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Physics Letters B 708 (2012) 186–190 Contents lists available at SciVerse ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Notes on the orbital angular momentum of quarks in the nucleon Yoshitaka Hatta Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Ibaraki 305-8571, Japan article info abstract Article history: Received 18 November 2011 Received in revised form 10 January 2012 Accepted 10 January 2012 Available online 12 January 2012 Editor: J.-P. Blaizot We discuss the orbital angular momentum of partons inside a longitudinally polarized proton in the recently proposed framework of spin decomposition. The quark orbital angular momentum defined by Ji can be decomposed into the ‘canonical’ and the ‘potential’ angular momentum parts, both of which are represented as the matrix element of a manifestly gauge invariant operator. © 2012 Elsevier B.V. All rights reserved. 1. Introduction Recent polarized beam experiments and global QCD analyses suggest that the contribution of the gluon helicity G to the spin of the proton is rather small [1]. This observation, together with the inexorable fact that the quark helicity contribution Σ is also small (less than 30%), lead one to suspect that the key to under- stand the proton spin puzzle is the orbital angular momentum (OAM) of quarks and gluons. However, progress in this direction has been hindered by a number of difficulties in measuring, and even defining the OAM. So far, the only well-recognized, gauge invariant definition of the quark OAM is the one by Ji [2] which can be measured, indirectly, as the difference between a certain moment of the generalized parton distribution and Σ . Although generally accepted, this approach may be criticized on the basis that the corresponding operator is not the ‘canonical’ one that satisfies the fundamental commutation relation of the angular mo- mentum operator in quantum mechanics. Efforts to improve upon this point have led Chen et al. to propose a completely new de- composition scheme of the QCD angular momentum tensor [3,4] which has triggered a flurry of activity lately [5–14]. However, the issue still remains very controversial, and the overarching impact of this new formalism as well as its practical usefulness in phe- nomenology are yet to be clarified. In this work, we investigate the quark OAM along the line of our previous work [10] which we view as the proper rendition of the formalism [3,4] in the context of high energy QCD. We shall show that one can represent the canonical OAM as the matrix el- ement of a manifestly gauge invariant operator which turns out to be equivalent to that obtained in the Wigner distribution approach [16]. This paves the way to measure the canonical OAM experi- mentally or numerically on a lattice, and thus helps to mitigate E-mail address: [email protected]. the criticism that the matrix elements defined in [3] do not have known physical measurements [17]. Actually, in the gluon helic- ity sector Ref. [10] has already shown how one can reconcile the gluon helicity defined in [3] with G which is measurable. We now extend this finding to the OAM sector. 2. Decomposition of the QCD angular momentum operator The main idea of [3,4] is that one can achieve a complete, gauge invariant decomposition of the QCD angular momentum operator by identifying the ‘physical’ and ‘pure gauge’ components of the gauge field A μ = A μ phys + A μ pure , (1) F μν pure = μ A ν pure ν A μ pure + ig A μ pure , A ν pure = 0, (2) which transform differently under gauge transformations A μ phys U A μ phys U , A μ pure U A μ pure U i g U μ U . (3) The QCD angular momentum tensor M μνλ can then be written as a sum of the helicity and the orbital angular momentum of quarks and gluons. In the ‘covariant’ form [5,6] useful for high energy ex- periments, the original proposal by Chen et al. [3,4] reads M μν λ quark-spin =− 1 2 μν λσ ¯ ψ γ 5 γ σ ψ, (4) M μν λ quark-orbit = ¯ ψ γ μ ( x ν iD λ pure x λ iD ν pure ) ψ, (5) M μν λ gluon-spin = F μλ a A νa phys F μν a A λa phys , (6) M μν λ gluon-orbit = F μα a ( x ν ( D λ pure A phys α ) a x λ ( D ν pure A phys α ) a ) , (7) 0370-2693/$ – see front matter © 2012 Elsevier B.V. All rights reserved. doi:10.1016/j.physletb.2012.01.024

Notes on the orbital angular momentum of quarks in the nucleon

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Physics Letters B 708 (2012) 186–190

