论文标题
从重离子碰撞到中子星的状态方程式的未来物理学观点
Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars
论文作者
论文摘要
借助当今可用的计算能力和算法改进，正在进行的星/rhic和Hades/GSI实验，未来的公平和NICA设施开始运行，以及从更好的和Ligo/Wigo中的新精确测量，高能核物理学和天体物理学社区具有非常严格的相互作用的位置。我们回顾了在均衡中和超高的重型重质物质描述中使用的不同方法的最新方法，并在相图中讨论了重合离子碰撞和中子星兼合并可以重叠的区域中的区域。讨论了未来的观点，以帮助定义一种全面的多学科策略，以绘制从重离子碰撞到中子恒星的强烈相互作用物质的相图。
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.
