# Undergraduate Mathematics/Fundamental theorem of calculus

Template:Calculus The fundamental theorem of calculus specifies the relationship between the two central operations of calculus, differentiation and integration.

The first part of the theorem, sometimes called the first fundamental theorem of calculus, shows that an indefinite integration[1] can be reversed by a differentiation. The first part is also important because it guarantees the existence of an antiderivatives for continuous functions. [2]

The second part, sometimes called the second fundamental theorem of calculus, allows one to compute the definite integral of a function by using any one of its infinitely many antiderivatives. This part of the theorem has invaluable practical applications, because it markedly simplifies the computation of definite integrals.

The first published statement and proof of a restricted version of the fundamental theorem was by James Gregory (1638–1675)[3]. Isaac Barrow (1630-1677) proved the first completely general version of the theorem, while Barrow's student Isaac Newton (1643–1727) completed the development of the surrounding mathematical theory. Gottfried Leibniz (1646–1716) systematized the knowledge into a calculus for infinitesimal quantities.

## Physical intuition

Intuitively, the theorem simply states that the sum of infinitesimal changes in a quantity over time (or some other quantity) add up to the net change in the quantity.

To comprehend this statement, we will start with an example. Suppose a particle travels in a straight line with its position, x, given by x(t) where t is time and x(t) means that x is a function of t. The derivative of this function is equal to the infinitesimal change in quantity, dx, per infinitesimal change in time, dt (of course, the derivative itself is dependent on time). Let us define this change in distance per change in time as the velocity v of the particle. In Leibniz's notation:

${\displaystyle {\frac {dx}{dt}}=v(t).}$

Rearranging this equation, it follows that:

${\displaystyle dx=v(t)\,dt.}$

By the logic above, a change in x (or Δx) is the sum of the infinitesimal changes dx. It is also equal to the sum of the infinitesimal products of the derivative and time. This infinite summation is integration; hence, the integration operation allows the recovery of the original function from its derivative. As one can reasonably infer, this operation works in reverse as we can differentiate the result of our integral to recover the original.

## Geometric intuition

The area shaded in light red stripes can be computed as h times ƒ(x), or if we knew the function A(x), it could be estimated as A(x + h) − A(x). These two values are approximately equal, particularly for small h.

Suppose we are given a smooth continuous function y = ƒ(x), and have plotted its graph as a curve. Then for each value of x, intuitively it makes sense that there is a corresponding area function A(x), representing the area beneath the curve between 0 and x. We may not know a "formula" for the function A(x), but intuitively we understand that it is simply the area under the curve.

Now suppose we wanted to compute the area under the curve between x and x + h. We could compute this area by finding the area between 0 and x + h, then subtracting the area between 0 and x. In other words, the area of this “sliver” would be A(x + h) − A(x).

There is another way to estimate the area of this same sliver. Multiply h by ƒ(x) to find the area of a rectangle that is approximately the same size as this sliver. In fact, it makes intuitive sense that for very small values of h, the approximation will become very good.

At this point we know that A(x + h) − A(x) is approximately equal to ƒ(xh, and we intuitively understand that this approximation becomes better as h grows smaller. In other words, ƒ(xhA(x + h) − A(x), with this approximation becoming an equality as h approaches 0 in the limit.

Divide both sides of this equation by h. Then we have

${\displaystyle f(x)\approx {\frac {A(x+h)-A(x)}{h}}.}$

As h approaches 0, we recognized that the right hand side of this equation is simply the derivative A’(x) of the area function A(x). The left-hand side of the equation simply remains ƒ(x), since no h is present.

We have shown informally that ƒ(x) = A’(x). In other words, the derivative of the area function A(x) is the original function ƒ(x). Or, to put it another way, the area function is simply the antiderivative of the original function.

What we have shown is that, intuitively, computing the derivative of a function and “finding the area” under its curve are "opposite" operations. This is the crux of the Fundamental Theorem of Calculus. The bulk of the theorem's proof is devoted to showing that the area function A(x) exists in the first place.

