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Rethinking the dynamical paradigm of low-mass stellar systems

重新思考低质量恒星系统的动力学范式

基本信息

批准号：
MR/S018859/1
负责人：
Anna Lisa Varri
金额：
$ 82.67万
依托单位：
University of Edinburgh
依托单位国家：
英国
项目类别：
Fellowship
财政年份：
2019
资助国家：
英国
起止时间：
2019 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=MR%2FS018859%2F1
关键词：
Rethinking dynamical paradigm low mass

项目摘要

All large galaxies, including our own Milky Way, contain hundreds of 'globular clusters'. Each is a dense group of about a million stars held together by their mutual gravitational attraction. Through a mathematician's eye, they correspond to the deep-rooted problem of understanding the motion of N bodies interacting by long-range forces. Through an astronomer's telescope, they appear as local relics of the ancient universe, as they were among the first stellar structures to emerge at the dawn of the formation of galaxies. Observational astronomers have studied star clusters for decades, but in recent years the quality and range of these observations has leapt beyond the range of existing theory. In particular, the European space observatory Gaia is now measuring the positions and the velocities of thousands of stars in globular clusters of our Galaxy, with unprecedented accuracy. This new generation of data, coupled with measurements by the Hubble Space Telescope and other state-of-the-art and forthcoming astronomical facilities, enable theorists to explore, for the first time, the full 'phase space' of star clusters by studying both the position and velocity of their individual stars.Theorists' models are based on simplifying assumptions, and at present almost always include the ideas that the clusters are spherical, do not rotate, and are composed only of stars - all born at the same time. Three recent developments are undermining these assumptions and requiring us to treat the clusters as they are, and not as we would wish them to be: (i) the realisation that the motions of their stars is much more complex than we expected and that their internal rotation is the rule rather than the exception; (ii) the empirical evidence that the stars in clusters were not all born at once in a single population (an assumption which was once part of their very definition); and (iii) the recent discovery of a numerous 'hybrid' stellar systems which now makes arduous to trace the distinction between 'star clusters' and 'dwarf galaxies'. In addition, star clusters have recently been recognised as prolific cradles for small, 'stellar-mass', black holes and they have been long speculated to be the ideal birth site of larger, 'intermediate-mass', ones. Currently undetected, this class of astrophysical objects is a crucial missing link in the population of cosmic black holes. But new facilities such as the Laser Interferometer Gravitational-Wave Observatory and the Kamioka Gravitational Wave Detector will soon help us tackle this open problem from a new perspective. With a combination of mathematical techniques and numerical simulations, I aim to propose a more realistic description of the dynamics of star clusters, to interpret such new-generation astronomical data. As a result, this research programme will allow me to address three open problems in modern astrophysics: the origin of stars which are among the oldest in the universe, the possible existence a 'missing link' in the population of cosmic black holes, and the limits of the presence of invisible 'dark' matter in small stellar systems.A fundamental understanding of the history and evolution of these intriguing stellar systems will, therefore, provide a new perspective on the first building blocks of galaxies and on the origin of our Milky Way.

所有的大型星系，包括我们的银河系，都包含数百个“球状星团”。每一个都是由大约一百万颗恒星组成的密集群，它们通过相互的引力吸引在一起。通过数学家的眼睛，它们对应于理解N个物体在长程力作用下的运动的根深蒂固的问题。通过天文学家的望远镜，它们似乎是古代宇宙的局部遗迹，因为它们是星系形成初期出现的第一批恒星结构。观测天文学家几十年来一直在研究星星团，但近年来这些观测的质量和范围已经超越了现有理论的范围。特别是，欧洲空间观测站盖亚现在正在以前所未有的精度测量我们银河系球状星团中数千颗恒星的位置和速度。这些新一代的数据，加上哈勃太空望远镜和其他最先进的天文设备的测量，使理论家能够通过研究单个恒星的位置和速度，第一次探索星星团的完整“相空间”。理论家的模型是基于简化的假设，目前几乎总是包括这样的想法，即星团是球形的，它们不旋转，只由恒星组成--它们都是同时诞生的。最近的三个发展破坏了这些假设，并要求我们按照星团的实际情况来对待它们，而不是按照我们所希望的那样来对待它们：（i）认识到它们的恒星的运动比我们预期的要复杂得多，它们的内部旋转是规则而不是例外;（ii）星团中的恒星并非同时在一个种群中诞生的经验证据（一个假设，这是曾经的一部分，他们的定义）;（iii）最近发现的许多'混合'恒星系统，现在很难跟踪之间的区别'星星集群'和'矮星系'。此外，星星团最近被认为是小型、“恒星质量”黑洞的多产摇篮，长期以来一直被推测是较大、“中等质量”黑洞的理想诞生地。目前未被发现的这类天体是宇宙黑洞种群中重要的缺失环节。但是，激光干涉引力波天文台和神冈引力波探测器等新设施将很快帮助我们从一个新的角度解决这个悬而未决的问题。通过结合数学方法和数值模拟，我的目标是提出一个更真实的描述星星集群的动态，解释这样的新一代天文数据。因此，这项研究计划将使我能够解决现代天体物理学中的三个开放问题：宇宙中最古老的恒星的起源，宇宙黑洞群中可能存在的“缺失环节”，以及小恒星系统中不可见的“暗”物质存在的极限。对这些有趣的恒星系统的历史和演化的基本理解将，因此，提供了一个新的视角，对星系的第一个积木和我们的银河系的起源。