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TECHNIQUES OF INTEGRATION

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7

TECHNIQUES OF INTEGRATION

There are two situations in which it is impossible to find the exact value of a definite integral.

The first situation arises from the fact that, in order to evaluate using the Fundamental Theorem of Calculus (FTC), we need to know an antiderivative of f.

However, sometimes, it is difficult, or even impossible, to find an antiderivative (Section 7.5).

- For example, it is impossible to evaluate the following integrals exactly:

The second situation arises when the function is determined from a scientific experiment through instrument readings or collected data.

- There may be no formula for the function (as we will see in Example 5).

In both cases, we need to find approximate values of definite integrals.

TECHNIQUES OF INTEGRATION

7.7Approximate Integration

In this section, we will learn:

How to find approximate values

of definite integrals.

We already know one method for approximate integration.

- Recall that the definite integral is defined as a limit of Riemann sums.
- So, any Riemann sum could be used as an approximation to the integral.

If we divide [a, b] into n subintervals of equal length âˆ†x = (b â€“ a)/n, we have:

where xi* is any point in the i th subinterval [xi -1, xi].

Equation 1

If xi* is chosen to be the left endpoint of the interval, then xi* = xi -1 and we have:

- The approximation Ln is called the left endpoint approximation.

If f(x) â‰¥ 0, the integral represents an area and Equation 1 represents an approximation of this area by the rectangles shown here.

Equation 2

If we choose xi* to be the right endpoint, xi* = xi and we have:

- The approximation Rniscalled right endpoint approximation.

In Section 5.2, we also considered the case where xi* is chosen to be the midpoint of the subinterval [xi -1, xi].

The figure shows the midpoint approximation Mn.

Mn appears to be better than either Ln or Rn.

where and

Another approximationâ€”called the Trapezoidal Ruleâ€”results from averaging the approximations in Equations 1 and 2, as follows.

where âˆ†x = (b â€“ a)/n and xi = a + i âˆ†x

The reason for the name can be seen from the figure, which illustrates the case f(x) â‰¥ 0.

The area of the trapezoid that lies above the i th subinterval is:

- If we add the areas of all these trapezoids,we get the right side of the Trapezoidal Rule.

Example 1

Approximate the integral with n = 5, using: a. Trapezoidal Rule

b. Midpoint Rule

Example 1 a

With n = 5, a = 1 and b = 2, we have: âˆ†x = (2 â€“ 1)/5 = 0.2

- So, the Trapezoidal Rule gives:

Example 1 a

The approximation is illustrated here.

Example 1 b

The midpoints of the five subintervals are: 1.1, 1.3, 1.5, 1.7, 1.9

Example 1 b

So, the Midpoint Rule gives:

In Example 1, we deliberately chose an integral whose value can be computed explicitly so that we can see how accurate the Trapezoidal and Midpoint Rules are.

- By the FTC,

The error in using an approximation is defined as the amount that needs to be added to the approximation to make it exact.

From the values in Example 1, we see that the errors in the Trapezoidal and Midpoint Rule approximations for n = 5 are:ETâ‰ˆ â€“ 0.002488 EMâ‰ˆ 0.001239

In general, we have:

The tables show the results of calculations similar to those in Example 1.

- However, these are for n = 5, 10, and 20 and for the left and right endpoint approximations and also the Trapezoidal and Midpoint Rules.

We can make several observations from these tables.

In all the methods. we get more accurate approximations when we increase n.

- However, very large values of n result in so many arithmetic operations that we have to beware of accumulated round-off error.

The errors in the left and right endpoint approximations are:

- Opposite in sign
- Appear to decrease by a factor of about 2 when we double the value of n

The Trapezoidal and Midpoint Rules are much more accurate than the endpoint approximations.

The errors in the Trapezoidal and Midpoint Rules are:

- Opposite in sign
- Appear to decrease by a factor of about 4 when we double the value of n

The size of the error in the Midpoint Rule is about half that in the Trapezoidal Rule.

The figure shows why we can usually expect the Midpoint Rule to be more accurate than the Trapezoidal Rule.

The area of a typical rectangle in the Midpoint Rule is the same as the area of the trapezoid ABCD whose upper side is tangent to the graph at P.

The area of this trapezoid is closer to the area under the graph than is the area of that used in the Trapezoidal Rule.

The midpoint error (shaded red) is smaller than the trapezoidal error (shaded blue).

These observations are corroborated in the following error estimatesâ€”which are proved in books on numerical analysis.

