cleaning up reg slides
This commit is contained in:
@@ -2251,664 +2251,11 @@ bootstrap is widely used.
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!split
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===== Statistics =====
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!bblock
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The *probability distribution function (PDF)* is a function
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$p(x)$ on the domain which, in the discrete case, gives us the
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probability or relative frequency with which these values of $X$ occur:
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!bt
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\[
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p(x) = \mathrm{prob}(X=x)
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\]
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!et
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In the continuous case, the PDF does not directly depict the
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actual probability. Instead we define the probability for the
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stochastic variable to assume any value on an infinitesimal interval
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around $x$ to be $p(x)dx$. The continuous function $p(x)$ then gives us
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the *density* of the probability rather than the probability
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itself. The probability for a stochastic variable to assume any value
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on a non-infinitesimal interval $[a,\,b]$ is then just the integral:
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!bt
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\[
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\mathrm{prob}(a\leq X\leq b) = \int_a^b p(x)dx
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\]
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!et
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Qualitatively speaking, a stochastic variable represents the values of
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numbers chosen as if by chance from some specified PDF so that the
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selection of a large set of these numbers reproduces this PDF.
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!eblock
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!split
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===== Statistics, moments =====
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!bblock
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A particularly useful class of special expectation values are the
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*moments*. The $n$-th moment of the PDF $p$ is defined as
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follows:
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!bt
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\[
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\langle x^n\rangle \equiv \int\! x^n p(x)\,dx
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\]
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!et
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The zero-th moment $\langle 1\rangle$ is just the normalization condition of
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$p$. The first moment, $\langle x\rangle$, is called the *mean* of $p$
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and often denoted by the letter $\mu$:
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!bt
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\[
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\langle x\rangle = \mu \equiv \int\! x p(x)\,dx
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\]
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!et
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!eblock
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!split
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===== Statistics, central moments =====
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!bblock
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A special version of the moments is the set of *central moments*,
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the n-th central moment defined as:
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!bt
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\[
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\langle (x-\langle x \rangle )^n\rangle \equiv \int\! (x-\langle x\rangle)^n p(x)\,dx
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\]
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!et
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The zero-th and first central moments are both trivial, equal $1$ and
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$0$, respectively. But the second central moment, known as the
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*variance* of $p$, is of particular interest. For the stochastic
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variable $X$, the variance is denoted as $\sigma^2_X$ or $\mathrm{var}(X)$:
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!bt
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\begin{align}
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\sigma^2_X\ \ =\ \ \mathrm{var}(X) & = \langle (x-\langle x\rangle)^2\rangle =
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\int\! (x-\langle x\rangle)^2 p(x)\,dx\\
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& = \int\! \left(x^2 - 2 x \langle x\rangle^{2} +
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\langle x\rangle^2\right)p(x)\,dx\\
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& = \langle x^2\rangle - 2 \langle x\rangle\langle x\rangle + \langle x\rangle^2\\
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& = \langle x^2\rangle - \langle x\rangle^2
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\end{align}
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!et
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The square root of the variance, $\sigma =\sqrt{\langle (x-\langle x\rangle)^2\rangle}$ is called the *standard deviation* of $p$. It is clearly just the RMS (root-mean-square)
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value of the deviation of the PDF from its mean value, interpreted
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qualitatively as the *spread* of $p$ around its mean.
