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Limit of a function

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Illustration showing four types of undefined limits in mathematical functions.

For the mathematical concept in general, see Limit (mathematics).

In mathematics, the limit of a function is a key idea in calculus and analysis. It helps us understand what happens to a function's output when its input gets very close to a certain value, even if that input isn't actually allowed.

Imagine a function that isn't defined at a specific point, like the function ⁠ sin ⁡ x x ⁠ as x approaches zero. Even though we can't calculate the function exactly at zero, we can see that as x gets closer and closer to zero, the value of ⁠ sin ⁡ x x ⁠ gets closer and closer to 1. We say the limit of ⁠ sin ⁡ x x ⁠ as x approaches zero is 1.

Limits are important because they help us define other big ideas in calculus. For example, they are used to define what it means for a function to be continuous—a function that doesn't have any sudden jumps or breaks. Limits also play a role in finding derivatives, which measure how a function changes at any point. By studying limits, we can understand the behavior of functions in ways that are useful for solving many kinds of problems.

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History

The idea of a limit of a function started to take shape during the time when calculus was being developed in the 1600s and 1700s. A mathematician named Bernard Bolzano in 1817 was the first to describe a method to define continuous functions using limits, but his work was not well known at the time. Later, in 1821, Augustin-Louis Cauchy wrote about limits and continuity in his book Cours d'analyse. Finally, in 1861, Karl Weierstrass gave the definition of a limit that we still use today. The way we write limits with an arrow underneath was introduced by G. H. Hardy in his 1908 book A Course of Pure Mathematics.

Motivation

Imagine you're walking on a landscape where your height above the ground is shown by a function y = f(x). Your horizontal position is x, like a map or a global positioning system. Suppose you walk towards a point where x equals p. As you get very close to this point, you notice that your height gets closer and closer to a specific number, called L.

This means that no matter how closely you want to get to L, there is always a way to be close enough to the point p so that your height stays very near to L. For example, if you want to be within ten meters of L, you can achieve this by staying within fifty meters of p. If you want to be even closer, like within one meter of L, you can do that by staying within five meters of p. In simple terms, the limit of a function f(x) as x approaches p is the number L that the function gets closer and closer to as x gets closer to p.

Functions of a single variable

The limit of a function is a key idea in mathematics, especially in calculus. It helps us understand how a function behaves as its input gets very close to a certain value.

When we talk about the limit of a function, we’re describing what value the function gets closer and closer to as the input approaches a specific point. This doesn’t always mean the function actually reaches that point, but it gives us insight into the function’s behavior near that point.

For example, imagine you’re walking towards a fence. The limit tells you how close you can get to the fence without actually touching it. This concept is important for understanding continuous functions and solving complex problems in calculus.

Functions of more than one variable

The limit of a function can also be studied when the function has more than one input variable. For example, consider a function that takes two inputs, x and y. We can think about what happens to the function's output when both x and y get close to certain values, say p and q.

There are different ways to approach this idea. One way is to look at what happens when we only let one variable, like x, get close to its value while keeping the other variable fixed. This gives us a new function that depends only on the remaining variable, y. Another way is to take the limit in one variable, and then take the limit of the result with respect to the second variable. The order in which we do this can sometimes change the answer.

Functions on metric spaces

The limit of a function is a way to describe how a function behaves near a certain point, even if that point isn't in the function's domain. In simple terms, it tells us what value the function gets close to as the input gets closer to a specific point.

For example, imagine you have a function that works for numbers very close to 2, but not exactly at 2. The limit helps us understand what the function would do if it could work at 2, based on its behavior around that point. This idea is important in many areas of mathematics, especially calculus.

Other characterizations

There are different ways to think about the limit of a function. One way is by using sequences. If we have a function and we look at a sequence of numbers getting closer and closer to a certain point, the limit tells us what the function values get close to. This idea was studied by mathematicians like Eduard Heine and Sierpiński.

Another way to understand limits is through a special kind of math called non-standard calculus, which uses something called hyperreal numbers. This method looks at how close numbers are to being infinitesimally small. Limits help us understand when a function is continuous, meaning it doesn’t jump or break at a certain point.

Properties

The limit of a function describes how the function behaves near a certain input value. If both the right-handed and left-handed limits at a point exist and are equal, then the overall limit at that point exists and equals this common value.

A function is continuous at a point if its limit at that point equals the function's value at the point. Limits also help us understand how functions behave when we combine them, such as adding, subtracting, multiplying, or dividing functions. There are special rules that make calculating these combined limits easier.

This article is a child-friendly adaptation of the Wikipedia article on Limit of a function, available under CC BY-SA 4.0.

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