Skip to main content
Contents
Embed
Dark Mode Prev Up Next
\(\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 5.1 Limits and continuity
Objectives
Use limits to describe when a function approaches a value.
Interpret continuity and one-sided behavior by examining how a function behaves near a point.
Recognize and classify common types of discontinuities.
Introduce limits as a way to ‘clean up’ the infinitesimal arguments we’ve been making so far.
Examine the cardinal sine function
\begin{equation*}
\sinc x=\frac{\sin x}{x}
\end{equation*}
around \(x=0\text{.}\) As \(x\to 0\text{,}\) \(\sinc x\to 1\text{,}\) so we say
\begin{equation*}
\limit{x\to 0}\frac{\sin x}{x}=1
\end{equation*}
Avoid the epsilon-delta definition at this stage... this can go in Part V. But we can perhaps still talk about ‘tolerance’ or ‘arbitrary closeness.’ Might even be able to use the symbols
\(\delta\) and
\(\eps\) for tolerance in the
\(x\) - and
\(y\) -directions, but hold back from the full formal definition.
Use the the Heaviside step function
\begin{equation*}
H(x)=\begin{cases}0 \amp \text{if }x\lt 0\\ 1 \amp \text{if }x\ge 0\end{cases}
\end{equation*}
to discuss one-sided limits
Continuity in terms of limits: \(f\) is continuous at \(x=a\) if
\begin{equation*}
\limit{x\to a}f(x)=f(a)
\end{equation*}
This means the function must be defined, the limit must exist, and the function must match the limit.
Types of discontinuity: removable, jump, infinite, oscillating
Importantly, do NOT throw away the infinitesimal ideas just because we’re using limits now! We’ll see the relationship between infinitesimals and everything we’ve done so far in more detail in Part V.