2.3: Limits

In the previous two sections we computed some quantities of interest (slope, velocity) by seeing that some expression "goes to'' or "approaches'' or "gets really close to'' a particular value. In the examples we saw, this idea may have been clear enough, but it is too fuzzy to rely on in more difficult circumstances. In this section we will see how to make the idea more precise.

There is an important feature of the examples we have seen. Consider again the formula \[{-19.6\Delta x-4.9\Delta x^2\over \Delta x}. \] We wanted to know what happens to this fraction as "\(\Delta x\) goes to zero.'' Because we were able to simplify the fraction, it was easy to see the answer, but it was not quite as simple as "substituting zero for \(\Delta x\),'' as that would give \[{-19.6\cdot 0 - 4.9\cdot 0\over 0},\] which is meaningless. The quantity we are really interested in does not make sense "at zero,'' and this is why the answer to the original problem (finding a velocity or a slope) was not immediately obvious. In other words, we are generally going to want to figure out what a quantity "approaches'' in situations where we can't merely plug in a value. If you would like to think about a hard example (which we will analyze later) consider what happens to \((\sin x)/x\) as \(x\) approaches zero.

Example \(\PageIndex{1}\)

Does \( \sqrt{x}\) approach 1.41 as \(x\) approaches 2?

Solution

In this case it is possible to compute the actual value \( \sqrt{2}\) to a high precision to answer the question. But since in general we won't be able to do that, let's not. We might start by computing \( \sqrt{x}\) for values of \(x\) close to 2, as we did in the previous sections. Here are some values: \( \sqrt{2.05} = 1.431782106\), \( \sqrt{2.04} = 1.428285686\), \( \sqrt{2.03} = 1.424780685\), \( \sqrt{2.02} = 1.421267040\), \( \sqrt{2.01} = 1.417744688\), \( \sqrt{2.005} = 1.415980226\), \( \sqrt{2.004} = 1.415627070\), \( \sqrt{2.003} = 1.415273825\), \( \sqrt{2.002} = 1.414920492\), \( \sqrt{2.001} = 1.414567072\). So it looks at least possible that indeed these values "approach'' 1.41---already \( \sqrt{2.001}\) is quite close. If we continue this process, however, at some point we will appear to "stall.'' In fact, \( \sqrt{2}=1.414213562\ldots\), so we will never even get as far as 1.4142, no matter how long we continue the sequence.

So in a fuzzy, everyday sort of sense, it is true that \( \sqrt{x}\) "gets close to'' 1.41, but it does not "approach'' 1.41 in the sense we want. To compute an exact slope or an exact velocity, what we want to know is that a given quantity becomes "arbitrarily close'' to a fixed value, meaning that the first quantity can be made "as close as we like'' to the fixed value. Consider again the quantities

\[{-19.6\Delta x-4.9\Delta x^2\over \Delta x}=-19.6-4.9\Delta x. \]

These two quantities are equal as long as \(\Delta x\) is not zero; if \(\Delta x\) is zero, the left hand quantity is meaningless, while the right hand one is \(-19.6\). Can we say more than we did before about why the right hand side "approaches'' \(-19.6\), in the desired sense? Can we really make it "as close as we want'' to \(-19.6\)? Let's try a test case. Can we make \(-19.6-4.9\Delta x\) within one millionth \(0.000001\) of \(-19.6\)? The values within a millionth of \(-19.6\) are those in the interval \((-19.600001,-19.599999)\). As \(\Delta x\) approaches zero, does \(-19.6-4.9\Delta x\) eventually reside inside this interval? If \(\Delta x\) is positive, this would require that \(-19.6-4.9\Delta x> -19.600001\). This is something we can manipulate with a little algebra:

\[\eqalign{-19.6-4.9\Delta x&> -19.600001\cr -4.9\Delta x&>-0.000001\cr \Delta x& < -0.000001/-4.9\cr \Delta x& < 0.0000002040816327\ldots\cr } \nonumber\]

Thus, we can say with certainty that if \(\Delta x\) is positive and less than \(0.0000002\), then \(\Delta x < 0.0000002040816327\ldots\) and so \(-19.6-4.9\Delta x > -19.600001\). We could do a similar calculation if \(\Delta x\) is negative.

