Re-creating the physics of astrophysical jets in laboratory experiments

在实验室实验中重建天体物理射流的物理原理

• 批准号: EP/G001324/1
• 负责人: Sergey Lebedev
• 金额: $ 242.33万
• 依托单位: Imperial College London
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2008
• 资助国家: 英国
• 起止时间: 2008 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=EP%2FG001324%2F1
• 关键词: Re; creating; physics; astrophysical; jets

The research outlined in this proposal lies at the border between Plasma Physics and Astrophysics and for the first time addresses experimentally the outstanding issue of how collapsing nebulae are able to launch highly collimated beams of matter. This area has been studied through observations and by numerical simulations for many years but it is our belief that well characterised quantitative experiments will play a decisive role in resolving a number of outstanding scientific issues. The proposed research will strongly advance the development of the novel research area of Laboratory Astrophysics, which seeks to enhance the understanding of the physics governing the behaviour of astrophysical objects via scaled laboratory experiments, combined with computer modelling. This proposal outlines an in-depth programme of research in this rapidly emerging area and focuses on the study of magnetized supersonic plasma jets. These jets will be formed in our MAGPIE plasma facility at Imperial College and will be studied using a variety of diagnostics including the use of intense proton beam imaging where the protons are formed using a short-pulse laser-produced plasma source adjacent to the jet. The use of proton beams as a diagnostic will allow us, for the first time, to diagnose the magnetic field structure within the jets. The understanding of the complex plasma processes involved in the formation and evolution of these jets involving high magnetic fields will, through our large-scale computational models, be transferred to plasma jets which form in a variety of astrophysical situations. Indeed plasma jets are observed in many astrophysical contexts and it is widely believed that magnetic fields play a crucial part in their structure and evolution. Moreover, it was recently suggested that magnetically driven jets play important role in gamma ray bursts and supernova explosions. This proposal will enable a decisive breakthrough in Laboratory Astrophysics, achieved by combining the three key ingredients which are now in place: a) a unique experimental approach allowing for the first time the creation of high Mach number (M>20) magnetically driven plasma jets with magnetic field topology relevant to astrophysical jet models; b) recent developments in laser technology and in plasma diagnostics to provide means for accurate diagnosis of the plasma parameters; c) 3-D MHD simulation codes developed by the laboratory plasma and astrophysics communities that are now mature enough to provide a strong connection between experiment, astrophysical models and observations. The timeliness of this proposal is also underlined by the growing interest in this field internationally with major efforts in USA (Rochester, Livermore, Cornell, San Diego, Reno). The combined expertise of the authors of this proposal and the involvement of international collaborators from Astrophysics community will allow us to create an unprecedented capability for the Laboratory Astrophysics research and provide both breadth and depth to the programme.

这项建议中概述的研究位于等离子体物理学和天体物理学之间，并首次从实验上解决了坍塌星云如何能够发射高度准直的物质束这一悬而未决的问题。多年来，人们一直通过观测和数值模拟来研究这一领域，但我们相信，具有良好特性的定量实验将在解决一些悬而未决的科学问题方面发挥决定性作用。拟议的研究将有力地推动实验室天体物理学这一新的研究领域的发展，该领域力求通过大规模的实验室实验，结合计算机模拟，加强对支配天体物理物体行为的物理学的理解。该提案概述了在这一迅速崛起的领域的深入研究方案，并侧重研究磁化超音速等离子喷流。这些喷注将在帝国理工学院的喜鹊等离子体设施中形成，并将使用各种诊断方法进行研究，包括使用高强度质子束成像，其中质子是使用喷注附近的短脉冲激光产生的等离子体源形成的。使用质子束作为诊断手段，将使我们第一次能够诊断喷流内部的磁场结构。通过我们的大规模计算模型，对这些涉及高磁场的喷流形成和演化所涉及的复杂等离子体过程的理解将转移到在各种天体物理情况下形成的等离子体喷流。事实上，在许多天体物理环境中都可以观察到等离子体喷流，人们普遍认为磁场在它们的结构和演化中起着至关重要的作用。此外，最近有人提出，磁驱动喷流在伽马射线暴和超新星爆炸中起着重要作用。这一提议将使实验室天体物理学取得决定性突破，其实现办法是结合目前已有的三个关键要素：(A)独特的实验方法，首次能够产生高马赫数(M&GT；20)磁驱动等离子体射流，其磁场拓扑与天体物理射流模型有关；b)激光技术和等离子体诊断学的最新发展，以提供准确诊断等离子体参数的手段；(C)由实验室等离子体和天体物理学团体开发的三维MHD模拟程序，现在已经足够成熟，可以在实验、天体物理模型和观测之间建立强有力的联系。国际上对这一领域的兴趣与日俱增，美国(罗切斯特、利弗莫尔、康奈尔、圣地亚哥、雷诺)做出了重大努力，这也突显了这一建议的及时性。这项建议的作者的专业知识和天体物理界的国际合作者的参与将使我们能够为实验室天体物理研究创造前所未有的能力，并为该方案提供广度和深度。

项目成果

Formation of radiatively cooled, supersonically rotating, plasma flows in Z-pinch experiments: Towards the development of an experimental platform to study accretion disk physics in the laboratory

Z 箍缩实验中辐射冷却、超音速旋转等离子体流的形成：致力于开发实验室研究吸积盘物理的实验平台

• DOI: 10.1016/j.hedp.2015.02.001
• 发表时间: 2015
• 期刊: High Energy Density Physics
• 影响因子: 1.6
• 作者: Bennett M

Rotating plasma disks in dense Z-pinch experiments

在密集 Z 箍缩实验中旋转等离子体盘

• DOI: 10.1063/1.4904780
• 发表时间: 2014
• 作者: Bennett M

Spectral enhancement in optical parametric amplifiers in the saturated regime

饱和状态下光学参量放大器的光谱增强

• DOI: 10.1007/s00340-013-5519-x
• 发表时间: 2013
• 期刊: Applied Physics B
• 作者: Bigourd D

Numerical simulations of Z-pinch experiments to create supersonic differentially-rotating plasma flows

用于产生超音速差速旋转等离子体流的 Z 箍缩实验的数值模拟

• DOI: 10.1016/j.hedp.2012.12.001
• 发表时间: 2013
• 期刊: High Energy Density Physics
• 影响因子: 1.6
• 作者: Bocchi M

Numerical study of jets produced by conical wire arrays on the Magpie pulsed power generator

Magpie脉冲发电机上锥形线阵产生射流的数值研究

• DOI: 10.1017/s1743921311007411
• 发表时间: 2011
• 期刊: Proceedings of the International Astronomical Union
• 作者: Bocchi M