Lesson 16: Normal Distributions
Lesson 16: Normal DistributionsOverview
In this lesson, we'll investigate one of the most prevalent probability distributions in the natural world, namely the normal distribution. Just as we have for other probability distributions, we'll explore the normal distribution's properties, as well as learn how to calculate normal probabilities.
Objectives
 To define the probability density function of a normal random variable.
 To learn the characteristics of a typical normal curve.
 To learn how to transform a normal random variable \(X\) into the standard normal random variable \(Z\).
 To learn how to calculate the probability that a normal random variable \(X\) falls between two values \(a\) and \(b\), below a value \(c\), or above a value \(d\).
 To learn how to read standard normal probability tables.
 To learn how to find the value \(x\) associated with a cumulative normal probability.
 To explore the key properties, such as the momentgenerating function, mean and variance, of a normal random variable.
 To investigate the relationship between the standard normal random variable and a chisquare random variable with one degree of freedom.
 To learn how to interpret a \(Z\)value.
 To learn why the Empirical Rule holds true.
 To understand the steps involved in each of the proofs in the lesson.
 To be able to apply the methods learned in the lesson to new problems.
16.1  The Distribution and Its Characteristics
16.1  The Distribution and Its Characteristics Normal Distribution

The continuous random variable \(X\) follows a normal distribution if its probability density function is defined as:
\(f(x)=\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x\mu}{\sigma}\right)^2\right\}\)
for \(\infty<x<\infty\), \(\infty<\mu<\infty\), and \(0<\sigma<\infty\). The mean of \(X\) is \(\mu\) and the variance of \(X\) is \(\sigma^2\). We say \(X\sim N(\mu, \sigma^2)\).
With a first exposure to the normal distribution, the probability density function in its own right is probably not particularly enlightening. Let's take a look at an example of a normal curve, and then follow the example with a list of the characteristics of a typical normal curve.
Example 161
Let \(X\) denote the IQ (as determined by the StanfordBinet Intelligence Quotient Test) of a randomly selected American. It has long been known that \(X\) follows a normal distribution with mean 100 and standard deviation of 16. That is, \(X\sim N(100, 16^2)\). Draw a picture of the normal curve, that is, the distribution, of \(X\).
Note that when drawing the above curve, I said "now what a standard normal curve looks like... it looks something like this." It turns out that the term "standard normal curve" actually has a specific meaning in the study of probability. As we'll soon see, it represents the case in which the mean \(\mu\) equals 0 and the standard deviation σ equals 1. So as not to cause confusion, I wish I had said "now what a typical normal curve looks like...." Anyway, on to the characteristics of all normal curves!
Characteristics of a Normal Curve
It is the following known characteristics of the normal curve that directed me in drawing the curve as I did so above.

All normal curves are bellshaped with points of inflection at \(\mu\pm \sigma\).
ProofThe proof is left for you as an exercise

All normal curves are symmetric about the mean \(\mu\).
ProofAll normal curves are symmetric about the mean \(\mu\), because \(f(\mu+x)=f(\mux)\) for all \(x\). That is:
\(f(\mu+x)=\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x+\mu\mu}{\sigma}\right)^2\right\} =\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x}{\sigma}\right)^2\right\}\)
equals:
\(f(\mux)=\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{\mux\mu}{\sigma}\right)^2\right\} =\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x}{\sigma}\right)^2\right\}=\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x}{\sigma}\right)^2\right\}\)
Therefore, by the definition of symmetry, the normal curve is symmetric about the mean \(\mu\).

The area under an entire normal curve is 1.
ProofWe prove this later on the Normal Properties page. 
All normal curves are positive for all \(x\). That is, \(f(x)>0\) for all \(x\).
ProofThe standard deviation \(\sigma\) is defined to be positive. The square root of \(2\pi\) is positive. And, the natural exponential function is positive. When you multiply positive terms together, you, of course, get a positive number.

The limit of \(f(x)\) as \(x\) goes to infinity is 0, and the limit of \(f(x)\) as \(x\) goes to negative infinity is 0. That is:
\(\lim\limits_{x\to \infty} f(x)=0\) and \(\lim\limits_{x\to \infty} f(x)=0\)
ProofThe function \(f(x)\) depends on \(x\) only through the natural exponential function \(\exp[x^2]\), which is known to approach 0 as \(x\) approaches infinity or negative infinity.

