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Dark matters in contemporary astrophysics: A case study in theory choice and evidential reasoning.

机译:当代天体物理学中的暗物质:理论选择和证据推理的案例研究。

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摘要

This dissertation examines the dynamical dark matter problem in twentieth century astrophysics from the point of view of History and Philosophy of Science. The dynamical dark matter problem (which should be distinguished from the cosmological dark matter problem) describes the situation astronomers find themselves in with regard to the dynamics of large scale astrophysical systems such as galaxies and galaxy clusters: The observed motions are incompatible with the visible distribution matter given the accepted law of gravitation. This discrepancy has two classes of possible solutions: either there exists copious amounts of some kind of matter that neither emits nor absorbs radiation (hence “dark”), or the law of gravitation must be revised.; Chapter 2 describes the physical and philosophical foundations of dynamical inferences—inferences from discrepancies between well-founded theoretical expectations and reliable observations to the characteristics of candidate solutions. Chapter 3 discusses the history of dark matter (beginning around 1930). Chapter 4 reviews the present evidence bearing on the dark matter problem. Chapter 5 evaluates the important candidate matter solutions in light of the available evidence. Chapter 6 evaluates two candidate gravitational solutions on evidential and methodological grounds, and addresses the problem of theory choice. I do not try to solve the dark matter problem, but to uncover and evaluate patterns of inference involved in evidential arguments for and against candidate solutions.; I show that Newton's “Reasoning from Phenomena” is a good framework from which to understand what is going on in this field. I argue that “higher order” and especially non-dynamical evidence is the best hope for solving this problem in dynamics. This is so in part because of “the dark matter double bind”: the very existence of the dark matter problem means that we cannot be sure of the overall matter distribution in astrophysical systems, and this in turn means that the observed motions by themselves cannot provide relative confirmation of any theory of gravitational interactions taking place at these scales. I use Newton's Rules of Reasoning to argue that we should retain General Relativity as our theory of gravity at galactic and greater scales, despite the lack of positive evidence to confirm it over its rivals at these scales.
机译:本文从历史和科学哲学的角度研究了二十世纪天体物理学中的动力学暗物质问题。动态暗物质问题(应与宇宙学暗物质问题区别开来)描述了天文学家发现的有关大型天体物理系统(例如星系和星系团)动力学的情况:观测到的运动与可见光分布不兼容考虑到万有引力定律的问题。这种差异有两类可能的解决方案:要么存在某种既不发射也不吸收辐射的物质(因此称为“暗”),或者必须修改万有引力定律。第2章描述了动态推论的物理和哲学基础,即从有说服力的理论期望与可靠观察结果之间的差异( )到候选解决方案的特征。第3章讨论了暗物质的历史(始于1930年)。第四章回顾了有关暗物质问题的现有证据。第五章根据现有证据评估重要的候选物质解决方案。第6章从证据和方法论的角度评估了两种候选引力解,并讨论了理论选择的问题。我不是试图解决暗物质问题,而是要发现和评估与候选解决方案有关的证据论证所涉及的推理模式。我证明牛顿的《现象的原因》是一个很好的框架,可以从中了解这一领域的情况。我认为,“高阶”,尤其是“ 非动力”证据是解决动力学问题的最大希望。之所以如此,部分原因是由于“暗物质双重约束”:暗物质问题的存在意味着我们无法确定天体物理系统中整体物质的分布,这又意味着观察到的运动本身无法提供了在这些尺度上发生的任何引力相互作用理论的相对证实。我使用牛顿的推理规则来论证,尽管缺乏在这些尺度上超越其相对论者的肯定证据,但我们应该在银河系和更大尺度上保留广义相对论作为我们的引力论。

著录项

  • 作者

    Vanderburgh, William L.;

  • 作者单位

    The University of Western Ontario (Canada).;

  • 授予单位 The University of Western Ontario (Canada).;
  • 学科 Philosophy.; History of Science.
  • 学位 Ph.D.
  • 年度 2001
  • 页码 272 p.
  • 总页数 272
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 哲学理论;自然科学史;
  • 关键词

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