Contents lists available at SciVerse ScienceDirect

Physics Letters B

www.elsevier.com/locate/physletb

Notes on the orbital angular momentum of quarks in the nucleon

Yoshitaka Hatta

Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Ibaraki 305-8571, Japan

a r t i c l e i n f o a b s t r a c t

Article history:Received 18 November 2011Received in revised form 10 January 2012Accepted 10 January 2012Available online 12 January 2012Editor: J.-P. Blaizot

We discuss the orbital angular momentum of partons inside a longitudinally polarized proton in therecently proposed framework of spin decomposition. The quark orbital angular momentum defined by Jican be decomposed into the ‘canonical’ and the ‘potential’ angular momentum parts, both of which arerepresented as the matrix element of a manifestly gauge invariant operator.

© 2012 Elsevier B.V. All rights reserved.

1. Introduction

Recent polarized beam experiments and global QCD analysessuggest that the contribution of the gluon helicity �G to the spinof the proton is rather small [1]. This observation, together withthe inexorable fact that the quark helicity contribution �Σ is alsosmall (less than 30%), lead one to suspect that the key to under-stand the proton spin puzzle is the orbital angular momentum(OAM) of quarks and gluons. However, progress in this directionhas been hindered by a number of difficulties in measuring, andeven defining the OAM. So far, the only well-recognized, gaugeinvariant definition of the quark OAM is the one by Ji [2] whichcan be measured, indirectly, as the difference between a certainmoment of the generalized parton distribution and �Σ . Althoughgenerally accepted, this approach may be criticized on the basisthat the corresponding operator is not the ‘canonical’ one thatsatisfies the fundamental commutation relation of the angular mo-mentum operator in quantum mechanics. Efforts to improve uponthis point have led Chen et al. to propose a completely new de-composition scheme of the QCD angular momentum tensor [3,4]which has triggered a flurry of activity lately [5–14]. However, theissue still remains very controversial, and the overarching impactof this new formalism as well as its practical usefulness in phe-nomenology are yet to be clarified.

In this work, we investigate the quark OAM along the line ofour previous work [10] which we view as the proper rendition ofthe formalism [3,4] in the context of high energy QCD. We shallshow that one can represent the canonical OAM as the matrix el-ement of a manifestly gauge invariant operator which turns out tobe equivalent to that obtained in the Wigner distribution approach[16]. This paves the way to measure the canonical OAM experi-mentally or numerically on a lattice, and thus helps to mitigate

E-mail address: [email protected].

0370-2693/$ – see front matter © 2012 Elsevier B.V. All rights reserved.doi:10.1016/j.physletb.2012.01.024

the criticism that the matrix elements defined in [3] do not haveknown physical measurements [17]. Actually, in the gluon helic-ity sector Ref. [10] has already shown how one can reconcile thegluon helicity defined in [3] with �G which is measurable. Wenow extend this finding to the OAM sector.

2. Decomposition of the QCD angular momentum operator

The main idea of [3,4] is that one can achieve a complete, gaugeinvariant decomposition of the QCD angular momentum operatorby identifying the ‘physical’ and ‘pure gauge’ components of thegauge field

Aμ = Aμphys + Aμ

pure, (1)

F μνpure = ∂μ Aν

pure − ∂ν Aμpure + ig

[Aμ

pure, Aνpure

] = 0, (2)

which transform differently under gauge transformations

Aμphys → U † Aμ

physU ,

Aμpure → U † Aμ

pureU − i

gU †∂μU . (3)

The QCD angular momentum tensor Mμνλ can then be written asa sum of the helicity and the orbital angular momentum of quarksand gluons. In the ‘covariant’ form [5,6] useful for high energy ex-periments, the original proposal by Chen et al. [3,4] reads

Mμνλ

quark-spin = −1

2εμνλσ ψ̄γ5γσ ψ, (4)

Mμνλ

quark-orbit = ψ̄γ μ(xν iDλ

pure − xλiDνpure

)ψ, (5)

Mμνλ

gluon-spin = F μλa Aνa

phys − F μνa Aλa

phys, (6)

