Dynamics of compact stars in extreme gravitational fields

极端引力场中致密恒星的动力学

• 批准号: RGPIN-2018-04640
• 负责人: Poisson, Eric
• 金额: $ 3.64万
• 依托单位: University of Guelph
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2020
• 资助国家: 加拿大
• 起止时间: 2020-01-01 至 2021-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=710748
• 关键词: Dynamics; compact; stars; extreme; gravitational

The 2015 discovery of gravitational waves from merging black holes marked the dawn of gravitational wave astronomy, a tremendous scientific development that was rewarded with the 2017 Nobel Prize in physics. Gravitational waves are ripples in the fabric of spacetime, produced by the accelerated motion of massive bodies. Their production requires the most dense objects to be found in the universe, such as neutron stars and black holes, and these objects must move extremely rapidly, which is the case when they form a tight binary system. Their measurement requires large dedicated facilities such as the LIGO and Virgo observatories. The detection of several sources of gravitational waves, involving both black holes and neutron stars, is a great triumph of the LIGO/Virgo collaboration, and the effort is ongoing. Gravitational-wave astronomy opens up a new window onto the universe, to better observe its darkest reaches. The long-term goal of my research is to exploit gravitational-wave astronomy to dramatically improve our understanding of neutron stars and black holes. To reach this goal, my students and I elucidate the physical processes at play when two such objects form a tight binary. For example, a neutron star raises a tide on a companion neutron star, much as the moon raises a tide on Earth, and the tidal deformation affects their orbital motion and the emission of gravitational waves. The tidal imprint on the waves can be measured, and this will reveal intimate details of the physics of neutron stars. This is very exciting, because neutron stars are poorly understood, involving densities of matter that are far beyond what can be found on Earth. As another example, the tidal interaction between two black holes changes the mass and spin of each object, and this can be revealed in the emitted gravitational waves. This also is very exciting, because the tidal effects featured in the waves will reveal some of the black hole's most elusive properties, such as the shape of its event horizon. The goal of this research proposal is to further the study of neutron stars and black holes, so as to better predict the gravitational waves emitted by such objects. To carry this out, my students and I will use the techniques of theoretical physics, manipulating the laws of physics governing black holes, neutron stars, and gravitational waves, so as to extract precise predictions to be shared with the wider scientific community.

2015年黑洞合并引力波的发现标志着引力波天文学的曙光，这是一项巨大的科学发展，并获得了2017年诺贝尔物理学奖。引力波是时空结构中的涟漪，由大质量物体的加速运动产生。它们的产生需要在宇宙中找到密度最大的物体，比如中子星和黑洞，这些物体必须以极快的速度移动，这就是它们形成紧密双星系统的情况。它们的测量需要大型专用设施，如LIGO和处女座天文台。探测到几个引力波源，包括黑洞和中子星，是LIGO/Virgo合作的一个巨大胜利，而且这项工作还在继续。引力波天文学打开了一扇通往宇宙的新窗口，可以更好地观察宇宙最黑暗的部分。