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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