Skip to main content\(\require{physics}\require{upgreek}\everymath{\displaystyle}
\newcommand{\N}{\mathbb N}
\newcommand{\Z}{\mathbb Z}
\newcommand{\Q}{\mathbb Q}
\newcommand{\R}{\mathbb R}
\newcommand{\inv}{^{-1}}
\newcommand{\DS}{\displaystyle}
\newcommand{\eps}{\varepsilon}
\newcommand{\tsub}[1]{_{\mathrm{#1}}}
\newcommand{\ee}{\mathrm{e}}
\newcommand{\ii}{\mathrm{i}}
\newcommand{\limit}[1]{\lim\limits_{#1}}
\newcommand{\resid}[1]{\underset{#1}{\Res}}
\DeclareMathOperator{\sinc}{sinc}
\DeclareMathOperator{\sgn}{sgn}
\newcommand{\pii}{\pi}
\DeclareMathOperator{\Prob}{P}
\DeclareMathOperator{\EV}{E}
\DeclareMathOperator{\Var}{Var}
\newcommand{\bv}[1]{\boldsymbol{#1}}
\newcommand{\uv}[1]{\hat{\bv{#1}}}
\newcommand{\cl}[1]{\mathcal{#1}}
\newcommand{\bb}[1]{\mathbb{#1}}
\DeclareMathOperator{\Cis}{cis}
\DeclareMathOperator{\RE}{Re}
\DeclareMathOperator{\IM}{Im}
\newcommand{\xd}{\mathbf{d}}
\newcommand{\seq}[3]{{#1}_{#2},\cdots,{#1}_{#3}}
\newcommand{\psup}[1]{^{(#1)}}
\newcommand{\hypext}{{}^*}
\DeclareMathOperator{\st}{st}
\newcommand{\set}[1]{\left\{#1\right\}}
\DeclareMathOperator{\Sin}{Sin}
\DeclareMathOperator{\Cos}{Cos}
\DeclareMathOperator{\Tan}{Tan}
\DeclareMathOperator{\Sec}{Sec}
\DeclareMathOperator{\Csc}{Csc}
\DeclareMathOperator{\Cot}{Cot}
\DeclareMathOperator{\Log}{Log}
\DeclareMathOperator{\Arg}{Arg}
\DeclareMathOperator{\Ln}{Ln}
\DeclareMathOperator{\Grad}{grad}
\DeclareMathOperator{\Div}{div}
\DeclareMathOperator{\Curl}{curl}
\newcommand{\rd}{\textstyle\mathop{}\!\mathrm{d}^{\!\!\!-}\hspace{-0.0555 em}}
\newcommand{\rpd}{\textstyle\mathop{}\!\partial^{\hspace{-0.5 em}-}\hspace{-0.1666 em}}
\newcommand{\rdv}[2]{\frac{\rd{#1}}{\rd{#2}}}
\newcommand{\rpdv}[2]{\frac{\rpd{#1}}{\rpd{#2}}}
\newcommand{\lt}{<}
\newcommand{\gt}{>}
\newcommand{\amp}{&}
\definecolor{fillinmathshade}{gray}{0.9}
\newcommand{\fillinmath}[1]{\mathchoice{\colorbox{fillinmathshade}{$\displaystyle \phantom{\,#1\,}$}}{\colorbox{fillinmathshade}{$\textstyle \phantom{\,#1\,}$}}{\colorbox{fillinmathshade}{$\scriptstyle \phantom{\,#1\,}$}}{\colorbox{fillinmathshade}{$\scriptscriptstyle\phantom{\,#1\,}$}}}
\)
Section 9.4 Probability distributions
Objectives
-
Describe probability densities and compute probabilities by integrating over intervals.
-
Summarize a distribution using mean, variance, and standard deviation.
-
Examine important examples such as the Gaussian curve and the error function.
-
Brief review of probability
-
A function \(f\) is a probability density function if
\begin{equation*}
\int_{-\infty}^{\infty} f(x)\dd{x}=1\text{.}
\end{equation*}
Then we say the probability that \(a\le x\le b\) is
\begin{equation*}
\Prob(a\le x\le b)=\int_{a}^{b} f(x)\dd{x}\text{.}
\end{equation*}
-
Mean of a random variable \(X\text{:}\)
\begin{equation*}
\mu=\EV(X)=\int_{-\infty}^{\infty} xf(x)\dd{x}
\end{equation*}
-
Variance:
\begin{equation*}
\Var(X)=\EV[(X-\EV(X))^{2}]=\EV(X^{2})-\EV(X)^{2}
\end{equation*}
Standard deviation:
\begin{equation*}
\sigma(X)=\sqrt{\Var(X)}
\end{equation*}
-
Gaussian integral:
\begin{equation*}
\int_{-\infty}^{\infty}\ee^{-x^2}\dd{x}=\sqrt{\pii}
\end{equation*}
Error function:
\begin{equation*}
\erf(x)=\frac{2}{\sqrt{\pii}}\int_{0}^{x}\ee^{-x^2}\dd{x}
\end{equation*}