arXiv · hep-ph/9808202
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: $L_q(x)={ }Δq_{QM}(x)$. The quark orbital angular momentum $L_q(x)$ and the quark helicity distribution $Δq(x)$ are connected to the quark model spin distribution $Δq_{QM}(x)$ by a relation: $\frac{1}{2}Δq(x)+ L_q(x)=\frac{1}{2}Δq_{QM}(x)$, which means that one can decompose the quark model spin contribution $Δq_{QM}(x)$ by a quark helicity term $Δq(x)$ {\it plus} an orbital angular momentum term $L_q(x)$. There is also a new relation connecting the quark orbital angular momentum with the measurable quark helicity distribution and transversity distribution ($δq(x)$): $Δq(x)+L_q(x)=δq(x)$, from which we may have new sum rules connecting the quark orbital angular momentum with the nucleon axial and tensor charges.
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Bo-Qiang Ma, Ivan Schmidt. 1998-08-02. The Quark Orbital Angular Momentum in a Light-Cone Representation. https://doi.org/10.1103/physrevd.58.096008
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