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!eblock
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!split
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===== Statistics, covariance =====
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!bblock
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Another important quantity is the so called covariance, a variant of
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the above defined variance. Consider again the set $\{X_i\}$ of $n$
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stochastic variables (not necessarily uncorrelated) with the
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multivariate PDF $P(x_1,\dots,x_n)$. The *covariance* of two
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of the stochastic variables, $X_i$ and $X_j$, is defined as follows:
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!bt
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\begin{align}
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\mathrm{cov}(X_i,\,X_j) &\equiv \langle (x_i-\langle x_i\rangle)(x_j-\langle x_j\rangle)\rangle
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\nonumber\\
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&=
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\int\!\cdots\!\int\!(x_i-\langle x_i \rangle)(x_j-\langle x_j \rangle)\,
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P(x_1,\dots,x_n)\,dx_1\dots dx_n
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label{eq:def_covariance}
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\end{align}
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!et
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with
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!bt
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\[
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\langle x_i\rangle =
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\int\!\cdots\!\int\!x_i\,P(x_1,\dots,x_n)\,dx_1\dots dx_n
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\]
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!et
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!eblock
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!split
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===== Statistics, more covariance =====
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!bblock
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If we consider the above covariance as a matrix $C_{ij}=\mathrm{cov}(X_i,\,X_j)$, then the diagonal elements are just the familiar
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variances, $C_{ii} = \mathrm{cov}(X_i,\,X_i) = \mathrm{var}(X_i)$. It turns out that
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all the off-diagonal elements are zero if the stochastic variables are
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uncorrelated. This is easy to show, keeping in mind the linearity of
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the expectation value. Consider the stochastic variables $X_i$ and
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$X_j$, ($i\neq j$):
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!bt
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\begin{align}
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\mathrm{cov}(X_i,\,X_j) &= \langle(x_i-\langle x_i\rangle)(x_j-\langle x_j\rangle)\rangle\\
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&=\langle x_i x_j - x_i\langle x_j\rangle - \langle x_i\rangle x_j + \langle x_i\rangle\langle x_j\rangle\rangle \\
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&=\langle x_i x_j\rangle - \langle x_i\langle x_j\rangle\rangle - \langle \langle x_i\rangle x_j\rangle +
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\langle \langle x_i\rangle\langle x_j\rangle\rangle\\
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&=\langle x_i x_j\rangle - \langle x_i\rangle\langle x_j\rangle - \langle x_i\rangle\langle x_j\rangle +
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\langle x_i\rangle\langle x_j\rangle\\
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&=\langle x_i x_j\rangle - \langle x_i\rangle\langle x_j\rangle
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\end{align}
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!et
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!eblock
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!split
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===== Covariance example =====
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Suppose we have defined three vectors $\bm{x}, \bm{y}, \bm{z}$ with
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$n$ elements each. The covariance matrix is defined as
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!bt
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\[
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\bm{\Sigma} = \begin{bmatrix} \sigma_{xx} & \sigma_{xy} & \sigma_{xz} \\
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\sigma_{yx} & \sigma_{yy} & \sigma_{yz} \\
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\sigma_{zx} & \sigma_{zy} & \sigma_{zz}
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\end{bmatrix},
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\]
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!et
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where for example
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!bt
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\[
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\sigma_{xy} =\frac{1}{n} \sum_{i=0}^{n-1}(x_i- \overline{x})(y_i- \overline{y}).
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\]
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!et
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The Numpy function _np.cov_ calculates the covariance elements using
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the factor $1/(n-1)$ instead of $1/n$ since it assumes we do not have
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the exact mean valu\ es.
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The following simple function uses the _np.vstack_ function which
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takes each vector of dimension $1\times n$ and produces a $3\times n$
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matrix $\bm{W}$
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!bt
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\[
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\bm{W} = \begin{bmatrix} x_0 & y_0 & z_0 \\
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x_1 & y_1 & z_1 \\
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x_2 & y_2 & z_2 \\
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\dots & \dots & \dots \\
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x_{n-2} & y_{n-2} & z_{n-2} \\
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x_{n-1} & y_{n-1} & z_{n-1}
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\end{bmatrix},
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\]
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!et
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which in turn is converted into into the $3\times 3$ covariance matrix
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$\bm{\Sigma}$ via the Numpy function _np.cov()_. We note that we can
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also calculate the mean value of each set of samples $\bm{x}$ etc
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using the Numpy function _np.mean(x)_. We can also extract the
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eigenvalues of the covariance matrix through the _np.linalg.eig()_
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function.