So now we know that we can make \(-19.6-4.9\Delta x\) within one millionth of \(-19.6\). But can we make it "as close as we want''? In this case, it is quite simple to see that the answer is yes, by modifying the calculation we've just done. It may be helpful to think of this as a game. I claim that I can make \(-19.6-4.9\Delta x\) as close as you desire to \(-19.6\) by making \(\Delta x\) "close enough'' to zero. So the game is: you give me a number, like \( 10^{-6}\), and I have to come up with a number representing how close \(\Delta x\) must be to zero to guarantee that \(-19.6-4.9\Delta x\) is at least as close to \(-19.6\) as you have requested.

Now if we actually play this game, I could redo the calculation above for each new number you provide. What I'd like to do is somehow see that I will always succeed, and even more, I'd like to have a simple strategy so that I don't have to do all that algebra every time. A strategy in this case would be a formula that gives me a correct answer no matter what you specify. So suppose the number you give me is \(\epsilon\). How close does \(\Delta x\) have to be to zero to guarantee that \(-19.6-4.9\Delta x\) is in \((-19.6-\epsilon, -19.6+\epsilon)\)? If \(\Delta x\) is positive, we need:

\[\eqalign{-19.6-4.9\Delta x&> -19.6-\epsilon\cr -4.9\Delta x&>-\epsilon\cr \Delta x& < -\epsilon/-4.9\cr \Delta x& < \epsilon/4.9\cr } \nonumber\]

So if I pick any number \(\delta\) that is less than \(\epsilon/4.9\), the algebra tells me that whenever \(\Delta x < \delta\) then \(\Delta x < \epsilon/4.9\) and so \(-19.6-4.9\Delta x\) is within \(\epsilon\) of \(-19.6\). (This is exactly what I did in the example: I picked \(\delta = 0.0000002 < 0.0000002040816327\ldots\).) A similar calculation again works for negative \(\Delta x\). The important fact is that this is now a completely general result---it shows that I can always win, no matter what "move'' you make.

Now we can codify this by giving a precise definition to replace the fuzzy, "gets closer and closer'' language we have used so far. Henceforward, we will say something like "the limit of \( (-19.6\Delta x-4.9\Delta x^2)/\Delta x\) as \(\Delta x\) goes to zero is \(-19.6\),'' and abbreviate this mouthful as

\[\displaystyle \lim_{\Delta x\to 0} {-19.6\Delta x-4.9\Delta x^2\over \Delta x} = -19.6. \nonumber \]

Here is the actual, official definition of "limit''.

Definition \(\PageIndex{2}\): Limits

Suppose \(f\) is a function. We say that \(\displaystyle \displaystyle \lim_{x\to a}f(x)=L\) if for every \(\epsilon>0\) there is a \(\delta > 0\) so that whenever \(0 < |x-a| < \delta\), \(|f(x)-L| < \epsilon\).

The \(\epsilon\) and \(\delta\) here play exactly the role they did in the preceding discussion. The definition says, in a very precise way, that \(f(x)\) can be made as close as desired to \(L\) (that's the \(|f(x)-L| < \epsilon\) part) by making \(x\) close enough to \(a\) (the \(0 < |x-a| < \delta\) part). Note that we specifically make no mention of what must happen if \(x=a\), that is, if \(|x-a|=0\). This is because in the cases we are most interested in, substituting \(a\) for \(x\) doesn't even make sense.

Make sure you are not confused by the names of important quantities. The generic definition talks about \(f(x)\), but the function and the variable might have other names. In the discussion above, the function we analyzed was

\[{-19.6\Delta x-4.9\Delta x^2\over \Delta x}. \nonumber \]

and the variable of the limit was not \(x\) but \(\Delta x\). The \(x\) was the variable of the original function; when we were trying to compute a slope or a velocity, \(x\) was essentially a fixed quantity, telling us at what point we wanted the slope. (In the velocity problem, it was literally a fixed quantity, as we focused on the time 2.) The quantity \(a\) of the definition in all the examples was zero: we were always interested in what happened as \(\Delta x\) became very close to zero.

Armed with a precise definition, we can now prove that certain quantities behave in a particular way. The bad news is that even proofs for simple quantities can be quite tedious and complicated; the good news is that we rarely need to do such proofs, because most expressions act the way you would expect, and this can be proved once and for all.

Example \(\PageIndex{3}\)

Let's show carefully that \(\displaystyle \displaystyle \lim_{x\to 2} x+4 = 6\).