Notice that Observation 4 corresponds to the n2 in each denominator because: (2n)2 = 4n2

That the estimates depend on the size of the second derivative is not surprising if you look at the figure.

- fâ€™â€™(x) measures how much the graph is curved.
- Recall that fâ€™â€™(x) measures how fast the slope of y = f(x) changes.

Estimate 3

Suppose | fâ€™â€™(x) | â‰¤ Kfor aâ‰¤ x â‰¤ b.

If ET and EM are the errors in the Trapezoidal and Midpoint Rules, then

Letâ€™s apply this error estimate to the Trapezoidal Rule approximation in Example 1.

- If f(x) = 1/x, then fâ€™(x) = -1/x2 and fâ€™â€™(x) = 2/x3.
- As 1 â‰¤ x â‰¤ 2, we have 1/x â‰¤ 1;so,

So, taking K = 2, a = 1, b = 2, and n = 5 in the error estimate (3), we see:

Comparing this estimate with the actual error of about 0.002488, we see that it can happen that the actual error is substantially less than the upper bound for the error given by (3).

Example 2

How large should we take n in order to guarantee that the Trapezoidal and Midpoint Rule approximations for are accurate to within 0.0001?

Example 2

We saw in the preceding calculation that | fâ€™â€™(x) | â‰¤ 2 for 1 â‰¤ x â‰¤ 2

- So, we can take K = 2, a = 1, and b = 2 in (3).

Example 2

Accuracy to within 0.0001 means that the size of the error should be less than 0.0001

- Therefore, we choose n so that:

Example 2

Solving the inequality for n, we get

or

- Thus, n = 41 will ensure the desired accuracy.

Example 2

Itâ€™s quite possible that a lower value for n would suffice.

- However, 41 is the smallest value for which the error-bound formula can guarantee us accuracy to within 0.0001

Example 2

For the same accuracy with the Midpoint Rule, we choose n so that:

This gives:

Example 3

- Use the Midpoint Rule with n = 10 to approximate the integral
- Give an upper bound for the error involved in this approximation.

Example 3 a

As a = 0, b = 1, and n = 10, the Midpoint Rule gives:

Example 3 a

The approximation is illustrated.

Example 3 b

As f(x) = ex2, we have: fâ€™(x) = 2xex2 and fâ€™â€™(x) = (2 + 4x2)ex2

Also, since 0 â‰¤ x â‰¤ 1, we have x2â‰¤ 1.

Hence, 0 â‰¤ fâ€™â€™(x) = (2 + 4x2) ex2â‰¤ 6e

Example 3 b

Taking K = 6e, a = 0, b = 1, and n = 10 in the error estimate (3), we see that an upper bound for the error is:

Error estimates give upper bounds for the error.

- They are theoretical, worst-case scenarios.
- The actual error in this case turns out to be about 0.0023

Another rule for approximate integration results from using parabolas instead of straight line segments to approximate a curve.

As before, we divide [a, b] into n subintervals of equal length h = âˆ†x = (b â€“ a)/n.

However, this time, we assume n is an evennumber.

Then, on each consecutive pair of intervals, we approximate the curve y = f(x) â‰¥ 0 by a parabola, as shown.

If yi = f(xi), then Pi(xi, yi) is the point on the curve lying above xi.

- A typical parabola passes through three consecutive points: Pi, Pi+1, Pi+2

To simplify our calculations, we first consider the case where: x0 = -h, x1 = 0, x2 = h

We know that the equation of the parabola through P0, P1, and P2is of the form y = Ax2 + Bx + C

Therefore, the area under the parabola from x = - h to x = h is:

However, as the parabola passes through P0(- h, y0), P1(0, y1), and P2(h, y2), we have: y0 = A(â€“ h)2 + B(- h) + C = Ah2 â€“ Bh + C

y1 = C

y2 = Ah2 + Bh + C

Therefore, y0 + 4y1 + y2 = 2Ah2 + 6C

So, we can rewrite the area under the parabola as:

Now, by shifting this parabola horizontally, we do not change the area under it.

This means that the area under the parabola through P0, P1, and P2 from x = x0 to x = x2is still:

Similarly, the area under the parabola through P2, P3, and P4 from x = x2 to x = x4is:

Thus, if we compute the areas under all the parabolas and add the results, we get:

Though we have derived this approximation for the case in which f(x) â‰¥ 0, it is a reasonable approximation for any continuous function f .