Mμνλ = F μαa

(xν

(Dλ

pure Aphysα

) − xλ(

Dνpure Aphys

α

) ), (7)

gluon-orbit a a

Y. Hatta / Physics Letters B 708 (2012) 186–190 187

where Dνpure ≡ ∂ν + ig Aν

pure, and a,b = 1,2, . . . ,8 are the color in-

dices.1 Using the transformation rule (3), it is easy to check thateach of the above components is gauge invariant. Such a completedecomposition goes beyond Ji’s framework in which the gluonicpart cannot be separated into the helicity and orbital parts. Theprice to pay, however, is that the decomposition is not local in thesense that Aμ

phys is in general nonlocally related to the total Aμ .

Moreover, it is not entirely covariant, either, because Aμphys actually

depends on the frame as we shall soon see. An alternative decom-position of the orbital part was suggested by Wakamatsu [5]

M ′μνλ

quark-orbit = ψ̄γ μ(xν iDλ − xλiDν

)ψ, (8)

M ′μνλ

gluon-orbit = F μαa

(xν

(Dλ

pure Aphysα

)a − xλ

(Dν

pure Aphysα

)a

)+ (

Dα F αμ)

a

(xν Aλa

phys − xλ Aνaphys

). (9)

The second term of (9) is gauge invariant on its own. Using theequation of motion Dα F αμ

a = gψ̄γ μtaψ , one sees that it accountsfor the difference between Dν

pure in (5) and Dν in (8).There is no consensus as to which definition, (5) or (8), is more

appropriate for the quark orbital angular momentum. To some ex-tent, it is a matter of choice. It is (5), but not (8), that is compatiblewith the (equal-time) canonical commutation relation of the angu-lar momentum operator �L × �L = i�L,

�L = �x × i �Dpure, �x = (x1, x2, x3). (10)

The pure gauge condition (2) is crucial for this. (5) may thus becalled the canonical angular momentum.2 On the other hand, (8)is the same as Ji’s definition [2] and is accessible from the analysisof the generalized parton distribution (GPD), whereas it has notbeen known how to measure (5).

We will derive an explicit expression of the canonical angularmomentum (5) in terms of a manifestly gauge invariant operatorwhose matrix element is, in principle, related to experimental pro-cesses or observables in lattice QCD simulations. For this purpose,one must specify what Aμ

phys is. There are several proposals for

Aμphys in the literature [4,7,10,13]. These definitions are not equiv-

alent as suggested by the work of Ref. [8] which showed that theygive different values of the gluon helicity (the proton matrix ele-ment of (6)). Here we employ the one proposed in [10]

Aμphys(x) = −

∫dy− K(y − x)W−

xy F +μ(

y−, �x)W−yx, (11)

where we use the notation �x = (x+, xi) from now on. W is theWilson line operator

W−xy ≡ P exp

(−ig

x−∫y−

A+(y′−, �x)dy′−

), (12)

in the fundamental representation. The superscript ‘−’ denotesthat the path ordering is in the x− direction. K(y−) is either12 ε(y−), θ(y−) or −θ(−y−), depending on the boundary condi-

1 Our convention is ε0123 = +1, γ5 = −iγ 0γ 1γ 2γ 3. We shall use the light-cone

coordinates x± = 1√2(x0 ± x3) and denote the transverse coordinates with Latin

indices xT = {xi}, (i, j, . . . = 1,2). The two-dimensional antisymmetric tensor is de-fined as ε i j = −ε+−i j , ε12 = ε12 = −ε21 = 1.

2 Throughout this Letter, we associate the term ‘canonical’ with the operator

iDμpure instead of the usual i∂μ . The former is actually the gauge covariant gen-

eralization of the latter without affecting the commutation relation.

tion at x− = ±∞ in the light-cone gauge A+ = 0.3 The pure gaugepart Apure is

Aμpure(x) ≡ − i

gW−

x,±∞W±∞∂μ(W−

x,±∞W±∞)†

, (13)

where W±∞ =P exp(−ig∫ �x

�∞ �A(±∞, �x′) · d�x′) is the Wilson line inthe spatial direction at x− = ±∞. It represents the residual gaugesymmetry of the light-cone gauge A+ = 0, and is fixed by spec-ifying the boundary condition of the gauge field at x− → ±∞mentioned above. It has been shown in [10] that (11) and (13)are a viable decomposition of the total gauge field Aμ . We wishto stress that this particular choice is singled out among others bythe criterion of measurability: The corresponding gluon helicity co-incides with the usual gluon helicity �G that has been measuredin experiments.

