The Extreme Gravity Dynamics and Gravitational Waves of Generic Compact Binary Inspirals

一般致密二元螺旋的极端重力动力学和引力波

基本信息

  • 批准号:
    1949838
  • 负责人:
  • 金额:
    $ 33.96万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2019
  • 资助国家:
    美国
  • 起止时间:
    2019-08-16 至 2022-08-31
  • 项目状态:
    已结题

项目摘要

Gravitational wave astrophysics has entered a new era of discovery and exploration, with the Nobel-Prize-earning, first detections of gravitational waves by the advanced LIGO and advanced Virgo ground-based observatories. One of the key missions of LIGO and Virgo is to test Einstein's theory of General Relativity where it has never been tested before: where the gravitational force is enormous and violently changing. Gravitational waves encode invaluable information about this extreme gravity regime, especially in the waves produced when black holes and neutron stars collide. The main objective of this award is to develop ready-to-use models to extract and interpret gravitational waves emitted in eccentric and precessing collisions, so that these models can be used to study astrophysics and test General Relativity with future observations. This research will be integrated with broader impact activities aimed at changing the attitudes of K-12 students and the general public toward physics and science through activities that will be developed in the eXtreme Gravity Institute at Montana State University, a fertile training ground for the next generation of scientists. This project is aimed at (i) the development of analytic, ready-to-use models for the orbital dynamics and gravitational waves emitted in the late inspiral of generic compact binaries (black hole and neutron star binaries with arbitrary spin and eccentricity), and (ii) the use of these models to analyze and interpret current and future ground-based gravitational wave data to study astrophysics and experimental relativity implications. The gravitational wave models used currently are restricted to (at most nearly) quasi-circular inspirals with (typically) spins aligned/anti-aligned with the orbital angular momentum (or to simple-precession-like approximations). Such models are sufficient for the detection and characterization of current GW observations, but as advanced LIGO is upgraded to reach design sensitivity and third-generation detectors are constructed, more accurate models will be needed. Not only will these models prevent the biasing of parameter estimation due to mis-modeling systematics, but the additional information they encode will allow for more accurate parameter estimation and the extraction of new information from the data. This new information, such as the orbital eccentricity and the spin vector components, can inform astrophysical population models, as well as allow for new tests of General Relativity in the mostly-unexplored, extreme gravity regime. The proposed research includes the implementation of the ready-to-use models in data analysis studies to determine the astrophysics and experimental-relativity information that can be extracted from current and future gravitational wave data. This research will be integrated with broader impact activities aimed at changing the attitudes of K-12 students and the general public toward physics and science. "The Art of Physics" activity is an art competition and residency program in the Department of Physics at MSU, in which undergraduate students will be educated in cutting-edge physics and create art works that convey its concepts. The art pieces will compete at a juried exhibition, with the winning artist becoming the resident artist in physics for the next year. The "Learn to Fail" activity is an art installation in which Montana State University faculty will share their failure stories with the MSU student population and general public on camera while contrasting their biggest achievements. Through this juxtaposition between failures and successes, the installation will generate an honest dialogue about the role and meaning of failure in academia. "eXtreme Gravity for Middle School? are fully-formed, standards-aligned lesson plans for middle school teachers aimed at supporting them in learning how to deliver content on topics including gravitational lensing, neutron stars, black holes and gravitational waves to middle school students. Other activities include a black-hole themed bout for the local roller derby team, public talks given by the PI, and continued STEM mentoring for middle-school students from local schools.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
引力波天体物理学进入了一个新的发现和探索时代,诺贝尔·普里尔(Nobel-Pribe)读取了先进的Ligo和先进的处女座地面观测值对引力波的首次检测。 Ligo和处女座的关键任务之一是测试爱因斯坦的一般相对论理论,从未对其进行过测试:重力巨大且剧烈变化。引力波编码有关这种极端重力状态的宝贵信息,尤其是在黑洞和中子星相撞时产生的波。该奖项的主要目的是开发现成的模型,以提取和解释在偏心和进攻碰撞中发出的引力波,以便这些模型可用于研究天体物理学并测试与未来观察结果的一般相对性。这项研究将与旨在通过将在蒙大拿州立大学极端重力研究所开发的活动来改变旨在改变K-12学生和公众对物理和科学的态度的更广泛的影响活动,这是下一代科学家的肥沃培训场。该项目的目的是(i)开发在通用紧凑型二进制二进制的后期灵感中发出的轨道动力学和引力波的分析,现成的模型(黑洞和中子星形二进制二进制型,具有任意旋转和偏心率),以及(ii)这些模型的使用来分析和解释当前和未来的Graveration Gractitation sellistion contriptication contrictication controptical resistications resistications contropticalssics and trastorys saltersics and tastorrations saltorpations saltersics和实验。当前使用的引力波模型仅限于(最多几乎)的准圆形灵感,其旋转与轨道角动量(或简单明显的近似值)对齐/抗对齐。这样的模型足以检测和表征当前的GW观测值,但是由于高级LIGO升级以达到设计敏感性,并构建了第三代探测器,因此需要更准确的模型。这些模型不仅会由于错误模型系统的系统而阻止参数估计的偏置,而且它们编码的其他信息将允许更准确的参数估计以及从数据中提取新信息。这些新信息,例如轨道偏心率和自旋矢量成分,可以为天体物理人群模型提供信息,并允许在大多数未阐明的极端重力制度中进行一般相对论的新测试。拟议的研究包括在数据分析研究中实施现成的模型,以确定可以从当前和将来的重力波数据中提取的天体物理学和实验率信息。这项研究将与旨在改变K-12学生和公众对物理和科学的公众态度的更广泛的影响活动相结合。 “物理艺术”活动是MSU物理学系的艺术竞争和居住计划,其中本科生将接受尖端物理学的教育,并创建传达其概念的艺术作品。艺术作品将在一个评审展览中竞争,获奖艺术家将成为明年物理学的常驻艺术家。 “学会失败”活动是一种艺术装置,蒙大拿州立大学教师将与MSU学生群体和公众在相机上分享他们的失败故事,同时与他们最大的成就进行对比。通过失败与成功之间的这种并置,该装置将就学术界失败的作用和含义产生诚实的对话。 “中学的极端引力吗?是针对中学老师的完整,标准一致的课程计划,旨在支持他们学习如何在包括重力镜头,中子明星,黑洞,黑洞和引力浪潮在内的主题上交付内容,向中学生提供其他活动。其他活动。 NSF的法定使命,并使用基金会的知识分子优点和更广泛的影响审查标准来评估值得支持。

