次领头阶的极化重夸克光产生
高能物理 - 唯象学
2017-08-23 v1
摘要
我们给出了纵向极化重夸克光产生的次领头阶解析计算结果。针对CERN和HERA可达到的能量范围，计算了某些微分截面和相应的不对称度。我们认为在这两个地方都有可能确定极化胶子分布：在HERA需要某些接受度截断。
引用
@article{arxiv.hep-ph/9911506,
title = {Polarized Heavy Quark Photoproduction in Next to Leading Order},
author = {Z. V. Merebashvili and A. P. Contogouris and G. Grispos},
journal= {arXiv preprint arXiv:hep-ph/9911506},
year = {2017}
}
备注
6 pages, 3 figures, invited talk given at the Int. Workshop "Symmetry and Spin. Praha-Spin99", 5-12 Sept. 1999, Prague, to appear in proceedings