CAREER: Strong Gravitational and Electromagnetic Fields
职业:强引力场和电磁场
基本信息
- 批准号:1752809
- 负责人:
- 金额:$ 40万
- 依托单位:
- 依托单位国家:美国
- 项目类别:Continuing Grant
- 财政年份:2018
- 资助国家:美国
- 起止时间:2018-09-01 至 2024-08-31
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
Our universe abounds with exotic objects that push the familiar phenomena of gravity, electricity, and magnetism to their extremes. Neutron stars have magnetic fields billions of times stronger than the strongest terrestrial magnets and drive electric current through space at more than a trillion volts. The gravity of a black hole is so strong that nothing -not even light- can escape its grip. A variety of astronomical mysteries, from fast radio bursts to intergalactic particle jets, are connected to these strong-field conditions. And a variety of new observational facilities, from radio to X-ray to gravitational waves, promise new probes of the intense physics near black holes and neutron stars. These exotic systems hold a perennial fascination with the public and present opportunities for public engagement. The research component of this proposal studies the physics of extreme gravity and electromagnetism, with the aim of discovering new physical processes to explain existing astronomical data and make new observational predictions. The education component leverages these results to catalyze a public conversation about science more generally, via an innovative series of videos to be posted on the video-sharing website YouTube.The PI will perform analytic studies of force-free electrodynamics, the physical theory that governs strong-field plasma near compact objects (black holes and neutron stars). He will investigate stability, turbulence, and the extraction of rotational energy from the compact object. He will search for new exact solutions and general theorems governing the breakdown of the theory. The PI will also study a class of 'extremal' black holes, which are comparatively ill-understood. In astrophysics, extremal means rapidly rotating, and the PI will search for new observational signatures of high-spin black holes. The PI will also study a recently-discovered instability of extremal black holes, aiming to determine the regimes in which it operates as well as its generic physical outcome. The PI will create a series of short videos about science and scientists and disseminate it on the video-sharing website YouTube. The videos will feature the PI's own research, as well as that of other scientists, in a format designed to be fun, casual, and informative. The main goal is to build public familiarity with the process of science and thereby increase public confidence in scientific results.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.
我们的宇宙充满了奇异的物体,它们将我们熟悉的引力、电和磁现象推向了极端。 中子星的磁场比最强的地球磁体强数十亿倍,并在太空中驱动超过一万亿伏的电流。 黑洞的引力非常强大,任何东西——甚至光——都无法逃脱它的控制。 从快速无线电爆发到星系间粒子喷流,各种天文谜团都与这些强场条件有关。 从无线电到X射线再到引力波的各种新观测设施有望对黑洞和中子星附近的强烈物理现象进行新的探测。 这些奇特的系统一直吸引着公众,并为公众参与提供了机会。该提案的研究部分研究极端重力和电磁学的物理学,目的是发现新的物理过程来解释现有的天文数据并做出新的观测预测。 教育部分通过在视频共享网站 YouTube 上发布的一系列创新视频,利用这些结果来促进更广泛的公众关于科学的对话。PI 将进行无力电动力学的分析研究,这是一种控制致密物体(黑洞和中子星)附近强场等离子体的物理理论。 他将研究稳定性、湍流以及从致密物体中提取旋转能量。 他将寻找新的精确解和管理理论崩溃的一般定理。 PI还将研究一类“极端”黑洞,人们对此知之甚少。 在天体物理学中,极值意味着快速旋转,PI将寻找高自旋黑洞的新观测特征。 PI还将研究最近发现的极值黑洞的不稳定性,旨在确定其运行状态及其一般物理结果。 PI 将制作一系列有关科学和科学家的短视频,并在视频共享网站 YouTube 上传播。 这些视频将以有趣、休闲和信息丰富的形式展示 PI 自己的研究以及其他科学家的研究。 主要目标是提高公众对科学过程的熟悉程度,从而提高公众对科学成果的信心。该奖项反映了 NSF 的法定使命,并通过使用基金会的智力价值和更广泛的影响审查标准进行评估,认为值得支持。
项目成果
期刊论文数量(20)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
An asymptotic framework for gravitational scattering
- DOI:10.1088/1361-6382/acf5c1
- 发表时间:2023-03
- 期刊:
- 影响因子:3.5
- 作者:G. Compère;S. Gralla;Hongjin Wei
- 通讯作者:G. Compère;S. Gralla;Hongjin Wei
Images and photon ring signatures of thick disks around black holes
黑洞周围厚圆盘的图像和光子环特征
- DOI:10.1051/0004-6361/202244339
- 发表时间:2022
- 期刊:
- 影响因子:6.5
- 作者:Vincent, F. H.;Gralla, S. E.;Lupsasca, A.;Wielgus, M.