Solution

This is not something we "need'' to prove, since it is "obviously'' true. But if we couldn't prove it using our official definition there would be something very wrong with the definition. As is often the case in mathematical proofs, it helps to work backwards. We want to end up showing that under certain circumstances \(x+4\) is close to 6; precisely, we want to show that \(|x+4-6| < \epsilon\), or \(|x-2| < \epsilon\). Under what circumstances? We want this to be true whenever \(0 < |x-2| < \delta\). So the question becomes: can we choose a value for \(\delta\) that guarantees that \(0 < |x-2| < \delta\) implies \(|x-2| < \epsilon\)? Of course: no matter what \(\epsilon\) is, \(\delta=\epsilon\) works.

So it turns out to be very easy to prove something "obvious,'' which is nice. It doesn't take long before things get trickier, however.

Example \(\PageIndex{4}\)

It seems clear that \(\displaystyle \displaystyle \lim_{x\to 2} x^2=4\). Let's try to prove it.

Solution

We will want to be able to show that \( |x^2-4| < \epsilon\) whenever \(0 < |x-2| < \delta\), by choosing \(\delta\) carefully. Is there any connection between \(|x-2|\) and \( |x^2-4|\)? Yes, and it's not hard to spot, but it is not so simple as the previous example. We can write \( |x^2-4|=|(x+2)(x-2)|\). Now when \(|x-2|\) is small, part of \(|(x+2)(x-2)|\) is small, namely \((x-2)\). What about \((x+2)\)? If \(x\) is close to 2, \((x+2)\) certainly can't be too big, but we need to somehow be precise about it. Let's recall the "game'' version of what is going on here. You get to pick an \(\epsilon\) and I have to pick a \(\delta\) that makes things work out. Presumably it is the really tiny values of \(\epsilon\) I need to worry about, but I have to be prepared for anything, even an apparently "bad'' move like \(\epsilon=1000\).

I expect that \(\epsilon\) is going to be small, and that the corresponding \(\delta\) will be small, certainly less than 1. If \(\delta\le 1\) then \(|x+2| < 5\) when \(|x-2| < \delta\) (because if \(x\) is within 1 of 2, then \(x\) is between 1 and 3 and \(x+2\) is between 3 and 5). So then I'd be trying to show that

\[|(x+2)(x-2)| < 5|x-2| < \epsilon. \nonumber\]

So now how can I pick \(\delta\) so that \(|x-2| < \delta\) implies \(5|x-2| < \epsilon\)? This is easy: use \(\delta=\epsilon/5\), so \(5|x-2| < 5(\epsilon/5) = \epsilon\). But what if the \(\epsilon\) you choose is not small? If you choose \(\epsilon=1000\), should I pick \(\delta=200\)? No, to keep things "sane'' I will never pick a \(\delta\) bigger than 1. Here's the final "game strategy:'' When you pick a value for \(\epsilon\) I will pick \(\delta=\epsilon/5\) or \(\delta=1\), whichever is smaller. Now when \(|x-2| < \delta\), I know both that \(|x+2| < 5\) and that \(|x-2| < \epsilon/5\). Thus

\[|(x+2)(x-2)| < 5(\epsilon/5) = \epsilon. \nonumber\]

This has been a long discussion, but most of it was explanation and scratch work. If this were written down as a proof, it would be quite short, like this:

Proof that \(\displaystyle \displaystyle \lim_{x\to 2}x^2=4\). Given any \(\epsilon\), pick \(\delta=\epsilon/5\) or \(\delta=1\), whichever is smaller. Then when \(|x-2| < \delta\), \(|x+2| < 5\) and \(|x-2| < \epsilon/5\). Hence

\[ |x^2-4|=|(x+2)(x-2)| < 5(\epsilon/5) = \epsilon \nonumber.\]

It probably seems obvious that \(\displaystyle \displaystyle \lim_{x\to2}x^2=4\), and it is worth examining more closely why it seems obvious. If we write \( x^2=x\cdot x\), and ask what happens when \(x\) approaches 2, we might say something like, "Well, the first \(x\) approaches 2, and the second \(x\) approaches 2, so the product must approach \(2\cdot2\).'' In fact this is pretty much right on the money, except for that word "must.'' Is it really true that if \(x\) approaches \(a\) and \(y\) approaches \(b\) then \(xy\) approaches \(ab\)? It is, but it is not really obvious, since \(x\) and \(y\) might be quite complicated. The good news is that we can see that this is true once and for all, and then we don't have to worry about it ever again. When we say that \(x\) might be "complicated'' we really mean that in practice it might be a function. Here is then what we want to know:

Theorem \(\PageIndex{5}\)

Suppose \(\displaystyle \displaystyle \lim_{x\to a} f(x)=L\) and \( \displaystyle\displaystyle \lim_{x\to a}g(x)=M\). Then

\[\displaystyle \lim_{x\to a} f(x)g(x) = LM.\]

Proof

We have to use the official definition of limit to make sense of this. So given any \(\epsilon\) we need to find a \(\delta\) so that \(0 < |x-a| < \delta\) implies \(|f(x)g(x)-LM| < \epsilon\). What do we have to work with? We know that we can make \(f(x)\) close to \(L\) and \(g(x)\) close to \(M\), and we have to somehow connect these facts to make \(f(x)g(x)\) close to \(LM\).

We use, as is so often the case, a little algebraic trick:

\[\eqalign{|f(x)g(x)-LM|&= |f(x)g(x)-f(x)M+f(x)M-LM|\cr &=|f(x)(g(x)-M)+(f(x)-L)M|\cr &\le |f(x)(g(x)-M)|+|(f(x)-L)M|\cr &=|f(x)||g(x)-M|+|f(x)-L||M|.\cr} \nonumber \]

This is all straightforward except perhaps for the "\(\le\)'. That is an example of the triangle inequality , which says that if \(a\) and \(b\) are any real numbers then \(|a+b|\le |a|+|b|\). If you look at a few examples, using positive and negative numbers in various combinations for \(a\) and \(b\), you should quickly understand why this is true; we will not prove it formally.

Since \( \displaystyle \displaystyle \lim_{x\to a}f(x) =L\), there is a value \( \delta_1\) so that \(0 < |x-a| < \delta_1\) implies \(|f(x)-L| < |\epsilon/(2M)|\), This means that \(0 < |x-a| < \delta_1\) implies \(|f(x)-L||M| < \epsilon/2\). You can see where this is going: if we can make \(|f(x)||g(x)-M| < \epsilon/2\) also, then we'll be done.

We can make \(|g(x)-M|\) smaller than any fixed number by making \(x\) close enough to \(a\); unfortunately, \(\epsilon/(2f(x))\) is not a fixed number, since \(x\) is a variable. Here we need another little trick, just like the one we used in analyzing \(x^2\). We can find a \(\delta_2\) so that \(|x-a| < \delta_2\) implies that \(|f(x)-L| < 1\), meaning that \(L-1 < f(x) < L+1\). This means that \(|f(x)| < N\), where \(N\) is either \(|L-1|\) or \(|L+1|\), depending on whether \(L\) is negative or positive. The important point is that \(N\) doesn't depend on \(x\). Finally, we know that there is a \(\delta_3\) so that \(0 < |x-a| < \delta_3\) implies \(|g(x)-M| < \epsilon/(2N)\). Now we're ready to put everything together. Let \(\delta\) be the smallest of \(\delta_1\), \(\delta_2\), and \(\delta_3\). Then \(|x-a| < \delta\) implies that \(|f(x)-L| < |\epsilon/(2M)|\), \(|f(x)| < N\), and \(|g(x)-M| < \epsilon/(2N)\). Then

\[\eqalign{|f(x)g(x)-LM|&\le|f(x)||g(x)-M|+|f(x)-L||M|\cr & < N{\epsilon\over 2N}+\left|{\epsilon\over 2M}\right||M|\cr &={\epsilon\over 2}+{\epsilon\over 2}=\epsilon.\cr} \nonumber \]

This is just what we needed, so by the official definition, \( \displaystyle \displaystyle \lim_{x\to a}f(x)g(x)=LM\).

\(\square\)

A handful of such theorems give us the tools to compute many limits without explicitly working with the definition of limit.