Note that the definition (11) already selects a particular frame—the infinite momentum frame where the partonic interpretation ofhadrons is clearest. As emphasized in [15], the decomposition ofspin into the helicity and the orbital parts cannot be made entirelycovariant, but depends on the frame of reference.

3. Potential angular momentum

We now focus on the orbital angular momentum of quarks in-side a longitudinally polarized proton. It is given by the forwardmatrix element of the μνλ = +i j component of (5) or (8)

ε i j LChen

≡ 1

2P+〈P S| ∫ dx− d2xT M+i j

quark-orbit|P S〉(2π)3δ3(0)

= 1

2P+〈P S| ∫ dx− d2xT ψ̄γ +(xi iD j

pure − x j iDipure)ψ |P S〉

(2π)3δ3(0),

(14)

ε i j LJi ≡ 1

2P+〈P S| ∫ dx− d2xT M ′+i j

quark-orbit|P S〉(2π)3δ3(0)

= 1

2P+〈P S| ∫ dx− d2xT ψ̄γ +(xi iD j − x j iDi)ψ |P S〉

(2π)3δ3(0), (15)

where P 2 = −S2 = M2 (the proton mass squared) and(2π)3δ3(0) = ∫

dx− d2xT is the momentum space delta func-tion. The longitudinal polarization means Sμ = (S+, S−, ST ) ≈(S+,0,0T ). We first observe that, since Aμ

pure = 0 in the light-conegauge A+ = 0 [10], LChen is actually identical to the Jaffe–Manohar(JM) definition [18] of the quark orbital angular momentum

LJM = 1

2P+〈P S| ∫ dx− d2xT ψ̄γ +(x1i∂2 − x2i∂1)ψ |P S〉LC

(2π)3δ3(0). (16)

The subscript LC means that the matrix element is evaluated inthe light-cone gauge. In other words, LChen is the generalization ofLJM to arbitrary gauges (see, also, [5]). We thus unify the notationsLChen = LJM ≡ Lcan by introducing the canonical orbital angularmomentum Lcan, and write

LJi = Lcan + Lpot, (17)

where the so-called potential angular momentum [19,5] is, withour choice of Aμ

phys,

3 From the viewpoint of the PT (parity and time-reversal) symmetry which will

be crucially used below, it seems that the choice K(y−) = 12 ε(y−) is the most

natural and convenient one, although the difference does not matter in the end.

188 Y. Hatta / Physics Letters B 708 (2012) 186–190

ε i j Lpot = 1

2P+(2π)3δ3(0)

× 〈P S|∫

dx− d2xT xiψ̄(x)γ +(−g)

× (xi A j

phys − x j Aiphys

)ψ(x)|P S〉

= 1

2P+(2π)3δ3(0)

× 〈P S|∫

dx− d2xT

{xiψ̄(x)γ +

×∫

dy− K(

y− − x−)W−

xy g F + j(y−, �x)W−yxψ(x)

− x jψ̄(x)γ +∫

dy− K(

y− − x−)×W−

xy g F +i(y−, �x)W−yxψ(x)

}|P S〉. (18)

Now consider the non-forward matrix element

1

2 P̄+(2π)3δ3(0)〈P ′ S ′|

∫dx− d2xT xiψ̄(x)γ +

×∫

dy− K(

y− − x−)W−

xy g F + j(y−, �x)W−yxψ(x)|P S〉,

where P̄μ = (Pμ + P ′μ)/2 and the momentum transfer will bedenoted as �μ ≡ P ′μ − Pμ . The explicit factor xi can be traded forthe derivative with respect to �i such that

