中能重离子碰撞中核子-核子散射的自旋极化

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Rong-Jun Liu , Jun Xu , Yu-Gang Ma
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引用次数: 0

摘要

提出了一种以核子自由度为主导的重离子碰撞产生自旋极化的新机制。通过结合基于相移数据的核子-核子散射中的自旋变化以及严格角动量守恒和泡利阻挡的约束,我们通过Boltzmann-Uehling-Uhlenbeck输运模型说明,在中能重离子碰撞中可以产生可观的自旋极化(约1 ~ 2%)。这一机制与核自旋轨道势可能有助于理解以核子自由度为主导的低gev重离子碰撞中的自旋极化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spin polarization from nucleon-nucleon scatterings in intermediate-energy heavy-ion collisions
We propose a new mechanism of generating spin polarization in heavy-ion collisions dominated by nucleon degree of freedom. By incorporating the spin change in nucleon-nucleon scatterings based on the phase shift data together with the constraint of rigorous angular momentum conservation and Pauli blocking, we illustrate through a Boltzmann-Uehling-Uhlenbeck transport model that appreciable spin polarization (about 12%) can be generated in intermediate-energy heavy-ion collisions. This mechanism, together with the nuclear spin-orbit potential, may help to understand the spin polarization in few-GeV heavy-ion collisions dominated by nucleon degree of freedom.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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