Let I=∫∞−∞e−x2dx and I=∫∞−∞e−y2dy
Then I2=∫∞−∞∫∞−∞e−(x2+y2)dxdy
Changing to polar coordinates requires use of the Jacobian r, treated after the evaluation of the integral: I2=∫∞0re−r2dr∫2π0dθ
I2=2π∫∞0re−r2dr
I2=2π[−12e−r2]∞0=π
Therefore I=√π and ∫∞−∞e−x2dx=√π
Now, about the Jacobian, let's suppose that x and y are functions of both u and v, that is x=g(u,v) and y=h(u,v). The Jacobian is defined as: ∂(x,y)∂(u,v)=|∂x∂u∂x∂v∂y∂u∂y∂v|
Let's work with the specific change from rectangular to polar coordinates that is used in the solution to the Gaussian Integral.
We have x=rcosθ and y=rsinθ
This means that ∂x∂r=cosθ and ∂x∂θ=−rsinθ
Also ∂y∂r=sinθ and ∂y∂θ=rcosθ. Thus: ∂(x,y)∂(r,θ)=|cosθ−rsinθsinθrcosθ|
The determinant evaluates to rcos2θ+rsin2θ=r (the value of the Jacobian).
The Gaussian Integral is closely connected with the normal distribution via the probability density function ϕ(x)=1√2πe−12x2, where ∫∞−∞ϕ(x)dx=1√2π∫∞−∞e−12x2dx=1
Wikipedia states that "in statistics one often uses the related error function, or erf(x), defined as the probability of a random variable with normal distribution of mean 0 and variance 1/2 falling in the range [−x,x]"; that is: erf(x)=1√π∫x−xe−t2dt
Here is an informative video which explains why π appears as the evaluation of the integral. It also explains how the double integral used to evaluate the integral is two dimensional and is finding the volume under a surface. By using the shell method to evaluate the integral, the need for the Jacobian is avoided:
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