从重离子碰撞到中子星状态方程的未来物理学展望

V. Dexheimer, J. Noronha, J. Noronha-Hostler, N. Yunes, C. Ratti
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引用次数: 33

摘要

随着今天计算能力和算法的改进,正在进行的STAR/RHIC和HADES/GSI实验,未来的FAIR和NICA设施开始运行,以及来自NICER和LIGO/VIRGO的新的精确测量,高能核物理学界和天体物理学界处于独特的位置,可以对强相互作用物质的状态方程设置非常严格的约束。我们回顾了用于描述处于和非平衡状态的高温和超密集重子物质的不同方法的最新进展,并讨论了相图中重离子碰撞和中子星合并可以重叠的区域。讨论了未来的观点,以帮助定义一个全面的,多学科的策略来绘制从重离子碰撞到中子星的强相互作用物质的相图。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars
With the computational power and algorithmic improvements available today, the ongoing STAR/RHIC and HADES/GSI experiments, the future FAIR and NICA facilities becoming operational, and the new precise measurements from NICER and LIGO/VIRGO, the high-energy nuclear physics and astrophysics communities are in the unique position to set very stringent constraints on the equation of state of strongly interacting matter. We review the state-of-the-art of different approaches used in the description of hot and ultradense baryonic matter in and out of equilibrium, and discuss the regions in the phase diagram where heavy-ion collisions and neutron star mergers can overlap. Future perspectives are discussed to help define a comprehensive, multi-disciplinary strategy to map out the phase diagram of strongly interacting matter from heavy ion collisions to neutron stars.
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