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The Quark Orbital Angular Momentum in a Light-Cone Representation

Abstract

We perform an analysis of the quark angular momentum in a light-cone representation by taking into account the effect due to the Melosh-Wigner rotation and find that there is a relativistic correction factor connecting the quark orbital angular momentum with the quark model spin distribution: Lq(x)=ΔqQM(x)L_q(x)={}\Delta q_{QM}(x). The quark orbital angular momentum Lq(x)L_q(x) and the quark helicity distribution Δq(x)\Delta q(x) are connected to the quark model spin distribution ΔqQM(x)\Delta q_{QM}(x) by a relation: 12Δq(x)+Lq(x)=12ΔqQM(x)\frac{1}{2}\Delta q(x)+ L_q(x)=\frac{1}{2}\Delta q_{QM}(x), which means that one can decompose the quark model spin contribution ΔqQM(x)\Delta q_{QM}(x) by a quark helicity term Δq(x)\Delta q(x) {\it plus} an orbital angular momentum term Lq(x)L_q(x). There is also a new relation connecting the quark orbital angular momentum with the measurable quark helicity distribution and transversity distribution (δq(x)\delta q(x)): Δq(x)+Lq(x)=δq(x)\Delta q(x)+L_q(x)=\delta q(x), from which we may have new sum rules connecting the quark orbital angular momentum with the nucleon axial and tensor charges.Comment: 20 latex pages, including an eps figure, to appear in Phys. Rev.

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