ε i j Lpot = 1

2P+ lim�→0

{∂

i∂�i〈P ′ S ′|ψ̄(0)γ +

×∫

dy− K(

y−)W−

0y g F + j(y−)W−

y0ψ(0)|P S〉

− (i ↔ j)

}. (19)

Parity and time-reversal (PT) symmetry tells that the followingparametrization of the matrix element is possible

〈P ′ S ′|ψ̄(0)γ +∫

dy− K(

y−)W−

0y g F +i(y−)W−

y0ψ(0)|P S〉= iε i j� j S̄+h(ξ) + · · · , (20)

where S̄ = (S + S ′)/2 and ξ ≡ −�+/2 P̄+ is the skewness pa-rameter. [The dependence of h(ξ) on the renormalization scale isimplicit. We also suppress the dependence on �2 ≈ −�2

T since itis of higher order. Similar comments apply to other distributionsdefined below.] This leads to

Lpot = h(0)S+

P+ . (21)

Eq. (20) thus defines the potential angular momentum as the ma-trix element of a manifestly gauge invariant operator.

The quark–gluon mixed operator that appears in the matrix el-ement (20) is familiar in the context of the twist-three mechanismof the single spin asymmetry (SSA). Let us pursue this analogy andconsider the following non-forward matrix element

T μν(x1, x2, ξ) =∫

dy− dz−

(2π)2e

i2 (x1+x2) P̄+z−+i(x2−x1) P̄+ y−

× 〈P ′S ′|ψ̄(−z−/2)γ +W−

−z2 y

g F μν(

y−)×W−

y z ψ(z−/2

)|P S〉

2

= 1

P̄+ εμνρσ S̄ρ P̄σ Ψ (x1, x2, ξ)

+ 1

P̄+ εμνρσ S̄ρ�σ Φ(x1, x2, ξ) + · · · . (22)

By symmetry considerations, it follows that Ψ (x1, x2, ξ) = Ψ (x2, x1,

−ξ) and Φ(x1, x2, ξ) = −Φ(x2, x1,−ξ). In the forward limit, andin the transversely polarized case Sμ = δ

μi S i , only the Ψ -term

survives. The function Ψ (x1, x2,0) plays the central role in theso-called soft gluonic pole mechanism of the SSA [20,21]. In thelongitudinally polarized case S̄μ ≈ δ

μ+ S̄+ , the Ψ -term vanishes for

the relevant component μν = + j. By performing Fourier transfor-mations, we find

〈P ′ S ′|ψ̄(0)γ +∫

dy− K(

y−)W0y g F + j(y−)

W−y0ψ(0)|P S〉

= i P̄+∫

dx1 dx2 K(x1 − x2)T + j(x1, x2)

= iε jk S̄+�k

∫dX dxK(x)Φ(X, x, ξ), (23)

where we switched to the notation X = x1+x22 , x = x1 − x2. The

kernel is

K(x) = p.v.1

x= 1

2

(1

x + iε+ 1

x − iε

), (24)

in the case K(y−) = 12 ε(y−) and

K(x) = 1

x ± iε, (25)

in the cases K(y−) = ±θ(±y−). Comparing with (20), we obtainan alternative expression for the potential angular momentum

Lpot =∫

dX dxK(x)Φ(X, x,0). (26)

Note that, since Φ(X,0,0) = 0, different choices for K lead to thesame result, as they should.

4. Canonical angular momentum

Next we exploit the relation between the twist-three approachto the SSA and the approach based on the transverse momentumdependent distribution (TMD).4 In the longitudinally polarized andnon-forward case, we define

f (x,qT ,�) ≡∫

dz− d2zT

(2π)3eixP̄+z−−iqT ·zT

× 〈P ′ S ′|ψ̄(−z−/2,−zT /2)γ +W−

−z2 ,±∞

×W T−zT2 ,

zT2W−

±∞, z2ψ

(z−/2, zT /2

)|P S〉, (27)

where W T is the Wilson line in the transverse direction atx− = ±∞. In the forward case � = 0, the matrix element (27)reduces to the usual TMD. As is well known in that context,there is freedom in choosing the path connecting the points(−z−/2,−zT /2) → (z−/2, zT /2). Using the Wilson line that goesto future infinity and then comes back −z−/2 → +∞ → z−/2,one takes care of the final state interaction. The TMD in thiscase is relevant to the semi-inclusive DIS (SIDIS). The other case

4 The following discussion is similar to the works of Refs. [22,16]. We improveupon these works by fully taking into account the gauge field and the issue of gaugeinvariance.