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!split
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===== Covariance in numpy =====
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!bc pycod
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# Importing various packages
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import numpy as np
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n = 100
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x = np.random.normal(size=n)
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print(np.mean(x))
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y = 4+3*x+np.random.normal(size=n)
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print(np.mean(y))
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z = x**3+np.random.normal(size=n)
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print(np.mean(z))
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W = np.vstack((x, y, z))
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Sigma = np.cov(W)
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print(Sigma)
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Eigvals, Eigvecs = np.linalg.eig(Sigma)
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print(Eigvals)
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!ec
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!bc pycod
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import numpy as np
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import matplotlib.pyplot as plt
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from scipy import sparse
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eye = np.eye(4)
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print(eye)
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sparse_mtx = sparse.csr_matrix(eye)
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print(sparse_mtx)
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x = np.linspace(-10,10,100)
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y = np.sin(x)
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plt.plot(x,y,marker='x')
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plt.show()
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!ec
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!split
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===== Statistics, independent variables =====
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!bblock
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If $X_i$ and $X_j$ are independent, we get
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$\langle x_i x_j\rangle =\langle x_i\rangle\langle x_j\rangle$, resulting in $\mathrm{cov}(X_i, X_j) = 0\ \ (i\neq j)$.
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Also useful for us is the covariance of linear combinations of
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stochastic variables. Let $\{X_i\}$ and $\{Y_i\}$ be two sets of
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stochastic variables. Let also $\{a_i\}$ and $\{b_i\}$ be two sets of
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scalars. Consider the linear combination:
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!bt
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\[
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U = \sum_i a_i X_i \qquad V = \sum_j b_j Y_j
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\]
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!et
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By the linearity of the expectation value
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!bt
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\[
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\mathrm{cov}(U, V) = \sum_{i,j}a_i b_j \mathrm{cov}(X_i, Y_j)
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\]
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!et
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!eblock
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!split
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===== Statistics, more variance =====
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!bblock
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Now, since the variance is just $\mathrm{var}(X_i) = \mathrm{cov}(X_i, X_i)$, we get
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the variance of the linear combination $U = \sum_i a_i X_i$:
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!bt
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\begin{equation}
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\mathrm{var}(U) = \sum_{i,j}a_i a_j \mathrm{cov}(X_i, X_j)
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label{eq:variance_linear_combination}
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\end{equation}
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!et
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And in the special case when the stochastic variables are
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uncorrelated, the off-diagonal elements of the covariance are as we
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know zero, resulting in:
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!bt
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\[
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\mathrm{var}(U) = \sum_i a_i^2 \mathrm{cov}(X_i, X_i) = \sum_i a_i^2 \mathrm{var}(X_i)
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\]
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!et
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!bt
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\[
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\mathrm{var}(\sum_i a_i X_i) = \sum_i a_i^2 \mathrm{var}(X_i)
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\]
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!et
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which will become very useful in our study of the error in the mean
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value of a set of measurements.
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!eblock
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!split
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===== Statistics and stochastic processes =====
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!bblock
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A *stochastic process* is a process that produces sequentially a
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chain of values:
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!bt
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\[
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\{x_1, x_2,\dots\,x_k,\dots\}.
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\]
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!et
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We will call these
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values our *measurements* and the entire set as our measured
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*sample*. The action of measuring all the elements of a sample
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we will call a stochastic *experiment* since, operationally,
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they are often associated with results of empirical observation of
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some physical or mathematical phenomena; precisely an experiment. We
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assume that these values are distributed according to some
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PDF $p_X^{\phantom X}(x)$, where $X$ is just the formal symbol for the
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stochastic variable whose PDF is $p_X^{\phantom X}(x)$. Instead of
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trying to determine the full distribution $p$ we are often only
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interested in finding the few lowest moments, like the mean
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$\mu_X^{\phantom X}$ and the variance $\sigma_X^{\phantom X}$.
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!eblock
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!split
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===== Statistics and sample variables =====
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!bblock
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In practical situations a sample is always of finite size. Let that
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size be $n$. The expectation value of a sample, the *sample mean*, is then defined as follows:
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!bt
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\[
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\bar{x}_n \equiv \frac{1}{n}\sum_{k=1}^n x_k
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\]
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!et
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The *sample variance* is:
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!bt
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\[
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\mathrm{var}(x) \equiv \frac{1}{n}\sum_{k=1}^n (x_k - \bar{x}_n)^2
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\]
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!et
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its square root being the *standard deviation of the sample*. The
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*sample covariance* is:
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!bt
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\[
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\mathrm{cov}(x)\equiv\frac{1}{n}\sum_{kl}(x_k - \bar{x}_n)(x_l - \bar{x}_n)
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\]
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!et
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!eblock
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!split
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===== Statistics, sample variance and covariance =====
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!bblock
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Note that the sample variance is the sample covariance without the
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cross terms. In a similar manner as the covariance in Eq.~(ref{eq:def_covariance}) is a measure of the correlation between
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two stochastic variables, the above defined sample covariance is a
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measure of the sequential correlation between succeeding measurements
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of a sample.