The height of any normal curve is maximized at \(x=\mu\).
ProofUsing what we know from our calculus studies, to find the point at which the maximum occurs, we must differentiate \(f(x)\) with respect to \(x\) and solve for \(x\) to find the maximum. Because our \(f(x)\) contains the natural exponential function, however, it is easier to take the derivative of the natural log of \(f(x)\) with respect to \(x\) and solve for \(x\) to find the maximum. [The maximum of \(f(x)\) is the same as the maximum of the natural log of \(f(x)\), because \(\log_e(x)\) is an increasing function of \(x\). That is, \(x_1<x_2\) implies that \(\log_e(x_1)<\log_e(x_2)\). Therefore, \(f(x_1)<f(x_2)\) implies \(\log_e(f(x_1))<\log_e(f(x_2))\).] That said, taking the natural log of \(f(x)\), we get:
\(\text{log}_e (f(x))=\text{log}\left(\dfrac{1}{\sigma \sqrt{2\pi}} \right)\dfrac{1}{2\sigma^2}(x\mu)^2\)
Taking the derivative of \(\log_e(f(x))\) with respect to \(x\), we get:
\(\dfrac{d\text{log}f(x)}{dx}=\dfrac{1}{2\sigma^2}\cdot 2(x\mu)\)
Now, setting the derivative of \(\log_e(f(x))\) to 0:
\(\dfrac{d\text{log}f(x)}{dx}=\dfrac{1}{2\sigma^2}\cdot 2(x\mu) \stackrel{\equiv}{\scriptscriptstyle{SET}} 0\)
and solving for \(x\), we get that \(x=\mu\). Taking the second derivative of \(\log_e(f(x))\) with respect to \(x\), we get:
\(\dfrac{d^2\text{log}f(x)}{dx^2}=\dfrac{1}{\sigma^2}\)
Because the second derivative of \(\log_e(f(x))\) is negative (for all \(x\), in fact), the point \(x=\mu\) is deemed a local maximum.

The shape of any normal curve depends on its mean \(\mu\) and standard deviation \(\sigma\).
ProofGiven that the curve \(f(x)\) depends only on \(x\) and the two parameters \(\mu\) and \(\sigma\), the claimed characteristic is quite obvious. An example is perhaps more interesting than the proof. Here is a picture of three superimposed normal curves —one of a \(N(0,9)\) curve, one of a \(N(0, 16)\) curve, and one of a \(N(1, 9)\) curve:
As claimed, the shapes of the three curves differ, as the means \(\mu\) and standard deviations \(\sigma\) differ.
16.2  Finding Normal Probabilities
16.2  Finding Normal ProbabilitiesExample 162
Let \(X\) equal the IQ of a randomly selected American. Assume \(X\sim N(100, 16^2)\). What is the probability that a randomly selected American has an IQ below 90?
Solution
As is the case with all continuous distributions, finding the probability involves finding the area under the curve and to the left of the line \(x=90\):
That is:
\(P(X \leq 90)=F(90)=\int^{90}_{\infty} \dfrac{1}{16\sqrt{2\pi}}\text{exp}\left\{\dfrac{1}{2}\left(\dfrac{x100}{16}\right)^2\right\} dx\)
There's just one problem... it is not possible to integrate the normal p.d.f. That is, no simple expression exists for the antiderivative. We can only approximate the integral using numerical analysis techniques. So, all we need to do is find a normal probability table for a normal distribution with mean \(\mu=100\) and standard deviation \(\sigma=16\). Aw, geez, there'd have to be an infinite number of normal probability tables. That strategy isn't going to work! Aha! The cumulative probabilities have been tabled for the \(N(0,1)\) distribution. All we need to do is transform our \(N(100, 16^2)\) distribution to a \(N(0, 1)\) distribution and then use the cumulative probability table for the \(N(0,1)\) distribution to calculate our desired probability. The theorem that follows tells us how to make the necessary transformation.
If \(X\sim N(\mu, \sigma^2)\), then:
\(Z=\dfrac{X\mu}{\sigma}\)
follows the \(N(0,1)\) distribution, which is called the standardized (or standard) normal distribution.
Proof
We need to show that the random variable \(Z\) follows a \(N(0,1)\) distribution. So, let's find the cumulative distribution function \(F(z)\), which is also incidentally referred to as \(\Phi(z)\) in the standard normal case (that's the greek letter phi, read "fee"):
\(F(z)=\Phi(z)=P(Z\leq z)=P \left(\dfrac{X\mu}{\sigma} \leq z \right)\)
which, by rearranging and using the normal p.d.f., equals:
\(F(z)=P(X\leq \mu+z\sigma)=\int^{\mu+z\sigma}_{\infty} \dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x\mu}{\sigma}\right)^2\right\} \)
To perform the integration, let's use the change of variable technique with:
\(w=\dfrac{x\mu}{\sigma}\)
so that:
\(x = \sigma(w) + \mu \) and \(dx = \sigma dw\)
Now for the endpoints of the integral: if \(x=\infty\), then \(w\) also equals \(\infty\); and if \(x=\mu+z\sigma\), then \(w=\frac{\mu+z\sigma \mu}{\sigma}\). Therefore, upon making all of the substitutions for \(x, w\), and \(dx\), our integration looks like this:
\(F(z)=\int^z_{\infty}\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} w^2\right\} \sigma dw\)
And since the \(\sigma\) in the denominator cancels out the \(\sigma\) in the numerator, we get:
\(F(z)=\int^z_{\infty}\dfrac{1}{\sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} w^2\right\} dw\)
We should now recognize that as the cumulative distribution of a normal random variable with mean \(\mu=0\) and standard deviation \(\sigma=1\). Our proof is complete.
The theorem leads us to the following strategy for finding probabilities \(P(z<X<b)\) when \(a\) and \(b\) are constants, and \(X\) is a normal random variable with mean \(\mu\) and standard deviation \(\sigma\):