Y. Hatta / Physics Letters B 708 (2012) 186–190 189

−z−/2 → −∞ → z−/2 includes the initial state interaction rele-vant to the Drell–Yan process. For the present purpose, one may aswell take the average of the two cases.

The relation between (27) and (20) is revealed by taking thesecond moment of f in qT [23]5

F i(x,�) ≡∫

d2qT qiT f (x,qT ,�)

= 1

2

∫dz−

2πeixP̄+z−

{〈P ′ S ′|ψ̄(−z−/2

)γ +

(W−

−z2 , z

2i−→D i − i

←−D iW−

−z2 , z

2

(z−/2

)|P S〉− 〈P ′S ′|ψ̄(−z−/2

)γ +

×∫

dy−(K

(y− − z−/2

) +K(

y− + z−/2))

×W−−z2 ,y

g F +i(y−)W−

y, z2ψ

(z−/2

)|P S〉}, (28)

where the kernel K is in one-to-one correspondence with thechoice of the Wilson line path in (27). In the forward case, (28)vanishes for the longitudinal polarization by rotational symmetryin the transverse plane. In the non-forward case, however, the fol-lowing structure

f (x,qT ,�) ∼ i

P̄+ ε+−i j S̄+qT i� j f̃(x,q2

T , ξ,�T · qT), (29)

is allowed, so that (28) is not necessarily zero. Note that, becauseof an extra minus sign from � j under the PT transformation, thefunction f̃ does not change signs when changing the directions ofthe Wilson line,6 in contrast to the known sign flip of the spin-dependent TMDs in the SIDIS and Drell–Yan reactions [24].

We then take the first moment in x∫dx F i(x,�) = 1

P̄+

{1

2〈P ′ S ′|ψ̄(0)γ +(

i−→D i − i

←−D i)ψ(0)|P S〉

− 〈P ′S ′|ψ̄(0)γ +∫

dy− K(

y−)W−

0y

× g F +i(y−)W−

y0ψ(0)|P S〉}

= 1

P̄+

{1

2〈P ′ S ′|ψ̄(0)γ +(

i−→D i − i

←−D i)ψ(0)|P S〉

+ 〈P ′S ′|ψ̄(0)γ + Aiphysψ(0)|P S〉

}

= 1

2 P̄+ 〈P ′ S ′|ψ̄(0)γ +(i−→D i

pure − i←−D i

pure

)ψ(0)|P S〉.

(30)

The matrix element (20) indeed appears in the second term of thefirst equality, but somewhat remarkably, it is absorbed by the co-variant derivative in the first term. The final expression featuresprecisely the ‘pure gauge’ part of the covariant derivative Dpure.Differentiating with respect to �, we arrive at

5 Cf. Eq. (39) of [23]. Via partial integration, qiT is replaced by the spatial deriva-

tive ∂ iT . When acting on the Wilson line, it brings down the factor ∂ i

T A+ = D+ Ai +F i+ which reduces to the two terms in (28).

6 More precisely, f̃ (x,q2T , ξ,�T ·qT ) → + f̃ (x,q2

T ,−ξ,−�T ·qT ) after changing thedirections. But the difference is immaterial in the limit � → 0.

ε i j Lcan = 1

2P+ lim�→0

i∂�i

× 〈P ′ S ′|ψ̄(0)γ +(i−→D j

pure − i←−D j

pure)ψ(0)|P S〉

= lim�→0

i∂�i

∫dx F j(x,�)

= lim�→0

i∂�i

∫dx d2qT q j

T f (x,qT ,�)

= ε i j S+

P+1

2

∫dx d2qT q2

T f̃(x,q2

T

). (31)

This is a formula relating the canonical OAM of quarks to thematrix element of a well-defined, manifestly gauge invariant oper-ator.7 The final expression in (31) agrees with the OAM constructedby Lorcé and Pasquini [16] from the Wigner distribution (neglect-ing gauge invariance). We have thus established a gauge invariantlink between the Wigner distribution approach and the spin de-composition framework of Chen et al.