## Formal statements

There are two parts to the Fundamental Theorem of Calculus. Loosely put, the first part deals with the derivative of an antiderivative, while the second part deals with the relationship between antiderivatives and definite integrals.

### First part

This part is sometimes referred to as the First Fundamental Theorem of Calculus.[4]

Let ƒ be a continuous real-valued function defined on a closed interval [a, b]. Let F be the function defined, for all x in [a, b], by

${\displaystyle F(x)=\int _{a}^{x}f(t)\,dt\,.}$

Then, F is continuous on [a, b], differentiable on the open interval (ab), and

${\displaystyle F'(x)=f(x)\,}$

for all x in (a, b).

### Corollary

The fundamental theorem is often employed to compute the definite integral of a function ƒ for which an antiderivative g is known. Specifically, if ƒ is a real-valued continuous function on [ab], and g is an antiderivative of ƒ in [ab], then

${\displaystyle \int _{a}^{b}f(x)\,dx=g(b)-g(a).}$

The corollary assumes continuity on the whole interval. This result is strengthened slightly in the following theorem.

### Second part

This part is sometimes referred to as the Second Fundamental Theorem of Calculus.[5]

Let ƒ be a real-valued function defined on a closed interval [a, b]. Suppose that ƒ admits an antiderivative g on [ab], that is, a function such that for all x in [ab],

${\displaystyle f(x)=g'(x)\,}$

(when an antiderivative g exists, then there are infinitely many antiderivatives for ƒ, obtained by adding to g an arbitrary constant. Also, by the first part of the theorem, antiderivatives of ƒ always exist when ƒ is continuous).

If ƒ is integrable on [ab] then

${\displaystyle \int _{a}^{b}f(x)\,dx\,=g(b)-g(a).}$

Notice that the Second part is somewhat stronger than the Corollary because it does not assume that ƒ is continuous.

Note. The second part is also known as Newton-Leibniz Axiom.

## Examples

As an example, suppose you need to calculate

${\displaystyle \int _{2}^{5}x^{2}\,dx.}$

Here, ${\displaystyle f(x)=x^{2}}$ and we can use ${\displaystyle F(x)={x^{3} \over 3}}$ as the antiderivative. Therefore:

${\displaystyle \int _{2}^{5}x^{2}\,dx=F(5)-F(2)={125 \over 3}-{8 \over 3}={117 \over 3}=39.}$

Or, more generally, suppose you need to calculate

${\displaystyle {d \over dx}\int _{0}^{x}t^{3}\,dt.}$

Here, ${\displaystyle f(t)=t^{3}}$ and we can use ${\displaystyle F(t)={t^{4} \over 4}}$ as the antiderivative. Therefore:

${\displaystyle {d \over dx}\int _{0}^{x}t^{3}\,dt={d \over dx}F(x)-{d \over dx}F(0)={d \over dx}{x^{4} \over 4}=x^{3}.}$

But this result could have been found much more easily as

${\displaystyle {d \over dx}\int _{0}^{x}t^{3}\,dt=f(x){dx \over dx}-f(0){d0 \over dx}=x^{3}.}$

## Proof of the First Part

For a given f(t), define the function F(x) as

${\displaystyle F(x)=\int _{a}^{x}f(t)\,dt\,.}$

For any two numbers x1 and x1 + Δx in [a, b], we have

${\displaystyle F(x_{1})=\int _{a}^{x_{1}}f(t)\,dt}$

and

${\displaystyle F(x_{1}+\Delta x)=\int _{a}^{x_{1}+\Delta x}f(t)\,dt\,.}$

Subtracting the two equations gives

${\displaystyle F(x_{1}+\Delta x)-F(x_{1})=\int _{a}^{x_{1}+\Delta x}f(t)\,dt-\int _{a}^{x_{1}}f(t)\,dt.\qquad (1)}$

It can be shown that

${\displaystyle \int _{a}^{x_{1}}f(t)\,dt+\int _{x_{1}}^{x_{1}+\Delta x}f(t)\,dt=\int _{a}^{x_{1}+\Delta x}f(t)\,dt.}$
(The sum of the areas of two adjacent regions is equal to the area of both regions combined.)