1) Specify the desired probability in terms of \(X\).

2) Transform \(X, a\), and \(b\), by:
\(Z=\dfrac{X\mu}{\sigma}\)

3) Use the standard normal \(N(0,1)\) table, typically referred to as the \(Z\)table, to find the desired probability.
Reading \(Z\)tables
Standard normal, or \(Z\)tables, can take a number of different forms. There are two standard normal tables, Table Va and Table Vb, in the back of our textbook. Table Va gives the cumulative probabilities for \(Z\)values, to two decimal places, between 0.00 and 3.09. Here's what the top of Table Va looks like:
\begin{aligned} P(Z \leq z)=& \Phi(z)=\int_{\infty}^{z} \frac{1}{\sqrt{2 \pi}} e^{w^{2} / 2} d w \\ \Phi(z) &=1\Phi(z) \end{aligned}
z  0.00  0.01  0.02  0.03  0.04  0.05  0.06  0.07  0.08  0.09 

0.0  0.5000  0.5040  0.5080  0.5120  0.5160  0.5199  0.5239  0.5279  0.5319  0.5359 
0.1  0.5398  0.5438  0.5478  0.5517  0.5557  0.5596  0.5636  0.5675  0.5714  0.5753 
0.2  0.5793  0.5832  0.5871  0.5910  0.5948  0.5987  0.6026  0.6064  0.6103  0.6141 
0.3  0.6179  0.6217  0.6255  0.6293  0.6310  0.6368  0.6406  0.6443  0.6480  0.6517 
0.4  0.6554  0.6591  0.6628  0.6664  0.6700  0.6736  0.6772  0.6808  0.6844  0.6879 
For example, you could use Table Va to find probabilities such as \(P(Z\le 0.01), P(Z\le 1.23)\), or \(P(Z\le 2.98)\). Table Vb, on the other hand, gives probabilities in the upper tail of the standard normal distribution. Here's what the top of Table Vb looks like:
\(P(Z > z_\alpha) = \alpha \)
\(P(Z > z) = 1  \Phi(z) = \Phi(z)\)
\(z_\alpha\)  0.00  0.01  0.02  0.03  0.04  0.05  0.06  0.07  0.08  0.09 