项目成果

期刊论文数量(19)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
More than the sum of its parts: Combining parametrized tests of extreme gravity
不仅仅是各个部分的总和:结合极端重力的参数化测试
  • DOI:
    10.1103/physrevd.100.084034
  • 发表时间:
    2019
  • 期刊:
  • 影响因子:
    5
  • 作者:
    Silva, Hector O.;Yunes, Nicolás
  • 通讯作者:
    Yunes, Nicolás
Probing fundamental physics with gravitational waves: The next generation
  • DOI:
    10.1103/physrevd.103.044024
  • 发表时间:
    2020-10
  • 期刊:
  • 影响因子:
    5
  • 作者:
    S. Perkins;N. Yunes;E. Berti
  • 通讯作者:
    S. Perkins;N. Yunes;E. Berti
Structure of the singular ring in Kerr-like metrics
类克尔度量中奇异环的结构
  • DOI:
    10.1103/physrevd.101.104048
  • 发表时间:
    2020
  • 期刊:
  • 影响因子:
    5
  • 作者:
    Chruściel, Piotr T.;Maliborski, Maciej;Yunes, Nicolás
  • 通讯作者:
    Yunes, Nicolás
Prospects for fundamental physics with LISA
LISA 基础物理的前景
  • DOI:
    10.1007/s10714-020-02691-1
  • 发表时间:
    2020-08-31
  • 期刊:
  • 影响因子:
    2.8
  • 作者:
    Barausse, Enrico;Berti, Emanuele;Zumalacarregui, M.
  • 通讯作者:
    Zumalacarregui, M.
Numerical black hole solutions in modified gravity theories: Axial symmetry case
修正引力理论中的数值黑洞解:轴对称情况
  • DOI:
    10.1103/physrevd.103.124058
  • 发表时间:
    2021
  • 期刊:
  • 影响因子:
    5
  • 作者:
    Sullivan, Andrew;Yunes, Nicolás;Sotiriou, Thomas P.
  • 通讯作者:
    Sotiriou, Thomas P.
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Nicolas Yunes其他文献