Manipulating this equation gives

${\displaystyle \int _{a}^{x_{1}+\Delta x}f(t)\,dt-\int _{a}^{x_{1}}f(t)\,dt=\int _{x_{1}}^{x_{1}+\Delta x}f(t)\,dt.}$

Substituting the above into (1) results in

${\displaystyle F(x_{1}+\Delta x)-F(x_{1})=\int _{x_{1}}^{x_{1}+\Delta x}f(t)\,dt.\qquad (2)}$

According to the mean value theorem for integration, there exists a c in [x1, x1 + Δx] such that

${\displaystyle \int _{x_{1}}^{x_{1}+\Delta x}f(t)\,dt=f(c)\Delta x\,.}$

Substituting the above into (2) we get

${\displaystyle F(x_{1}+\Delta x)-F(x_{1})=f(c)\Delta x\,.}$

Dividing both sides by Δx gives

${\displaystyle {\frac {F(x_{1}+\Delta x)-F(x_{1})}{\Delta x}}=f(c).}$
Notice that the expression on the left side of the equation is Newton's difference quotient for F at x1.

Take the limit as Δx → 0 on both sides of the equation.

${\displaystyle \lim _{\Delta x\to 0}{\frac {F(x_{1}+\Delta x)-F(x_{1})}{\Delta x}}=\lim _{\Delta x\to 0}f(c).}$

The expression on the left side of the equation is the definition of the derivative of F at x1.

${\displaystyle F'(x_{1})=\lim _{\Delta x\to 0}f(c).\qquad (3)}$

To find the other limit, we will use the squeeze theorem. The number c is in the interval [x1, x1 + Δx], so x1cx1 + Δx.

Also, ${\displaystyle \lim _{\Delta x\to 0}x_{1}=x_{1}}$ and ${\displaystyle \lim _{\Delta x\to 0}x_{1}+\Delta x=x_{1}\,.}$

Therefore, according to the squeeze theorem,

${\displaystyle \lim _{\Delta x\to 0}c=x_{1}\,.}$

Substituting into (3), we get

${\displaystyle F'(x_{1})=\lim _{c\to x_{1}}f(c)\,.}$

The function f is continuous at c, so the limit can be taken inside the function. Therefore, we get

${\displaystyle F'(x_{1})=f(x_{1})\,.}$

which completes the proof.

(Leithold et al, 1996)

## Proof of the corollary

Let ${\displaystyle F(x)=\int _{a}^{x}f(t)\,dt.}$  If g is an antiderivative of ƒ, then g and F have the same derivative. It follows that there is a number c such that ${\displaystyle F(x)=g(x)+c\,}$ for all x in [ab]. Letting x = 0,

${\displaystyle 0=g(a)+c\,,}$

which means ${\displaystyle c=-g(a)\,}$. In other words ${\displaystyle F(x)=g(x)-g(a)\,}$ and so

${\displaystyle \int _{a}^{b}f(x)\,dx=g(b)-g(a).}$

## Proof of the Second Part

This is a limit proof by Riemann sums.

Let f be continuous on the interval [a, b], and let F be an antiderivative of f. Begin with the quantity

${\displaystyle F(b)-F(a)\,.}$

Let there be numbers

x1, ..., xn

such that

${\displaystyle a=x_{0}

It follows that

${\displaystyle F(b)-F(a)=F(x_{n})-F(x_{0})\,.}$

Now, we add each F(xi) along with its additive inverse, so that the resulting quantity is equal:

${\displaystyle {\begin{matrix}F(b)-F(a)&=&F(x_{n})\,+\,[-F(x_{n-1})\,+\,F(x_{n-1})]\,+\,\ldots \,+\,[-F(x_{1})+F(x_{1})]\,-\,F(x_{0})\,\\&=&[F(x_{n})\,-\,F(x_{n-1})]\,+\,[F(x_{n-1})\,+\,\ldots \,-\,F(x_{1})]\,+\,[F(x_{1})\,-\,F(x_{0})]\,.\end{matrix}}}$

The above quantity can be written as the following sum:

${\displaystyle F(b)-F(a)=\sum _{i=1}^{n}\,[F(x_{i})-F(x_{i-1})]\,.\qquad (1)}$

Next we will employ the mean value theorem. Stated briefly,

Let F be continuous on the closed interval [a, b] and differentiable on the open interval (a, b). Then there exists some c in (a, b) such that

${\displaystyle F'(c)={\frac {F(b)-F(a)}{b-a}}\,.}$

It follows that

${\displaystyle F'(c)(b-a)=F(b)-F(a).\,}$

The function F is differentiable on the interval [a, b]; therefore, it is also differentiable and continuous on each interval xi-1. Therefore, according to the mean value theorem (above),

${\displaystyle F(x_{i})-F(x_{i-1})=F'(c_{i})(x_{i}-x_{i-1})\,.}$

Substituting the above into (1), we get

${\displaystyle F(b)-F(a)=\sum _{i=1}^{n}\,[F'(c_{i})(x_{i}-x_{i-1})]\,.}$

The assumption implies ${\displaystyle F'(c_{i})=f(c_{i}).}$ Also, ${\displaystyle x_{i}-x_{i-1}}$ can be expressed as ${\displaystyle \Delta x}$ of partition ${\displaystyle i}$.

${\displaystyle F(b)-F(a)=\sum _{i=1}^{n}\,[f(c_{i})(\Delta x_{i})]\,.\qquad (2)}$
A converging sequence of Riemann sums. The numbers in the upper right are the areas of the grey rectangles. They converge to the integral of the function.

Notice that we are describing the area of a rectangle, with the width times the height, and we are adding the areas together. Each rectangle, by virtue of the Mean Value Theorem, describes an approximation of the curve section it is drawn over. Also notice that ${\displaystyle \Delta x_{i}}$ does not need to be the same for any value of ${\displaystyle i}$, or in other words that the width of the rectangles can differ. What we have to do is approximate the curve with ${\displaystyle n}$ rectangles. Now, as the size of the partitions get smaller and n increases, resulting in more partitions to cover the space, we will get closer and closer to the actual area of the curve.

By taking the limit of the expression as the norm of the partitions approaches zero, we arrive at the Riemann integral. We know that this limit exists because f was assumed to be integrable. That is, we take the limit as the largest of the partitions approaches zero in size, so that all other partitions are smaller and the number of partitions approaches infinity.

So, we take the limit on both sides of (2). This gives us

${\displaystyle \lim _{\|\Delta \|\to 0}F(b)-F(a)=\lim _{\|\Delta \|\to 0}\sum _{i=1}^{n}\,[f(c_{i})(\Delta x_{i})]\,.}$

Neither F(b) nor F(a) is dependent on ||Δ||, so the limit on the left side remains F(b) - F(a).

${\displaystyle F(b)-F(a)=\lim _{\|\Delta \|\to 0}\sum _{i=1}^{n}\,[f(c_{i})(\Delta x_{i})]\,.}$

The expression on the right side of the equation defines an integral over f from a to b. Therefore, we obtain

${\displaystyle F(b)-F(a)=\int _{a}^{b}f(x)\,dx\,,}$

which completes the proof.

