论文标题
巴里昂结构在中子星中的作用
The Role of Baryon Structure in Neutron Stars
论文作者
论文摘要
了解密集核物质状态的方程是核物理学的基本挑战。这是尤其是及时，有趣的挑战，因为我们已经达到了一个时期，即中子恒星（其中包含宇宙中最密集的核物质）现在正在以全新的方式进行研究，从引力波到基于卫星的望远镜。我们回顾了计算该状态方程的理论方法，该方程涉及重生子的结构。
Understanding the equation of state of dense nuclear matter is a fundamental challenge for nuclear physics. It is especially timely and interesting challenge as we have reached a period where neutron stars, which contain the most dense nuclear matter in the Universe, are now being studied in completely new ways, from gravitational waves to satellite based telescopes. We review the theoretical approaches to calculating this equation of state which involve a change in the structure of the baryons.