0.0  0.5000  0.4960  0.4920  0.4880  0.4840  0.4801  0.4761  0.4721  0.4681  0.4641 
0.1  0.4602  0.4562  0.4522  0.4483  0.4443  0.4404  0.4364  0.4325  0.4286  0.4247 
0.2  0.4207  0.4168  0.4129  0.4090  0.4520  0.4013  0.3974  0.3936  0.3897  0.3859 
0.3  0.3821  0.3783  0.3745  0.3707  0.3669  0.3632  0.3594  0.3570  0.3557  0.3483 
0.4  0.3446  0.3409  0.3372  0.3336  0.3300  0.3264  0.3228  0.3192  0.3192  0.3121 
That is, for \(Z\)values, to two decimal places, between 0.00 and 3.49, we can use Table Vb to find probabilities such as \(P(Z>0.12), P(Z>1.96)\), and \(P(Z>3.32)\).
Now, we just need to learn how to read the probabilities off of each of the tables. First Table Va:
And, then Table Vb:
Now we know how to read the given \(Z\)tables. Now, we just need to work with some real examples to see that finding probabilities associated with a normal random variable usually involves rewriting the problems just a bit in order to get them to "fit" with the available \(Z\)tables.
Example 162 Continued
Let \(X\) equal the IQ of a randomly selected American. Assume \(X\sim N(100, 16^2)\). What is the probability that a randomly selected American has an IQ below 90?
Answer
Whenever I am faced with finding a normal probability, I always always always draw a picture of the probability I am trying to find. Then, the problem usually just solves itself... oh, how we wish:
So, we just found that the desired probability, that is, that the probability that a randomly selected American has an IQ below 90 is 0.2643. (If you haven't already, you might want to make sure that you can independently read that probability off of Table Vb.)
Now, although I used Table Vb in finding our desired probability, it is worth mentioning that I could have alternatively used Table Va. How's that? Well:
\(P(X<90)=P(Z<0.63)=P(Z>0.63)=1P(Z<0.63)\)
where the first equality comes from the transformation from \(X\) to \(Z\), the second equality comes from the symmetry of the normal distribution, and the third equality comes from the rule of complementary events. Using Table Va to look up \(P(Z<0.63)\), we get 0.7357. Therefore,
\(P(X<90)=1P(Z<0.63)=10.7357=0.2643\)
We should, of course, be reassured that our logic produced the same answer regardless of the method used! That's always a good thing!
What is the probability that a randomly selected American has an IQ above 140?
Answer
Again, I am going to solve this problem by drawing a picture:
So, we just found that the desired probability, that is, that the probability that a randomly selected American has an IQ above 140 is 0.0062. (Again, if you haven't already, you might want to make sure that you can independently read that probability off of Table Vb.)
We again could have alternatively used Table Va to find our desired probability:
\(P(X>140)=P(Z>2.50)=1P(Z<2.50\)
where the first equality comes from the transformation from \(X\) to \(Z\), and the second equality comes from the rule of complementary events. Using Table Va to look up \(P(Z<2.5)\), we get 0.9938. Therefore,
\(P(X>140)=1P(Z<2.50)=10.9938=0.0062\)
Again, we arrived at the same answer using two different methods.
What is the probability that a randomly selected American has an IQ between 92 and 114?
Answer
Again, I am going to solve this problem by drawing a picture:
So, we just found that the desired probability, that is, that the probability that a randomly selected American has an IQ between 92 and 114 is 0.5021. (Again, if you haven't already, you might want to make sure that you can independently read the probabilities that we used to get the answer from Tables Va and Vb.)
The previous three examples have illustrated each of the three possible normal probabilities you could be faced with finding —below some number, above some number, and between two numbers. Once you have mastered each case, then you should be able to find any normal probability when asked.
16.3  Using Normal Probabilities to Find X
16.3  Using Normal Probabilities to Find XOn the last page, we learned how to use the standard normal curve N(0, 1) to find probabilities concerning a normal random variable X with mean \(\mu\) and standard deviation \(\sigma\). What happens if it's not the probability that we want to find, but rather the value of X? That's what we'll investigate on this page. That is, we'll consider what I like to call "insideout" problems, in which we use known probabilities to find the value of the normal random variable X. Let's start with an example.
Example 163
Suppose X, the grade on a midterm exam, is normally distributed with mean 70 and standard deviation 10. The instructor wants to give 15% of the class an A. What cutoff should the instructor use to determine who gets an A?
Solution
My approach to solving this problem is, of course, going to involve drawing a picture:
The instructor now wants to give 10% of the class an A−. What cutoff should the instructor use to determine who gets an A−?
Solution
We'll use the same method as we did previously:
In summary, in order to use a normal probability to find the value of a normal random variable X:

Find the z value associated with the normal probability.