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These quantities, being known experimental values, differ
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significantly from and must not be confused with the similarly named
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quantities for stochastic variables, mean $\mu_X$, variance $\mathrm{var}(X)$
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and covariance $\mathrm{cov}(X,Y)$.
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!eblock
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!split
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===== Statistics, law of large numbers =====
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!bblock
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The law of large numbers
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states that as the size of our sample grows to infinity, the sample
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mean approaches the true mean $\mu_X^{\phantom X}$ of the chosen PDF:
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!bt
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\[
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\lim_{n\to\infty}\bar{x}_n = \mu_X^{\phantom X}
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\]
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!et
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The sample mean $\bar{x}_n$ works therefore as an estimate of the true
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mean $\mu_X^{\phantom X}$.
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What we need to find out is how good an approximation $\bar{x}_n$ is to
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$\mu_X^{\phantom X}$. In any stochastic measurement, an estimated
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mean is of no use to us without a measure of its error. A quantity
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that tells us how well we can reproduce it in another experiment. We
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are therefore interested in the PDF of the sample mean itself. Its
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standard deviation will be a measure of the spread of sample means,
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and we will simply call it the *error* of the sample mean, or
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just sample error, and denote it by $\mathrm{err}_X^{\phantom X}$. In
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practice, we will only be able to produce an *estimate* of the
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sample error since the exact value would require the knowledge of the
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true PDFs behind, which we usually do not have.
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!eblock
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!split
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===== Statistics, more on sample error =====
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!bblock
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Let us first take a look at what happens to the sample error as the
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size of the sample grows. In a sample, each of the measurements $x_i$
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can be associated with its own stochastic variable $X_i$. The
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stochastic variable $\overline X_n$ for the sample mean $\bar{x}_n$ is
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then just a linear combination, already familiar to us:
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!bt
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\[
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\overline X_n = \frac{1}{n}\sum_{i=1}^n X_i
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\]
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!et
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All the coefficients are just equal $1/n$. The PDF of $\overline X_n$,
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denoted by $p_{\overline X_n}(x)$ is the desired PDF of the sample
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means.
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!eblock
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!split
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===== Statistics =====
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!bblock
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The probability density of obtaining a sample mean $\bar x_n$
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is the product of probabilities of obtaining arbitrary values $x_1,
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x_2,\dots,x_n$ with the constraint that the mean of the set $\{x_i\}$
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is $\bar x_n$:
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!bt
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\[
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p_{\overline X_n}(x) = \int p_X^{\phantom X}(x_1)\cdots
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\int p_X^{\phantom X}(x_n)\
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\delta\!\left(x - \frac{x_1+x_2+\dots+x_n}{n}\right)dx_n \cdots dx_1
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\]
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!et
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And in particular we are interested in its variance $\mathrm{var}(\overline X_n)$.
