Nicolas Yunes领导的研究通过引力波分析,揭示了二进制中子恒星系统中可探测到的平衡性潮汐力量。 Study led by Nicolas Yunes reveals detectable out-of-equilibrium tidal forces in binary neutron star systems through gravitational wave analysis.

伊利诺伊大学城市-坎帕因大学的尼古拉斯·尤恩斯领导的一项研究通过对引力波的分析,揭示了中子星的新特性。 A study led by Nicolas Yunes at the University of Illinois Urbana-Champaign has revealed new properties of neutron stars through the analysis of gravitational waves. 研究显示,在自然天文学中,二进制中子恒星系统中的平衡潮汐力量可以通过这些波浪探测出来,使人们能够洞察到这些波浪的内部粘度。 Published in Nature Astronomy, the research indicates that out-of-equilibrium tidal forces in binary neutron star systems are detectable via these waves, providing insights into their internal viscosity. 这项工作增进了我们对宇宙动态的了解,可以推动未来的技术进步。 This work enhances our understanding of the universe's dynamics and could drive future technological advancements.