Use the transformation \(x = \mu + z \sigma\) to find the value of x.
16.4  Normal Properties
16.4  Normal PropertiesSo far, all of our attention has been focused on learning how to use the normal distribution to answer some practical problems. We'll turn our attention for a bit to some of the theoretical properties of the normal distribution. We'll start by verifying that the normal p.d.f. is indeed a valid probability distribution. Then, we'll derive the momentgenerating function \(M(t)\) of a normal random variable \(X\). We'll conclude by using the moment generating function to prove that the mean and standard deviation of a normal random variable \(X\) are indeed, respectively, \(\mu\) and \(\sigma\), something that we thus far have assumed without proof.
The Normal P.D.F. is Valid
Recall that the probability density function of a normal random variable is:
\(f(x)=\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} \left(\dfrac{x\mu}{\sigma}\right)^2\right\}\)
for \(\infty<x<\infty\), \(\infty<\mu<\infty\), and \(0<\sigma<\infty\). Also recall that in order to show that the normal p.d.f. is a valid p.d.f, we need to show that, firstly \(f(x)\) is always positive, and, secondly, if we integrate \(f(x)\) over the entire support, we get 1.
Let's start with the easy part first, namely, showing that \(f(x)\) is always positive. The standard deviation \(\sigma\) is defined to be positive. The square root of \(2\pi\) is positive. And, the natural exponential function is positive. When you multiply positive terms together, you, of course, get a positive number. Check... the first part is done.
Now, for the second part. Showing that \(f(x)\) integrates to 1 is a bit messy, so bear with me here. Let's define \(I\) to be the integral that we are trying to find. That is:
\(I=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x\mu)^2\right\}dx\)
Our goal is to show that \(I=1\). Now, if we change variables with:
\(w=\dfrac{x\mu}{\sigma}\)
our integral \(I\) becomes:
\(I=\int_{\infty}^\infty \dfrac{1}{\sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2} w^2\right\}dw\)
Now, squaring both sides, we get:
\(I^2=\left(\int_{\infty}^\infty \dfrac{1}{\sqrt{2\pi}} \text{exp}\left\{\dfrac{x^2}{2} \right\}dx\right) \left(\int_{\infty}^\infty \dfrac{1}{\sqrt{2\pi}} \text{exp}\left\{\dfrac{y^2}{2} \right\}dy\right)\)
And, pulling the integrals together, we get:
\(I^2=\dfrac{1}{2\pi}\int_{\infty}^\infty \int_{\infty}^\infty \text{exp}\left\{\dfrac{x^2}{2} \right\} \text{exp}\left\{\dfrac{y^2}{2} \right\}dxdy\)
Now, combining the exponents, we get:
\(I^2=\dfrac{1}{2\pi}\int_{\infty}^\infty \int_{\infty}^\infty \text{exp}\left\{\dfrac{1}{2}(x^2+y^2) \right\} dxdy\)
Converting to polar coordinates with:
\(x=r\cos\theta\) and \(y=r\sin\theta\)
we get:
\(I^2=\dfrac{1}{2\pi}\int_0^{2\pi}\left(\int_0^\infty \text{exp}\left\{\dfrac{r^2}{2} \right\} rdr\right)d\theta \)
Now, if we do yet another change of variables with:
\(u=\dfrac{r^2}{2}\) and \(du=rdr\)
our integral \(I\) becomes:
\(I^2=\dfrac{1}{2\pi}\int_0^{2\pi}\left(\int_0^\infty e^{u}du\right)d\theta \)
Evaluating the inside integral, we get:
\(I^2=\dfrac{1}{2\pi}\int_0^{2\pi}\left\{\lim\limits_{b\to \infty} [e^{u}]^{u=b}_{u=0}\right\}d\theta \)
And, finally, completing the integration, we get:
\(I^2=\dfrac{1}{2\pi} \int_0^{2\pi} (01) d \theta= \dfrac{1}{2\pi}\int_0^{2\pi} d \theta =\dfrac{1}{2\pi} (2\pi)=1\)
Okay, so we've shown that \(I^2=1\). Therefore, that means that \(I=+1\) or \(I=1\). But, we know that \(I\) must be positive, since \(f(x)>0\). Therefore, \(I\) must equal 1. Our proof is complete. Finally.
The Moment Generating Function
Theorem
