Phys. Rev. D 58, 096008 (1998) [7 pages]

Quark orbital angular momentum in a light-cone representation

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Bo-Qiang Ma *
CCAST (World Laboratory), P.O. Box 8730, Beijing 100080, China
Institute of High Energy Physics, Academia Sinica, P.O. Box 918(4), Beijing 100039, China

Ivan Schmidt
Departamento de Física, Universidad Técnica Federico Santa María, Casilla 110-V, Valparaíso, Chile

Received 18 May 1998; published 5 October 1998

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)=〈ML(x)〉ΔqQM(x). The quark orbital angular momentum Lq(x) and the quark helicity distribution Δq(x) are connected to the quark model spin distribution ΔqQM(x) by a relation 1 / 2Δq(x)+Lq(x)=1 / 2ΔqQM(x), which means that one can decompose the quark model spin contribution ΔqQM(x) by a quark helicity term Δq(x) plus an orbital angular momentum term Lq(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)+Lq(x)=δq(x), from which we may have new sum rules connecting the quark orbital angular momentum with the nucleon axial and tensor charges.


©1998 The American Physical Society

URL: http://link.aps.org/abstract/PRD/v58/e096008
DOI: 10.1103/PhysRevD.58.096008
PACS: 11.55.Hx, 13.60.Hb, 13.88.+e, 14.20.Dh

* Email address: mabq@bepc3.ihep.ac.cn
Email address: ischmidt@fis.utfsm.cl

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