? is defined as ~ Ts? ðbÞ Z d2 q~ ? ~ 1 eiq~ ? b þ 2 2P ð2Þ ~ ~? q þ þ; q ; s Pþ ; ? ; s? ð0Þ ; P J 2 2 ? Q2 , J þ J 0 þ J 3 , and b~ specifies the quark position in the xy plane relative to the center of mass. Choosing the transverse spin vector along the x axis, the quadrupole moment of this two-dimensional charge distribution is defined as [21]: Z ~ ~ 2x b2y Þ ðbÞ: Q e d2 bðb (8) s? Ts? In terms of the EM form factors [21], 1 e Q 3=2 ¼ f2½GM1 ð0Þ 3e þ ½GE2 ð0Þ þ 3e g 2 : (9) 2 m The term proportional to ½GM1 ð0Þ 3e is an electric quadrupole moment induced in the moving frame due to the magnetic dipole moment. For a spin-3=2 particle without internal structure, GM1 ð0Þ ¼ 3e , GE2 ð0Þ ¼ 3e [21,33], and the quadrupole moment of the transverse charge density vanishes. Hence, Q s? , and thus the deformation of the two-dimensional transverse charge density, is only sensitive to the anomalous parts of the spin-3=2 magnetic dipole and electric quadrupole moments, and vanishes for a particle without internal structure. The analogous property holds for a spin-1 particle [32], indicating the generality of this description in terms of transverse densities. þ Figure 5 shows the transverse density Ts? for a with transverse spin s? ¼ þ3=2 calculated from the fit to the quenched Wilson lattice results for the form factors (which has the smallest statistical errors of the three cal- (7) where the photon transverse momentum q~ ? satisfies q~ 2? ¼ 0 GE2 −1 −2 quenched Wilson, m = 410 MeV −3 π hybrid, mπ = 353 MeV −4 dynamical Wilson, m = 384 MeV π 0 0.5 1 1.5 Q2 in GeV2 FIG. 4 (color online). The electric quadrupole form factor. The notation is the same as that in Fig. 1. The value of GE2 , in units of e=ð2m2 Þ, at Q2 ¼ 0 are 0:810 0:291 for the quenched calculation, 0:87 0:67 for the dynamical Wilson case, and 2:06þ1:27 2:35 for the hybrid calculation. FIG. 5 (color online). Quark transverse charge density in a þ polarized along the x axis, with s? ¼ þ3=2. The light (dark) regions correspond with the largest (smallest) values of the density. 014507-4 -BARYON ELECTROMAGNETIC FORM FACTORS IN . . . þ culations). It is seen that the quark charge density is elongated along the axis of the spin (prolate). This prolate deformation is robust in the sense that the values for Q 3=2 obtained from Eq. (9) and given in Table I are all consistently positive. The connection between the results on deformation in the current formulation and previous ones will be discussed in a forthcoming publication [21]. In the case of the magnetic octupole form factor [21], which is related to the magnetic octupole moment O ¼ GM3 ð0Þe=2m3 , our statistics are insufficient to distinguish the result from zero. IV. CONCLUSIONS In summary, a formalism for the accurate evaluation of the electromagnetic form factors as functions of q2 has been developed and used in quenched QCD and full QCD with two and 2 þ 1 flavors. 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