Theorem \(\PageIndex{6}\)

Suppose that \(\displaystyle \lim_{x\to a}f(x)=L\) and \(\displaystyle \displaystyle \lim_{x\to a}g(x)=M\) and \(k\) is some constant. Then

\[\eqalign{ &\displaystyle \lim_{x\to a} kf(x) = k\displaystyle \lim_{x\to a}f(x)=kL\cr &\displaystyle \lim_{x\to a} (f(x)+g(x)) = \displaystyle \lim_{x\to a}f(x)+\displaystyle \lim_{x\to a}g(x)=L+M\cr &\displaystyle \lim_{x\to a} (f(x)-g(x)) = \displaystyle \lim_{x\to a}f(x)-\displaystyle \lim_{x\to a}g(x)=L-M\cr &\displaystyle \lim_{x\to a} (f(x)g(x)) = \displaystyle \lim_{x\to a}f(x)\cdot\displaystyle \lim_{x\to a}g(x)=LM\cr &\displaystyle \lim_{x\to a} {f(x)\over g(x)} = {\displaystyle \lim_{x\to a}f(x)\over\displaystyle \lim_{x\to a}g(x)}={L\over M},\hbox{ if \(M\) is not 0}\cr }\]

Roughly speaking, these rules say that to compute the limit of an algebraic expression, it is enough to compute the limits of the "innermost bits'' and then combine these limits. This often means that it is possible to simply plug in a value for the variable, since \( \displaystyle \displaystyle \lim_{x\to a} x =a\).

Example \(\PageIndex{7}\)

Compute \( \displaystyle \displaystyle \lim_{x\to 1}{x^2-3x+5\over x-2}\).

Solution

If we apply the theorem in all its gory detail, we get

\[\eqalign{ \displaystyle \lim_{x\to 1}{x^2-3x+5\over x-2}&= {\displaystyle \lim_{x\to 1}(x^2-3x+5)\over \displaystyle \lim_{x\to1}(x-2)}\cr &={(\displaystyle \lim_{x\to 1}x^2)-(\displaystyle \lim_{x\to1}3x)+(\displaystyle \lim_{x\to1}5)\over (\displaystyle \lim_{x\to1}x)-(\displaystyle \lim_{x\to1}2)}\cr &={(\displaystyle \lim_{x\to 1}x)^2-3(\displaystyle \lim_{x\to1}x)+5\over (\displaystyle \lim_{x\to1}x)-2}\cr &={1^2-3\cdot1+5\over 1-2}\cr &={1-3+5\over -1} = -3\cr } \nonumber \]

It is worth commenting on the trivial limit \( \displaystyle \displaystyle \lim_{x\to1}5\). From one point of view this might seem meaningless, as the number 5 can't "approach'' any value, since it is simply a fixed number. But 5 can, and should, be interpreted here as the function that has value 5 everywhere, \(f(x)=5\), with graph a horizontal line. From this point of view it makes sense to ask what happens to the height of the function as \(x\) approaches 1.

Of course, as we've already seen, we're primarily interested in limits that aren't so easy, namely, limits in which a denominator approaches zero. There are a handful of algebraic tricks that work on many of these limits.

Example \(\PageIndex{8}\)

Compute \(\displaystyle \displaystyle \lim_{x\to1}{x^2+2x-3\over x-1}\).

Solution

We cannot simply plug in \(x=1\) because that makes the denominator zero. However:

\[\eqalign{ \displaystyle \lim_{x\to1}{x^2+2x-3\over x-1}&=\displaystyle \lim_{x\to1}{(x-1)(x+3)\over x-1}\cr &=\displaystyle \lim_{x\to1}(x+3)=4\cr }\]

While theorem \(\PageIndex{6}\) is very helpful, we need a bit more to work easily with limits. Since the theorem applies when some limits are already known, we need to know the behavior of some functions that cannot themselves be constructed from the simple arithmetic operations of the theorem, such as \( \sqrt{x}\). Also, there is one other extraordinarily useful way to put functions together: composition. If \(f(x)\) and \(g(x)\) are functions, we can form two functions by composition: \(f(g(x))\) and \(g(f(x))\). For example, if \( f(x)=\sqrt{x}\) and \( g(x)=x^2+5\), then \( f(g(x))=\sqrt{x^2+5}\) and \( g(f(x))=(\sqrt{x})^2+5=x+5\). Here is a companion to theorem \(\PageIndex{6}\) for composition:

Theorem \(\PageIndex{9}\)

Suppose that \(\displaystyle \displaystyle \lim_{x\to a}g(x)=L\) and \(\displaystyle \displaystyle \lim_{x\to L}f(x)=f(L)\). Then

\[\displaystyle \lim_{x\to a} f(g(x)) = f(L).\]

Note the special form of the condition on \(f\): it is not enough to know that \( \displaystyle \displaystyle \lim_{x\to L}f(x) = M\), though it is a bit tricky to see why. Many of the most familiar functions do have this property, and this theorem can therefore be applied. For example:

Theorem \(\PageIndex{10}\)

Suppose that \(n\) is a positive integer. Then

\[\displaystyle \lim_{x\to a}\root n\of{x} = \root n\of{a},\]

provided that \(a\) is positive if \(n\) is even.

