Interactive · 4 questions

Continuity at a point (which you may or may not have seen yet) is defined as follows:

A function ff is continuous at a point pp if for every ϵ>0\epsilon > 0, there exists a δ>0\delta > 0 so that every xx within δ\delta of pp is within ϵ\epsilon of f(p)f(p).

However, continuity at a particular point pp is a "local" condition, in that we only care what's happening "near" pp. But for any particular ϵ\epsilon, the δ\delta's can vary drastically among different particular values of pp. (Indeed, we may write δ=δ(ϵ,p)\delta = \delta(\epsilon,p) to emphasize that δ\delta may depend on ϵ\epsilon and pp.) For example, let's consider the function f(x)=x2f(x) = x^2.

Let's take ϵ=1\epsilon = 1.

What's the biggest value of δ\delta we can use at p=0p=0?

Video

(Video) Continuous and Uniformly Continuous Functions

by Steve Stein

Here's a video by Steve Stein explaining what uniform continuity is and how it differs from regular continuity.

Type a concept, like “slope” or “photosynthesis”.

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