It almost looks like the first part follows directly from the second because the equation ${\displaystyle g(x)-g(a)=\int _{a}^{x}f}$ where g is an antiderivate of f implies that ${\displaystyle F(x)=\int _{a}^{x}f(t)\,dt\,}$ has the same derivative as g and therefore F' = f. This argument only works if we already know that f has an antiderivative. The only way we know that all continuous functions have antiderivatives is by the first part of the Fundamental Theorem [6] It is important not to interprete the second part of the theorem as the definition of the integral. This is partly because there are many functions that are integrable but lack antiderivatives, and many functions that have antiderivatives are not Reimann integrable (see volterra's function). More importantly, we know that every continuous function is the derivative of some other function only because of the First fundamental theorem of calculus. [7]

For example if f(x) = e−x2 then f has an antiderivative, namely

${\displaystyle g(x)=\int _{0}^{x}f\,}$ and there is no simpler function with this property.

## Generalizations

We don't need to assume continuity of ƒ on the whole interval. Part I of the theorem then says: if ƒ is any Lebesgue integrable function on [a, b] and x0 is a number in [a, b] such that ƒ is continuous at x0, then

${\displaystyle F(x)=\int _{a}^{x}f(t)\,dt}$

is differentiable for x = x0 with F'(x0) = ƒ(x0). We can relax the conditions on ƒ still further and suppose that it is merely locally integrable. In that case, we can conclude that the function F is differentiable almost everywhere and F'(x) = ƒ(x) almost everywhere. On the real line this statement is equivalent to Lebesgue's differentiation theorem. These results remain true for the Henstock–Kurzweil integral which allows a larger class of integrable functions (Bartle 2001, Thm. 4.11).

In higher dimensions Lebesgue's differentiation theorem generalizes the Fundamental theorem of calculus by stating that for almost every x, the average value of a function ƒ over a ball of radius r centered at x will tend to ƒ(x) as r tends to 0.

Part II of the theorem is true for any Lebesgue integrable function ƒ which has an antiderivative F (not all integrable functions do, though). In other words, if a real function F on [ab] admits a derivative ƒ(x) at every  point x of [a, b] and if this derivative ƒ is Lebesgue integrable on [ab], then

${\displaystyle F(b)-F(a)=\int _{a}^{b}f(t)\,\mathrm {d} t.}$    Rudin (1987, th. 7.21)

This result may fail for continuous functions F that admit a derivative ƒ(x) at almost every point x, as the example of the Cantor function shows. But the result remains true if F is absolutely continuous: in that case, F admits a derivative ƒ(x) at almost every point x and, as in the formula above, F(b) − F(a) is equal to the integral of ƒ on [ab].

The conditions of this theorem may again be relaxed by considering the integrals involved as Henstock-Kurzweil integrals. Specifically, if a continuous function F(x) admits a derivative ƒ(x) at all but countably many points, then ƒ(x) is Henstock-Kurzweil integrable and F(b) − F(a) is equal to the integral of ƒ on [ab]. The difference here is that the integrability of ƒ does not need to be assumed. (Bartle 2001, Thm. 4.7)

The version of Taylor's theorem which expresses the error term as an integral can be seen as a generalization of the Fundamental Theorem.

There is a version of the theorem for complex functions: suppose U is an open set in C and ƒ : U → C is a function which has a holomorphic antiderivative F on U. Then for every curve γ : [ab] → U, the curve integral can be computed as

${\displaystyle \int _{\gamma }f(z)\,dz=F(\gamma (b))-F(\gamma (a))\,.}$

The fundamental theorem can be generalized to curve and surface integrals in higher dimensions and on manifolds.

One of the most powerful statements in this direction is Stokes' theorem: Let M be an oriented piecewise smooth manifold of dimension n and let ${\displaystyle \omega }$ be an n−1 form that is a compactly supported differential form on M of class C1. If ∂M denotes the boundary of M with its induced orientation, then

${\displaystyle \int _{M}\mathrm {d} \omega =\oint _{\partial M}\omega \,.}$

Here ${\displaystyle \mathrm {d} \!\,}$ is the exterior derivative, which is defined using the manifold structure only.

The theorem is often used in situations where M is an embedded oriented submanifold of some bigger manifold on which the form ${\displaystyle \omega }$ is defined.