The moment generating function of a normal random variable \(X\) is:
\(M(t)=\text{exp}\left\{\mu t+\dfrac{\sigma^2 t^2}{2}\right\}\)
Proof
Well, I better start this proof out by saying this one is a bit messy, too. Jumping right into it, using the definition of a momentgenerating function, we get:
\(M(t)=E(e^{tX})=\int_{\infty}^\infty e^{tx}f(x)dx=\int_{\infty}^\infty e^{tx}\left[\dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x\mu)^2\right\} \right]dx\)
Simply expanding the term in the second exponent, we get:
\(M(t)=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}}\text{exp}\{tx\} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x^22x\mu+\mu^2)\right\} dx\)
And, combining the two exponents, we get:
\(M(t)=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x^22x\mu+\mu^2)+tx \right\} dx\)
Pulling the \(tx\) term into the parentheses in the exponent, we get:
\(M(t)=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x^22x\mu2\sigma^2tx+\mu^2) \right\} dx\)
And, simplifying just a bit more in the exponent, we get:
\(M(t)=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}} \text{exp}\left\{\dfrac{1}{2\sigma^2} (x^22x(\mu+\sigma^2 t)+\mu^2) \right\} dx\)
And, simplifying just a bit more in the exponent, we get:
Now, let's take a little bit of an aside by focusing our attention on just this part of the exponent:
\((x^22(\mu+\sigma^2t)x+\mu^2)\)
If we let:
\(a=\mu+\sigma^2t\) and \(b=\mu^2\)
then that part of our exponent becomes:
\(x^22(\mu+\sigma^2t)x+\mu^2=x^22ax+b\)
Now, complete the square by effectively adding 0:
\(x^22(\mu+\sigma^2t)x+\mu^2=x^22ax+a^2a^2+b\)
And, simplifying, we get:
\(x^22(\mu+\sigma^2t)x+\mu^2=(xa)^2a^2+b\)
Now, inserting in the values we defined for \(a\) and \(b\), we get:
\(x^22(\mu+\sigma^2t)x+\mu^2=(x(\mu+\sigma^2t))^2(\mu+\sigma^2t)^2+\mu^2\)
Okay, now stick our modified exponent back into where we left off in our calculation of the momentgenerating function:
\(M(t)=\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}}\text{exp}\left\{\dfrac{1}{2\sigma^2}\left[(x(\mu+\sigma^2t))^2(\mu+\sigma^2t)^2+\mu^2\right]\right\}dx\)
We can now pull the part of the exponent that doesn't depend on \(x\) through the integral getting:
\(M(t)=\text{exp}\left\{\dfrac{1}{2\sigma^2}\left[(\mu+\sigma^2t)^2+\mu^2\right]\right\} \int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}}\text{exp}\left\{\dfrac{1}{2\sigma^2}\left[(x(\mu+\sigma^2t))^2 \right]\right\}dx\)
Now, we should recognize that the integral integrates to 1 because it is the integral over the entire support of the p.d.f. of a normal random variable \(X\) with:
mean \(\mu+\sigma^2t\) and variance \(\sigma^2\)
That is, because the integral is 1:
\(\int_{\infty}^\infty \dfrac{1}{\sigma \sqrt{2\pi}}\text{exp}\left\{\dfrac{1}{2\sigma^2}\left[(x(\mu+\sigma^2t))^2 \right]\right\}dx = 1\)
\(\text{Since, }\ N(\mu+\sigma^2t, \sigma^2)\)
our momentgenerating function reduces to this:
\(M(t)=\text{exp}\left\{\dfrac{1}{2\sigma^2}\left[\mu^22\mu\sigma^2t\sigma^4t^2+\mu^2\right]\right\}\)
Now, it's just a matter of simplifying:
\(M(t)=\text{exp}\left\{\dfrac{2\mu\sigma^2t+\sigma^4t^2}{2\sigma^2}\right\}\)
and simplifying a bit more:
\(M(t)=\text{exp}\left\{\mu t +\dfrac{\sigma^2t^2}{2}\right\}\)
Our second messy proof is complete!
The Mean and Variance
Theorem
The mean and variance of a normal random variable \(X\) are, respectively, \(\mu\) and \(\sigma^2\).
Proof
We'll use the moment generating function:
\(M(t)=\text{exp}\left\{\mu t +\dfrac{\sigma^2t^2}{2}\right\}\)
to find the mean and variance. Recall that finding the mean involves evaluating the derivative of the momentgenerating function with respect to \(t\) at \(t=0\):