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!eblock
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!split
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===== Statistics, central limit theorem =====
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!bblock
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It is generally not possible to express $p_{\overline X_n}(x)$ in a
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closed form given an arbitrary PDF $p_X^{\phantom X}$ and a number
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$n$. But for the limit $n\to\infty$ it is possible to make an
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approximation. The very important result is called *the central limit theorem*. It tells us that as $n$ goes to infinity,
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$p_{\overline X_n}(x)$ approaches a Gaussian distribution whose mean
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and variance equal the true mean and variance, $\mu_{X}^{\phantom X}$
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and $\sigma_{X}^{2}$, respectively:
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!bt
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\begin{equation}
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\lim_{n\to\infty} p_{\overline X_n}(x) =
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\left(\frac{n}{2\pi\mathrm{var}(X)}\right)^{1/2}
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e^{-\frac{n(x-\bar x_n)^2}{2\mathrm{var}(X)}}
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label{eq:central_limit_gaussian}
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\end{equation}
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!et
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!eblock
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!split
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===== Statistics, more technicalities =====
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!bblock
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The desired variance
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$\mathrm{var}(\overline X_n)$, i.e. the sample error squared
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$\mathrm{err}_X^2$, is given by:
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!bt
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\begin{equation}
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\mathrm{err}_X^2 = \mathrm{var}(\overline X_n) = \frac{1}{n^2}
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\sum_{ij} \mathrm{cov}(X_i, X_j)
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label{eq:error_exact}
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\end{equation}
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!et
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We see now that in order to calculate the exact error of the sample
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with the above expression, we would need the true means
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$\mu_{X_i}^{\phantom X}$ of the stochastic variables $X_i$. To
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calculate these requires that we know the true multivariate PDF of all
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the $X_i$. But this PDF is unknown to us, we have only got the measurements of
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one sample. The best we can do is to let the sample itself be an
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estimate of the PDF of each of the $X_i$, estimating all properties of
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$X_i$ through the measurements of the sample.
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!eblock
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|
||||
!split
|
||||
===== Statistics =====
|
||||
!bblock
|
||||
Our estimate of $\mu_{X_i}^{\phantom X}$ is then the sample mean $\bar x$
|
||||
itself, in accordance with the the central limit theorem:
|
||||
!bt
|
||||
\[
|
||||
\mu_{X_i}^{\phantom X} = \langle x_i\rangle \approx \frac{1}{n}\sum_{k=1}^n x_k = \bar x
|
||||
\]
|
||||
!et
|
||||
Using $\bar x$ in place of $\mu_{X_i}^{\phantom X}$ we can give an
|
||||
*estimate* of the covariance in Eq.~(ref{eq:error_exact})
|
||||
!bt
|
||||
\[
|
||||
\mathrm{cov}(X_i, X_j) = \langle (x_i-\langle x_i\rangle)(x_j-\langle x_j\rangle)\rangle
|
||||
\approx\langle (x_i - \bar x)(x_j - \bar{x})\rangle,
|
||||
\]
|
||||
!et
|
||||
resulting in
|
||||
!bt
|
||||
\[
|
||||
\frac{1}{n} \sum_{l}^n \left(\frac{1}{n}\sum_{k}^n (x_k -\bar x_n)(x_l - \bar x_n)\right)=\frac{1}{n}\frac{1}{n} \sum_{kl} (x_k -\bar x_n)(x_l - \bar x_n)=\frac{1}{n}\mathrm{cov}(x)
|
||||
\]
|
||||
!et
|
||||
!eblock
|
||||
|
||||
!split
|
||||
===== Statistics and sample variance =====
|
||||
!bblock
|
||||
By the same procedure we can use the sample variance as an
|
||||
estimate of the variance of any of the stochastic variables $X_i$
|
||||
!bt
|
||||
\[
|
||||
\mathrm{var}(X_i)=\langle x_i - \langle x_i\rangle\rangle \approx \langle x_i - \bar x_n\rangle\nonumber,
|
||||
\]
|
||||
!et
|
||||
which is approximated as
|
||||
!bt
|
||||
\begin{equation}
|
||||
\mathrm{var}(X_i)\approx \frac{1}{n}\sum_{k=1}^n (x_k - \bar x_n)=\mathrm{var}(x)
|
||||
label{eq:var_estimate_i_think}
|
||||
\end{equation}
|
||||
!et
|
||||
|
||||
Now we can calculate an estimate of the error
|
||||
$\mathrm{err}_X^{\phantom X}$ of the sample mean $\bar x_n$:
|
||||
!bt
|
||||
\begin{align}
|
||||
\mathrm{err}_X^2
|
||||
&=\frac{1}{n^2}\sum_{ij} \mathrm{cov}(X_i, X_j) \nonumber \\
|
||||
&\approx&\frac{1}{n^2}\sum_{ij}\frac{1}{n}\mathrm{cov}(x) =\frac{1}{n^2}n^2\frac{1}{n}\mathrm{cov}(x)\nonumber\\
|
||||
&=\frac{1}{n}\mathrm{cov}(x)
|
||||
label{eq:error_estimate}
|
||||
\end{align}
|
||||
!et
|
||||
which is nothing but the sample covariance divided by the number of
|
||||
measurements in the sample.