Similarly, for the gluon orbital angular momentum one can de-fine

g(x,qT ,�) ≡ −i

∫dz− d2zT

(2π)3eixP̄+z−−iqT ·zT

× 〈P ′ S ′|F +α(−z−/2,−zT /2

)W−

−z2 ,±∞

×W T−zT2 ,

zT2W−

±∞, z2

Aphysα

(z−/2, zT /2

)|P S〉, (32)

where Aphys is as in (11), and now the Wilson lines are in theadjoint representation. Under the PT transformation, one gets thesame operator back (up to the direction of the Wilson line) pro-vided the skewness parameter ξ vanishes, which we assume here.In deeply virtual Compton scattering (DVCS), ξ = 0 corresponds tothe elastic scattering of the photon.

Proceeding as before, one finds the double moment in x and qT∫dx d2qT qi

T g(x,qT ,�)

= 1

2 P̄+ 〈P ′S ′|F +α(−→

D ipure − ←−

D ipure

)Aphys

α |P S〉. (33)

The matrix element of (7) thus becomes

1

2P+〈P S| ∫ dx− d2xT M+i j

gluon-orbit|P S〉(2π)3δ3(0)

= lim�→0

i∂�i

∫dx d2qT q j

T g(x,qT ,�)

= ε i j S+

P+1

2

∫dx d2qT q2

T g̃(x,q2

T

), (34)

where we parameterized, as � → 0,

g(x,qT ,�) = i

P̄+ ε+−i j S̄+qT i� j g̃(x,q2

T

) + · · · . (35)

5. Conclusions

We have shown that the physical part of the gauge field Aphysproposed in [10] leads to well-defined expressions for the canoni-cal and potential angular momenta in terms of the matrix elementof certain gauge invariant operators. If one defines �G as the gluonhelicity, consistency requires that (31) is the corresponding canon-ical angular momentum. Now that we can, at least in principle,

7 We note that a possible UV regularization of the qT -integral (31) and its evolu-tion requires an entirely separate analysis.

190 Y. Hatta / Physics Letters B 708 (2012) 186–190

measure LJi , Lcan and the difference Lpot = LJi − Lcan separately, itseems more legitimate to call Lcan, or equivalently the OAM fromthe Wigner distribution [16,25], the quarks’ genuine orbital angularmomentum since it satisfies the fundamental commutation rela-tion.

Regarding measurability, it should be possible to compute (31)in lattice QCD simulations as in the case of the ordinary (forward)TMD (see, e.g., [26]). Since there is no sign flip in (27) when chang-ing the directions of the Wilson lines, the matrix element may notbe very sensitive to the choice of the path. If so, and if one is notinterested in the x-dependence, one may first integrate over x in(27) and connect the quark operators (at the same value of z− = 0)by a purely spatial Wilson line in the transverse plane. This avoidsthe introduction of lightlike Wilson lines on a Euclidean latticewhich appears to be a vague issue. For the gluon orbital angu-lar momentum (34) with g defined in (32), one has to deal withlightlike Wilson lines even after the x-integration.

Finally, from the experimental point of view, the matrix ele-ments such as (22) are related to the twist-three GPDs [27,28]which are hard to extract. It would be interesting to see if thereare processes in which these functions contribute to the cross sec-tion at leading order as in the single spin asymmetry.

Acknowledgements

I am indebted to Kazuhiro Tanaka for many discussions, and forreading the manuscript and bringing [22] to my attention. I alsothank Terry Goldman, Yuji Koike and Jian-Wei Qiu for helpful con-versations and correspondence. This work is supported by SpecialCoordination Funds for Promoting Science and Technology of theMinistry of Education, the Japanese Government.

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