- Note the pattern of coefficients: 1, 4, 2, 4, 2, 4, 2, . . . , 4, 2, 4, 1

This is called Simpsonâ€™s Ruleâ€”after the English the English mathematician Thomas Simpson (1710â€“1761).

Rule

where n is even and âˆ†x = (b â€“ a)/n.

Example 4

Use Simpsonâ€™s Rule with n = 10 to approximate

Example 4

Putting f(x) = 1/x, n = 10, and âˆ†x = 0.1 in Simpsonâ€™s Rule, we obtain:

In Example 4, notice that Simpsonâ€™s Rule gives a much better approximation (S10 â‰ˆ 0.693150) to the true value of the integral (ln 2 â‰ˆ 0.693147) than does either:

- Trapezoidal Rule (T10 â‰ˆ 0.693771)
- Midpoint Rule (M10 â‰ˆ 0.692835)

It turns out that the approximations in Simpsonâ€™s Rule are weighted averages of those in the Trapezoidal and Midpoint Rules:

- Recall that ET and EM usually have opposite signs and | EM | is about half the size of | ET |.

In many applications of calculus, we need to evaluate an integral even if no explicit formula is known for y as a function of x.

- A function may be given graphically or as a table of values of collected data.

If there is evidence that the values are not changing rapidly, then the Trapezoidal Rule or Simpsonâ€™s Rule can still be used to find an approximate value for .

Example 5

The figure shows data traffic on the link from the U.S. to SWITCH, the Swiss academic and research network, on February 10, 1998.

- D(t) is the data throughput, measured in megabits per second (Mb/s).

Example 5

Use Simpsonâ€™s Rule to estimate the total amount of data transmitted on the link up to noon on that day.

Example 5

Since we want the units to be consistent and D(t) is measured in Mb/s, we convert the units for t from hours to seconds.

Example 5

If we let A(t) be the amount of data (in Mb) transmitted by time t, where t is measured in seconds, then Aâ€™(t) = D(t).

- So, by the Net Change Theorem (Section 5.4), the total amount of data transmitted by noon (when t = 12 x 602 = 43,200) is:

Example 5

We estimate the values of D(t) at hourly intervals from the graph and compile them here.

Example 5

Then, we use Simpsonâ€™s Rule with n = 12 and âˆ†t = 3600 to estimate the integral, as follows.

Example 5

- The total amount of data transmitted up to noon is 144,000 Mbs, or 144 gigabits.

The table shows how Simpsonâ€™s Rule compares with the Midpoint Rule for the integral , whose true value is about 0.69314718

This table shows how the error Esin Simpsonâ€™s Rule decreases by a factor of about 16 when n is doubled.

That is consistent with the appearance of n4in the denominator of the following error estimate for Simpsonâ€™s Rule.

- It is similar to the estimates given in (3) for the Trapezoidal and Midpoint Rules.
- However, it uses the fourth derivative of f.

Estimate 4

Suppose that | f (4)(x) | â‰¤ Kfor aâ‰¤ x â‰¤ b.

If Es is the error involved in using Simpsonâ€™s Rule, then

Example 6

How large should we take n to guarantee that the Simpsonâ€™s Rule approximation for is accurate to within 0.0001?

Example 6

If f(x) = 1/x, then f (4)(x) = 24/x5.

Since xâ‰¥ 1, we have 1/xâ‰¤ 1, and so

- Thus, we can take K = 24 in (4).

Example 6

So, for an error less than 0.0001, we should choose n so that:

- This gives or

Example 6

Therefore, n = 8 (n must be even) gives the desired accuracy.

- Compare this with Example 2, where we obtained n = 41 for the Trapezoidal Rule and n = 29 for the Midpoint Rule.

Example 7

- Use Simpsonâ€™s Rule with n = 10 to approximate the integral .
- Estimate the error involved in this approximation.

Example 7 a

If n =10, then âˆ†x = 0.1 and the rule gives:

Example 7 b

The fourth derivative of f(x) = ex2 is: f(4)(x) = (12 + 48x2 + 16x4)ex2

So, since 0 â‰¤ x â‰¤ 1, we have: 0 â‰¤ f(4)(x) â‰¤ (12 + 48 +16)e1 = 76e

Example 7 b

Putting K = 76e, a = 0, b = 1, and n = 10 in (4), we see that the error is at most:

- Compare this with Example 3.

Example 7 b

Thus, correct to three decimal places, we have: