NEW APPLICANT: Enabling rapid observation of compact binary mergers with a network of gravitational-wave observatories

新申请人：利用引力波观测站网络快速观测紧凑型双星合并

• 批准号: ST/T000333/1
• 负责人: Ian Harry
• 金额: $ 27.25万
• 依托单位: University of Portsmouth
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2020
• 资助国家: 英国
• 起止时间: 2020 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FT000333%2F1
• 关键词: NEW; APPLICANT; Enabling; rapid; observation

Gravitational waves are one of the most remarkable predictions of Einstein's General Theory of Relativity. These can be thought of as ripples in the fabric of spacetime propagating at the speed of light. Gravitational waves are emitted by non-spherically symmetric accelerated masses, such as two black holes or neutron stars orbiting each other. Gravitational waves are incredibly difficult to detect, but in the last years large-scale observatories, including Advanced LIGO, Advanced Virgo and KAGRA, have reached the necessary sensitivity to observe gravitational waves.The first gravitational-wave signal observed in September 2015 was produced by two black holes roughly 35 times the mass of our Sun colliding approximately one billion light years away. Since then nine additional binary black hole mergers have been observed. The crowning achievement of gravitational-wave astronomy to date was the observation of two merging neutron stars in August 2017. This signal was special because it was observed simultaneously as a gamma-ray burst by the Fermi observatory and then, following the release of the gravitational-wave sky localization region to astronomers, was observed across the electromagnetic spectrum.The potential of "multi-messenger" astronomy-observing sources with multiple "messengers", such as gravitational-waves, photons, neutrinos or cosmic rays-is remarkable. We can explore the validity of Einstein's theory in one of the most extreme environments possible. We can make an independent measurement of the rate at which the Universe is accelerating. We can probe the nature of matter deep within a neutron star, where it is so dense that 1 teaspoon of material weighs as much as a mountain on the Earth.However, all of this requires us to actually observe these gravitational-wave signals, and to do it quickly enough that we can alert external astronomers to search for a coincident signal. In this grant we will develop methods to promptly search data from Advanced LIGO, Advanced Virgo and KAGRA to observe the gravitational-wave signature of merging compact objects. We will ensure that such observations are rapidly localized on the sky and that this information is rapidly communicated to external observers. We will also develop techniques to further improve the sensitivity of these searches, allowing us to dig deeper into the noise, and to observe new types of compact binary mergers that have not been observed to date.We will also exploit the astrophysical potential of our observations. We will investigate if double black hole systems form from binary star systems, where both stars have gone through a supernova resulting in a pair of orbiting black holes, or if the two black holes formed in isolation and were later came together as a result of interactions in some dense environment. We will also look to probe the behaviour of matter at the core of neutron stars, one of the most extreme environments in the Universe.

引力波是爱因斯坦的广义相对论中最引人注目的预言之一。这些可以被认为是时空结构中以光速传播的涟漪。引力波是由非球对称的加速质量发射的，例如两个黑洞或中子星相互环绕。引力波是非常难以探测的，但在过去的几年里，包括Advanced LIGO、Advanced Virgo和KAGRA在内的大型天文台已经达到了观测引力波的必要灵敏度。2015年9月观测到的第一个引力波信号是由两个质量约为太阳35倍的黑洞在大约10亿光年外碰撞产生的。从那时起，又观测到了9个双黑洞合并。迄今为止，引力波天文学的最高成就是在2017年8月观测到两颗合并的中子星。这个信号很特别，因为它是费米天文台同时观测到的伽马射线爆发，然后，在向天文学家发布引力波天空定位区域之后，通过电磁波谱观测到的。“多信使”天文学的潜力是显着的，观测具有多个“信使”的源，如引力波，光子，中微子或宇宙射线。我们可以在最极端的环境中探索爱因斯坦理论的有效性。我们可以独立测量宇宙加速的速率。我们可以探测中子星星内部物质的性质，那里的物质密度很大，一茶匙的物质就像地球上的一座山一样重。然而，所有这些都需要我们实际观察这些引力波信号，而且要足够快，以便我们可以提醒外部天文学家寻找一个符合的信号。在这项资助中，我们将开发方法来迅速搜索来自Advanced LIGO，Advanced Virgo和KAGRA的数据，以观察合并紧凑物体的引力波特征。我们将确保这些观测迅速定位在天空中，并将这些信息迅速传达给外部观测者。我们还将开发技术来进一步提高这些搜索的灵敏度，使我们能够更深入地挖掘噪音，并观察到迄今为止尚未观察到的新型紧凑双星合并。我们还将开发我们观测的天体物理潜力。我们将研究双黑洞系统是否由星星系统形成，其中两颗恒星都经历了超新星，导致一对轨道黑洞，或者如果两个黑洞孤立地形成，后来由于在一些稠密环境中的相互作用而聚集在一起。我们还将探索中子星核心的物质行为，这是宇宙中最极端的环境之一。

项目成果

GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

• DOI: 10.1103/physrevd.102.043015
• 发表时间: 2020-08-24
• 期刊: PHYSICAL REVIEW D
• 影响因子: 5
• 作者: Abbott, R.;Abbott, T. D.;Zweizig, J.
• 通讯作者: Zweizig, J.

A Unified $p_\mathrm{astro}$ for Gravitational Waves: Consistently Combining Information from Multiple Search Pipelines

引力波的统一 $p_mathrm{astro}$：一致地组合来自多个搜索管道的信息

• DOI: 10.48550/arxiv.2305.00071
• 发表时间: 2023
• 作者: Banagiri S