- 通讯作者:Wielgus, M.
Effective field theory of force-free electrodynamics
无力电动力学的有效场论
- DOI:10.1103/physrevd.99.105004
- 发表时间:2019
- 期刊:
- 影响因子:5
- 作者:Gralla, Samuel E.;Iqbal, Nabil
- 通讯作者:Iqbal, Nabil
Can the EHT M87 results be used to test general relativity?
- DOI:10.1103/physrevd.103.024023
- 发表时间:2021-01-12
- 期刊:
- 影响因子:5
- 作者:Gralla, Samuel E.
- 通讯作者:Gralla, Samuel E.
Self-force effects in post-Minkowskian scattering
后闵可夫斯基散射中的自力效应
- DOI:10.1088/1361-6382/ac5d88
- 发表时间:2022
- 期刊:
- 影响因子:3.5
- 作者:Gralla, Samuel E;Lobo, Kunal
- 通讯作者:Lobo, Kunal
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Samuel Gralla其他文献
Samuel Gralla的其他文献
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{{ truncateString('Samuel Gralla', 18)}}的其他基金
Strong Gravitational Fields: Theoretical Properties and Observational Signatures
强引力场:理论特性和观测特征
- 批准号:
2309191 - 财政年份:2023
- 资助金额:
$ 40万 - 项目类别:
Standard Grant
Strong Gravitational and Electromagnetic Fields
强引力场和电磁场
- 批准号:
1506027 - 财政年份:2015
- 资助金额:
$ 40万 - 项目类别:
Standard Grant
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- 资助金额:55 万元
- 项目类别:面上项目
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Probing the Cosmos with Strong Gravitational Lensing
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Testing alternative theories of gravity in strong gravitational field by searching for gravitational-wave polarization from compact binary coalescences
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22KJ1650 - 财政年份:2023
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Exploring Strong-Field Gravity through Gravitational-Wave and Multimessenger Observations
通过引力波和多信使观测探索强场引力
- 批准号:
2309066 - 财政年份:2023
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CAREER: Exploring Strong-field Gravity and Dense Matter Physics through Gravitational-wave Observations
职业:通过引力波观测探索强场引力和稠密物质物理
- 批准号:
2339969 - 财政年份:2023
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Strong Gravitational Fields: Theoretical Properties and Observational Signatures
强引力场:理论特性和观测特征
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Dynamical and Strong-Field Gravitational-Wave Phenomenology
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2309021 - 财政年份:2023
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Exploring Physics in the Strong Gravity through a Novel Gravitational Wave Data Analysis Method
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- 资助金额:
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Collaborative Proposal: Measuring the Physical Properties of Dark Matter with Strong Gravitational Lensing
合作提案:用强引力透镜测量暗物质的物理特性
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Strong-gravity compact objects and fundamental gravity tests in the era of gravitational-wave astronomy
引力波天文学时代的强引力致密天体与基础引力测试
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Collaborative Research: Measuring the physical properties of darkmatter with strong gravitational lensing
合作研究:利用强引力透镜测量暗物质的物理特性
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2205100 - 财政年份:2022
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