RHIC上$\sqrt(s)$ = 500 GeV极化pp对撞的STAR W自旋物理计划
核实验
2019-08-13 v1
摘要
在纵向极化pp对撞中产生W玻色子为探测极化质子中海夸克极化的味依赖性提供了一个极好的工具。本文介绍了RHIC上STAR探测器的W物理计划的现状和未来计划，并评论了我们关于部分子海的性质和起源的认识。
引用
@article{arxiv.0907.0797,
title = {The STAR W Spin Physics Program with $\sqrt(s)$ = 500 GeV Polarized pp Collisions at RHIC},
author = {W. W. Jacobs},
journal= {arXiv preprint arXiv:0907.0797},
year = {2019}
}
备注
Talk given at the Tenth Conference on the Intersections of Particle and Nuclear Physics (CIPANP 2009), 26-31 May 2009, San Diego CA, USA; 4 pages, 3 figures