The 13th annual Stanford Mathematics Tournament was held on February 19, 2011. My favorite problem on the contest was the last problem on the calculus subject test.

**Theorem 1** * Compute the integral *

*
** for . *

**Solution 1:**

This integral can be computed using a Riemann sum. Divide the interval of integration into parts to get the Riemann sum

Recall that

We can rewrite this sum of logs as a product and factor the inside to get

The terms are all of the -th roots of unity except for , so the inside product contains all of the factors of except for and . The Riemann sum is therefore equal to

To compute the value of the desired integral, we compute the limit of the Riemann sum as ; this is

(This is problem 471 of Razvan Gelca and Titu Andreescu’s book *Putnam and Beyond*. The solution is due to Siméon Poisson.)

**Solution 2:**

Let the desired integral be , where we think of this integral as a function of the parameter . In this solution, we differentiate by to convert the desired integral to an integral of a rational function in :

All integrals of this form can be computed using the substitution . Then , so and

so our integral becomes

In the first integral, we do the substitution . Then and we have

Therefore, our desired integral is the integral of the previous quantity, or

**Solution 3:**

We use Chebyshev polynomials. First, define the Chebyshev polynomial of the first kind to be . This is a polynomial in , and note that . Note that

so that and hence the Chebyshev polynomials satisfy the recurrence .

Therefore, the Chebyshev polynomials satisfy the generating function

Now, substituting and , we have

So

Then

Now, since

we see that

**Solution 4:**

We can also give a solution based on physics. By symmetry, we can evaluate the integral from to and divide the answer by , so

Now let’s calculate the 2D gravitational potential of a point mass falling along the axis towards a unit circle mass centered around the origin. We set the potential at infinity to . We also note that, since the 2D gravitational force between two masses is proportional to , the potential between two masses is proportional to . So to calculate the gravitational potential, we integrate over the unit circle. But if the point mass is at , then the distance between the point mass and the section of the circle at angle is . So we get the integral

This is exactly the integral we want to calculate! We can also calculate this potential by concentrating the mass of the circle at its center. The circle has mass and its center is distance from the point mass. So the potential is simply . Thus, the final answer is .

**Solution 5:**

This problem also has a solution which uses the Residue Theorem from complex analysis. It is easy to show that

Furthermore, observe that . Thus, our integral is

where the integrals are performed on the real parts of the logarithms in the second expression. In the first integral, substitute , ; the resulting contour integral is

By the Residue Theorem, this is equal to . The second integral is identical. Thus, the final answer is .

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*Related*

Here is another solution. http://sivaramambikasaran.blogspot.com/2013/04/displaystyle-int0pi-ln-1-2a-cosx-a2-dx.html