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Nonparametric inference with applications to dark matter estimation in astronomy and degradation modeling in reliability.

机译:非参数推理在天文学暗物质估计和可靠性退化建模中的应用。

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摘要

This dissertation deals with nonparametric inference methods that arise in two major areas of application: astronomy and reliability engineering. In both of these areas, extensive amounts of data are now routinely being collected. Nonparametric methods are especially useful in such environments.; The first part of this dissertation focused on mapping the distribution of dark matter in galaxies close to the Milky Way. One interesting and difficult problem is an inverse problem in which one attempts to infer the mass distribution of the galaxy from the projected positions and line-of-sight velocities of the stars. Let X = (X1, X2, X3) and V = (V1, V2, V3) denote the 3-dimensional position and velocity of a star within a galaxy. We observe only a sample of (X 1, X2, V3) with a proper choice of coordinates. With the assumptions of spherical symmetry and velocity isotropy, estimating the mass distribution tends to determine the second derivative of function Psi, which is subject to certain shape restrictions: non-negative, decreasing and convex. The new procedure of estimation we have developed combines spline techniques with the isotonic methods to obtain a consistent estimate of mass distribution. Within the context of dark matter distributions, an important quantity to estimate is the velocity dispersion, E&parl0;∥V∥ 2&vbm0;X=x&parr0; . We extend the isotonic analysis in Groneboom and Jongbloed (Ann. of Stat., 1995) to estimate a regression function. The main result is a version of the Kiefer-Wolfowitz theorem comparing the empirical distribution to its least concave majorant, but with a faster rate, n -1 log n, of convergence than n -2/3 log n. The main result is useful in obtaining asymptotic distributions for different estimators such as isotonic or kernel estimators.; The second part of the dissertation is aimed at developing a class of degradation models based on non-homogeneous Levy processes. Let X (t) be a homogeneous Levy process with mean t and variance betat where beta is an unknown parameter. We consider degradation models obtained through time-transformations of the form Y(t) = X(Λ( t)) for some nondecreasing function Λ(t). This yields a very flexible class of models that accommodate a variety of degradation shapes including increasing, decreasing, and constant degradation rates. We consider nonhomogeneous Gaussian processes with X( t) given by a Brownian motion with linear drift and nonhomogeneous Gamma process as the special cases of Levy process. If we define time-to-failure as the first-passage time, this model leads to tractable time-to-failure distributions. This allows us to combine degradation and time-to-failure data for inference. Nonparameric methods are used to estimate the degradation function Λ( t) based on different types of degradation data (destructive and non-destructive), time-to-failure data, and different sample configurations (number of degradation pathes leading to infinity, number of sample points in a degradation path going to infinity, etc.). The asymptotic behavior is used for model selection.
机译:本文研究了在两个主要应用领域出现的非参数推理方法:天文学和可靠性工程。在这两个领域中,现在通常都在收集大量数据。非参数方法在这种环境下特别有用。本文的第一部分着重于绘制暗星在银河系附近的分布图。一个有趣且困难的问题是一个反问题,其中人们试图从恒星的投射位置和视线速度推断出银河系的质量分布。令X =(X1,X2,X3)和V =(V1,V2,V3)表示星系中恒星的3维位置和速度。我们仅观察到(X 1,X2,V3)的样本,并选择了适当的坐标。在具有球对称性和速度各向同性的假设下,估计质量分布倾向于确定函数Psi的二阶导数,该函数受到某些形状限制:非负,递减和凸。我们开发的新估计程序将样条技术与等渗方法结合起来,以获得一致的质量分布估计值。在暗物质分布的背景下,要估计的重要量是速度色散E&parl; V∥ v。 2&vbm0; X = x&parr0; 。我们在Groneboom和Jongbloed(统计年鉴,1995年)中扩展了等渗分析,以估计回归函数。主要结果是一个Kiefer-Wolfowitz定理的版本,它比较了经验分布与其最小凹主要成分,但是其收敛速度n -1 log n比n -2/3 log n快。主要结果对于获得不同估计量(例如等张或核估计量)的渐近分布很有用。本文的第二部分旨在基于非齐次征税过程建立一类退化模型。令X(t)是均值Le和方差betat的齐次Levy过程,其中beta是未知参数。对于某些非递减函数Λ(t),我们考虑通过Y(t)= X(Λ(t))形式的时间变换获得的退化模型。这样便产生了非常灵活的一类模型,可以适应各种退化形状,包括增加,减少和恒定的退化率。我们将具有线性漂移的布朗运动和非齐次伽玛过程给出的X(t)的非齐次高斯过程视为Levy过程的特殊情况。如果我们将失效时间定义为首次通过时间,则此模型会导致易于计算的失效时间分布。这使我们可以将降级和故障时间数据结合起来进行推断。非参数方法用于根据不同类型的退化数据(破坏性和非破坏性),失效时间数据以及不同的样本配置(导致无穷大的退化路径数量,退化路径中的采样点将达到无穷大等)。渐近行为用于模型选择。

著录项

  • 作者

    Wang, Xiao.;

  • 作者单位

    University of Michigan.;

  • 授予单位 University of Michigan.;
  • 学科 Statistics.; Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 2005
  • 页码 117 p.
  • 总页数 117
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 统计学;天文学;
  • 关键词

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