|
||||
!eblock
|
||||
|
||||
!split
|
||||
===== Statistics, uncorrelated results =====
|
||||
!bblock
|
||||
|
||||
In the special case that the measurements of the sample are
|
||||
uncorrelated (equivalently the stochastic variables $X_i$ are
|
||||
uncorrelated) we have that the off-diagonal elements of the covariance
|
||||
are zero. This gives the following estimate of the sample error:
|
||||
!bt
|
||||
\[
|
||||
\mathrm{err}_X^2=\frac{1}{n^2}\sum_{ij} \mathrm{cov}(X_i, X_j) =
|
||||
\frac{1}{n^2} \sum_i \mathrm{var}(X_i),
|
||||
\]
|
||||
!et
|
||||
resulting in
|
||||
!bt
|
||||
\begin{equation}
|
||||
\mathrm{err}_X^2\approx \frac{1}{n^2} \sum_i \mathrm{var}(x)= \frac{1}{n}\mathrm{var}(x)
|
||||
label{eq:error_estimate_uncorrel}
|
||||
\end{equation}
|
||||
!et
|
||||
where in the second step we have used Eq.~(ref{eq:var_estimate_i_think}).
|
||||
The error of the sample is then just its standard deviation divided by
|
||||
the square root of the number of measurements the sample contains.
|
||||
This is a very useful formula which is easy to compute. It acts as a
|
||||
first approximation to the error, but in numerical experiments, we
|
||||
cannot overlook the always present correlations.
|
||||
!eblock
|
||||
|
||||
!split
|
||||
===== Statistics, computations =====
|
||||
!bblock
|
||||
For computational purposes one usually splits up the estimate of
|
||||
$\mathrm{err}_X^2$, given by Eq.~(ref{eq:error_estimate}), into two
|
||||
parts
|
||||
!bt
|
||||
\[
|
||||
\mathrm{err}_X^2 = \frac{1}{n}\mathrm{var}(x) + \frac{1}{n}(\mathrm{cov}(x)-\mathrm{var}(x)),
|
||||
\]
|
||||
!et
|
||||
which equals
|
||||
!bt
|
||||
\begin{equation}
|
||||
\frac{1}{n^2}\sum_{k=1}^n (x_k - \bar x_n)^2 +\frac{2}{n^2}\sum_{k<l} (x_k - \bar x_n)(x_l - \bar x_n)
|
||||
label{eq:error_estimate_split_up}
|
||||
\end{equation}
|
||||
!et
|
||||
The first term is the same as the error in the uncorrelated case,
|
||||
Eq.~(ref{eq:error_estimate_uncorrel}). This means that the second
|
||||
term accounts for the error correction due to correlation between the
|
||||
measurements. For uncorrelated measurements this second term is zero.
|
||||
!eblock
|
||||
|
||||
!split
|
||||
===== Statistics, more on computations of errors =====
|
||||
!bblock
|
||||
Computationally the uncorrelated first term is much easier to treat
|
||||
efficiently than the second.
|
||||
!bt
|
||||
\[
|
||||
\mathrm{var}(x) = \frac{1}{n}\sum_{k=1}^n (x_k - \bar x_n)^2 =
|
||||
\left(\frac{1}{n}\sum_{k=1}^n x_k^2\right) - \bar x_n^2
|
||||
\]
|
||||
!et
|
||||
We just accumulate separately the values $x^2$ and $x$ for every
|
||||
measurement $x$ we receive. The correlation term, though, has to be
|
||||
calculated at the end of the experiment since we need all the
|
||||
measurements to calculate the cross terms. Therefore, all measurements
|
||||
have to be stored throughout the experiment.
