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Topics in LIGO-related physics: Interferometric speed meters and tidal work.

机译:LIGO相关物理学的主题:干涉速度计和潮汐工作。

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摘要

In the quest to develop viable designs for third-generation interferometric gravitational-wave detectors (such as the Laser Interferometer Gravitational-Wave Observatory, LIGO), one strategy is monitoring the relative momentum or speed of the test-mass mirrors, rather than monitoring their relative position. The most straightforward design for a speed-meter interferometer that accomplishes this is analyzed in Chapter 2. It is shown that in principle this design can beat the standard quantum limit (SQL) by an arbitrarily large amount, over an arbitrarily wide range of frequencies. However, in practice, this specific speed meter requires exorbitantly high input light power.; Chapter 3 proposes a more sophisticated version of a speed meter. This new design requires modest input power and appears to be a fully practical candidate for third-generation detectors. It can beat the SQL over a broad range of frequencies (∼10 to 100 Hz in practice) by a factor h/hSQL WSQLcirc/Wc irc . Here Wcirc is the light power circulating in the interferometer arms and WSQL ≃ 800 kW is the circulating power required to beat the SQL at 100 Hz. If squeezed vacuum (with a power-squeeze factor e−2 R) is injected into the interferometer's output port, the SQL can be beat with less laser power: h/h SQL WSQLcirc/Wc irce2R . For realistic parameters (e2 R ≃ 10 and Wcirc ≃ 800 kW), the SQL can be beat by a factor ∼3 from 10 to 100 Hz. By performing frequency-dependent homodyne detection on the output (using two kilometer-scale filter cavities), one can markedly improve the interferometer's sensitivity at frequencies above 100 Hz.; Chapter 4 is a contribution to the foundations for analyzing sources of gravitational waves. Specifically, it presents an analysis of the tidal work done on a self-gravitating body in an external tidal field. By examining the change in the mass-energy of the body as a result of the tidal field, it is shown that the work done is gauge invariant, while the body-tidal-field interaction energy contained within the body's local asymptotic rest frame is gauge dependent. This is analogous to Newtonian theory, where the interaction energy depends on the localization of the gravitational energy, but the work done on the body is independent of that localization.
机译:为了为第三代干涉式重力波探测器(例如激光干涉仪重力波天文台,LIGO)开发可行的设计,一种策略是监视测试质量镜的相对动量或速度,而不是监视它们相对位置。完成此操作的速度表干涉仪的最直接的设计在第二章中进行了分析。结果表明,原则上的设计可以超越标准的量子极限(SQL)在任意宽的频率范围内任意增加。但是,实际上,这种特定的速度表需要过高的输入光功率。第3章提出了速度计的一种更复杂的版本。这种新设计需要适度的输入功率,并且似乎是第三代探测器的完全可行的候选者。它可以在很宽的频率范围内(实际上是10至100 Hz)击败SQL,达到 h / h SQL 〜< math> W SQL circ / W c irc < / inf> 。这里 W circ 是干涉仪臂中循环的光功率,而 W SQL &sime; 800 kW是在100 Hz时击败SQL所需的循环功率。如果将压缩真空(功率压缩因子为 e -2 R 注入干涉仪的输出端口) ,可以用更少的激光功率击败SQL: h / h SQL W SQL circ / W c irc e 2R 。对于实际参数( e 2 R &sime; 10和 W 大约800 kW),则SQL可以以10到100 Hz的3倍被击败。通过对输出进行频率相关的零差检测(使用两个公里级的滤波器腔),可以显着提高干涉仪在高于100 Hz的频率下的灵敏度。第四章为分析引力波源奠定了基础。具体而言,它提供了对外部引力场中自重体所做的潮汐工作的分析。通过检查潮汐场导致的身体质量能的变化,表明完成的工作是尺度不变的,而包含在身体局部渐近静止框架中的身体-潮汐场相互作用能是尺度的依赖。这类似于牛顿理论,在该理论中,相互作用能取决于重力能的局域性,但是在人体上所做的功与该局域性无关。

著录项

  • 作者

    Purdue, Patricia Marie.;

  • 作者单位

    California Institute of Technology.;

  • 授予单位 California Institute of Technology.;
  • 学科 Physics Optics.
  • 学位 Ph.D.
  • 年度 2003
  • 页码 108 p.
  • 总页数 108
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 光学;
  • 关键词

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