This theorem is not too difficult to prove from the definition of limit. Another of the most common algebraic tricks was used in section 2.1. Here's another example:

Example \(\PageIndex{11}\)

Compute \(\displaystyle \displaystyle \lim_{x\to-1} {\sqrt{x+5}-2\over x+1}\).

Solution

\[ \eqalign{\displaystyle \lim_{x\to-1} {\sqrt{x+5}-2\over x+1}&= \displaystyle \lim_{x\to-1} {\sqrt{x+5}-2\over x+1}{\sqrt{x+5}+2\over \sqrt{x+5}+2}\cr &=\displaystyle \lim_{x\to-1} {x+5-4\over (x+1)(\sqrt{x+5}+2)}\cr &=\displaystyle \lim_{x\to-1} {x+1\over (x+1)(\sqrt{x+5}+2)}\cr &=\displaystyle \lim_{x\to-1} {1\over \sqrt{x+5}+2}={1\over4}\cr} \]

At the very last step we have used theorems 2.3.9 and \(\PageIndex{10}\).

Occasionally we will need a slightly modified version of the limit definition. Consider the function \( f(x)=\sqrt{1-x^2}\), the upper half of the unit circle. What can we say about \( \displaystyle \displaystyle \lim_{x\to 1}f(x)\)? It is apparent from the graph of this familiar function that as \(x\) gets close to 1 from the left, the value of \(f(x)\) gets close to zero. It does not even make sense to ask what happens as \(x\) approaches 1 from the right, since \(f(x)\) is not defined there. The definition of the limit, however, demands that \(f(1+\Delta x)\) be close to \(f(1)\) whether \(\Delta x\) is positive or negative. Sometimes the limit of a function exists from one side or the other (or both) even though the limit does not exist. Since it is useful to be able to talk about this situation, we introduce the concept of one sided limit:

Definition \(\PageIndex{12}\): One Sided Limits

Suppose that \(f(x)\) is a function. We say that \( \displaystyle \displaystyle \lim_{x\to a^-}f(x)=L\) if for every \(\epsilon>0\) there is a \(\delta > 0\) so that whenever \(0 < a-x < \delta\), \(|f(x)-L| < \epsilon\). We say that \(\displaystyle \lim_{x\to a^+}f(x)=L\) if for every \(\epsilon>0\) there is a \(\delta > 0\) so that whenever \(0 < x-a < \delta\), \(|f(x)-L| < \epsilon\).

Usually \( \displaystyle \displaystyle \lim_{x\to a^-}f(x)\) is read "the limit of \(f(x)\) from the left'' and \( \displaystyle \displaystyle \lim_{x\to a^+}f(x)\) is read "the limit of \(f(x)\) from the right''.

Example \(\PageIndex{13}\)

Discuss \( \displaystyle \displaystyle \lim_{x\to 0}{x\over|x|}\), \( \displaystyle \displaystyle \lim_{x\to 0^-}{x\over|x|}\), and \( \displaystyle \displaystyle \lim_{x\to 0^+}{x\over|x|}\).

Solution

The function \(f(x)=x/|x|\) is undefined at 0; when \(x>0\), \(|x|=x\) and so \(f(x)=1\); when \(x < 0\), \(|x|=-x\) and \(f(x)=-1\). Thus \( \displaystyle \displaystyle \lim_{x\to 0^-}{x\over|x|}=\displaystyle \lim_{x\to 0^-}-1=-1\) while \( \displaystyle \displaystyle \lim_{x\to 0^+}{x\over|x|}=\displaystyle \lim_{x\to 0^+}1=1\). The limit of \(f(x)\) must be equal to both the left and right limits; since they are different, the limit \( \displaystyle \displaystyle \lim_{x\to 0}{x\over|x|}\) does not exist.

Contributors

• David Guichard (Whitman College)

• Integrated by Justin Marshall.