|
||||
!eblock
|
||||
|
||||
|
||||
|
||||
|
||||
!split
|
||||
===== Statistics, wrapping up 1 =====
|
||||
!bblock
|
||||
Let us analyze the problem by splitting up the correlation term into
|
||||
partial sums of the form:
|
||||
!bt
|
||||
\[
|
||||
f_d = \frac{1}{n-d}\sum_{k=1}^{n-d}(x_k - \bar x_n)(x_{k+d} - \bar x_n)
|
||||
\]
|
||||
!et
|
||||
The correlation term of the error can now be rewritten in terms of
|
||||
$f_d$
|
||||
!bt
|
||||
\[
|
||||
\frac{2}{n}\sum_{k<l} (x_k - \bar x_n)(x_l - \bar x_n) =
|
||||
2\sum_{d=1}^{n-1} f_d
|
||||
\]
|
||||
!et
|
||||
The value of $f_d$ reflects the correlation between measurements
|
||||
separated by the distance $d$ in the sample samples. Notice that for
|
||||
$d=0$, $f$ is just the sample variance, $\mathrm{var}(x)$. If we divide $f_d$
|
||||
by $\mathrm{var}(x)$, we arrive at the so called *autocorrelation function*
|
||||
!bt
|
||||
\[
|
||||
\kappa_d = \frac{f_d}{\mathrm{var}(x)}
|
||||
\]
|
||||
!et
|
||||
which gives us a useful measure of pairwise correlations
|
||||
starting always at $1$ for $d=0$.
|
||||
!eblock
|
||||
|
||||
|
||||
!split
|
||||
===== Statistics, final expression =====
|
||||
!bblock
|
||||
The sample error (see eq.~(ref{eq:error_estimate_split_up})) can now be
|
||||
written in terms of the autocorrelation function:
|
||||
!bt
|
||||
\begin{align}
|
||||
\mathrm{err}_X^2 &=
|
||||
\frac{1}{n}\mathrm{var}(x)+\frac{2}{n}\cdot\mathrm{var}(x)\sum_{d=1}^{n-1}
|
||||
\frac{f_d}{\mathrm{var}(x)}\nonumber\\ &=&
|
||||
\left(1+2\sum_{d=1}^{n-1}\kappa_d\right)\frac{1}{n}\mathrm{var}(x)\nonumber\\
|
||||
&=\frac{\tau}{n}\cdot\mathrm{var}(x)
|
||||
label{eq:error_estimate_corr_time}
|
||||
\end{align}
|
||||
!et
|
||||
and we see that $\mathrm{err}_X$ can be expressed in terms the
|
||||
uncorrelated sample variance times a correction factor $\tau$ which
|
||||
accounts for the correlation between measurements. We call this
|
||||
correction factor the *autocorrelation time*:
|
||||
!bt
|
||||
\begin{equation}
|
||||
\tau = 1+2\sum_{d=1}^{n-1}\kappa_d
|
||||
label{eq:autocorrelation_time}
|
||||
\end{equation}
|
||||
!et
|
||||
!eblock
|
||||
|
||||
!split
|
||||
===== Statistics, effective number of correlations =====
|
||||
!bblock
|
||||
For a correlation free experiment, $\tau$
|
||||
equals 1. From the point of view of
|
||||
eq.~(ref{eq:error_estimate_corr_time}) we can interpret a sequential
|
||||
correlation as an effective reduction of the number of measurements by
|
||||
a factor $\tau$. The effective number of measurements becomes:
|
||||
!bt
|
||||
\[
|
||||
n_\mathrm{eff} = \frac{n}{\tau}
|
||||
\]
|
||||
!et
|
||||
To neglect the autocorrelation time $\tau$ will always cause our
|
||||
simple uncorrelated estimate of $\mathrm{err}_X^2\approx \mathrm{var}(x)/n$ to
|
||||
be less than the true sample error. The estimate of the error will be
|
||||
too *good*. On the other hand, the calculation of the full
|
||||
autocorrelation time poses an efficiency problem if the set of
|
||||
measurements is very large.
|
||||
!eblock
|
||||
|
||||
|
||||
|
||||
!split
|
||||
===== Linking the regression analysis with a statistical interpretation =====
|
||||
|
||||
Finally, we are going to discuss several statistical properties which can be obtained in terms of analytical expressions.
|
||||
|
||||
The
|
||||
advantage of doing linear regression is that we actually end up with
|
||||
analytical expressions for several statistical quantities.
|
||||
|
||||
Reference in New Issue
Block a user