液体ヘリウムを用いた軽い暗黒物質探索用超伝導検出器(LEKID)の開発(2)
开发使用液氦寻找光暗物质的超导探测器 (LEKID) (2)
  • DOI:
  • 发表时间:
    2016
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Nicholas Loutrel;Takahiro Tanaka;Nicolas Yunes;喜田洋介
  • 通讯作者:
    喜田洋介
Scalar Tops and Perturbed Quadrupoles: Probing Fundamental Physics with Spin-Precessing Binaries
标量顶和扰动四极杆:用自旋进动双星探索基础物理
  • DOI:
  • 发表时间:
    2019
  • 期刊:
  • 影响因子:
    3.5
  • 作者:
    Nicholas Loutrel;Takahiro Tanaka;Nicolas Yunes
  • 通讯作者:
    Nicolas Yunes
月のこよみ2014
月光 2014
  • DOI:
  • 发表时间:
    2013
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Hong Liu;Hirosi Ooguri;Bogdan Stoica;Nicolas Yunes;相馬充 (監修)
  • 通讯作者:
    相馬充 (監修)

Nicolas Yunes的其他文献

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{{ truncateString('Nicolas Yunes', 18)}}的其他基金

Probing Extreme Gravity with Gravitational Waves
用引力波探测极端重力
  • 批准号:
    2207650
  • 财政年份:
    2022
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Continuing Grant
Frameworks: MUSES, Modular Unified Solver of the Equation of State
框架:MUSES,状态方程的模块化统一求解器
  • 批准号:
    2103680
  • 财政年份:
    2021
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Standard Grant
WoU-MMA: Collaborative Research: Gravitational wave cosmology with tidal Love numbers
WoU-MMA:合作研究:引力波宇宙学与潮汐洛夫数
  • 批准号:
    2009268
  • 财政年份:
    2020
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Standard Grant
The Extreme Gravity Dynamics and Gravitational Waves of Generic Compact Binary Inspirals
一般致密二元螺旋的极端重力动力学和引力波
  • 批准号:
    1759615
  • 财政年份:
    2018
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Continuing Grant
Extreme Gravity Workshop to be held at Montana State University; August 20-22, 2015.
极端重力研讨会将在蒙大拿州立大学举行;
  • 批准号:
    1522783
  • 财政年份:
    2015
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Standard Grant
CAREER: Gravitational Waves from Compact Binaries as Probes of the Universe
职业:作为宇宙探测器的致密双星引力波
  • 批准号:
    1250636
  • 财政年份:
    2013
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Continuing Grant
Travel Support for Workshop on Gravitational Wave Tests of Alternative Theories of Gravity in the Advanced Detector Era at Montana State University April 5-7, 2013
2013 年 4 月 5 日至 7 日在蒙大拿州立大学举办的高级探测器时代替代重力理论​​的引力波测试研讨会的差旅支持
  • 批准号:
    1234826
  • 财政年份:
    2012
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Standard Grant
Probing Strong Gravity with Gravitational Waves
用引力波探测强引力
  • 批准号:
    1114374
  • 财政年份:
    2011
  • 资助金额:
    $ 33.96万
  • 项目类别:
    Standard Grant

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Collaborative Research: Probing internal gravity wave dynamics and dissipation using global observations and numerical simulations
合作研究:利用全球观测和数值模拟探测内部重力波动力学和耗散
  • 批准号:
    2319142
  • 财政年份:
    2023
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    Standard Grant
Collaborative Research: Probing internal gravity wave dynamics and dissipation using global observations and numerical simulations
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  • 批准号:
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基于不同引力场类比的塑料3D打印机性能提升
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Collaborative Research: Probing internal gravity wave dynamics and dissipation using global observations and numerical simulations
合作研究:利用全球观测和数值模拟探测内部重力波动力学和耗散
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