So, we just found that the first derivative of the momentgenerating function with respect to \(t\) is:
\(M'(t)=\text{exp}\left(\mu t +\dfrac{\sigma^2t^2}{2}\right)\times (\mu+\sigma^2t)\)
We'll use it to help us find the variance:
16.5  The Standard Normal and The ChiSquare
16.5  The Standard Normal and The ChiSquareTheorem
We have one more theoretical topic to address before getting back to some practical applications on the next page, and that is the relationship between the normal distribution and the chisquare distribution. The following theorem clarifies the relationship.
If \(X\) is normally distributed with mean \(\mu\) and variance \(\sigma^2>0\), then:
\(V=\left(\dfrac{X\mu}{\sigma}\right)^2=Z^2\)
is distributed as a chisquare random variable with 1 degree of freedom.
Proof
To prove this theorem, we need to show that the p.d.f. of the random variable \(V\) is the same as the p.d.f. of a chisquare random variable with 1 degree of freedom. That is, we need to show that:
\(g(v)=\dfrac{1}{\Gamma(1/2)2^{1/2}}v^{\frac{1}{2}1} e^{v/2}\)
The strategy we'll take is to find \(G(v)\), the cumulative distribution function of \(V\), and then differentiate it to get \(g(v)\), the probability density function of \(V\). That said, we start with the definition of the cumulative distribution function of \(V\):
\(G(v)=P(V\leq v)=P(Z^2 \leq v)\)
That second equality comes, of course, from the fact that \(V=Z^2\). Now, taking note of the behavior of a parabolic function:
we can simplify \(G(v)\) to get:
\(G(v)=P(\sqrt{v} < Z <\sqrt{v})\)
Now, to find the desired probability we need to integrate, over the given interval, the probability density function of a standard normal random variable \(Z\). That is:
\(G(v)= \int^{\sqrt{v}}_{\sqrt{v}}\dfrac{1}{ \sqrt{2\pi}}\text{exp} \left(\dfrac{z^2}{2}\right) dz\)
By the symmetry of the normal distribution, we can integrate over just the positive portion of the integral, and then multiply by two:
\(G(v)= 2\int^{\sqrt{v}}_0 \dfrac{1}{ \sqrt{2\pi}}\text{exp} \left(\dfrac{z^2}{2}\right) dz\)
Okay, now let's do the following change of variables:
\(\text{Let}\ z=\sqrt{y}=y^{1/2}\)
\(\text{So, }\ dz=\frac{1}{2}y^{1/2}\ dy=\frac{1}{z\sqrt{y}}dy\)
\(z^2=y,\ \\ \begin{aligned} z&=0 \Rightarrow y=0 \\ z&=\sqrt{v} \Rightarrow y=v\end{aligned}\)
Doing so, we get:
\(G(v)= 2\int^v_0 \dfrac{1}{ \sqrt{2\pi}}\text{exp} \left(\dfrac{y}{2}\right) \left(\dfrac{1}{2\sqrt{y}}\right) dy\)
\(G(v)= \int^v_0 \dfrac{1}{ \sqrt{\pi}\sqrt{2}} y^{\frac{1}{2}1} \text{exp} \left(\dfrac{y}{2}\right) dy\)
for \(v>0\). Now, by one form of the Fundamental Theorem of Calculus:
\(\text{Given, }\)
\(\int^x_a f(t)dt=F(x)F(a)\)
\(\frac{d}{dx}\int^x_a f(t)dt=F'(x)=f(x)\)
we can take the derivative of \(G(v)\) to get the probability density function \(g(v)\):
\(g(v)=G'(v)= \dfrac{1}{ \sqrt{\pi}\sqrt{2}} v^{\frac{1}{2}1} e^{v/2}\)
for \(0<v<\infty\). If you compare this \(g(v)\) to the first \(g(v)\) that we said we needed to find way back at the beginning of this proof, you should see that we are done if the following is true:
\(\Gamma \left(\dfrac{1}{2}\right)=\sqrt{\pi}\)
It is indeed true, as the following argument illustrates. Because \(g(v)\) is a p.d.f., the integral of the p.d.f. over the support must equal 1:
\(\int_0^\infty \dfrac{1}{ \sqrt{\pi}\sqrt{2}} v^{\frac{1}{2}1} e^{v/2} dv=1\)
Now, change the variables by letting \(v=2x\), so that \(dv=2dx\). Making the change, we get:
\(\dfrac{1}{ \sqrt{\pi}} \int_0^\infty \dfrac{1}{ \sqrt{2}} (2x)^{\frac{1}{2}1} e^{x}2dx=1\)
Rewriting things just a bit, we get:
\(\dfrac{1}{ \sqrt{\pi}} \int_0^\infty \dfrac{1}{ \sqrt{2}}\dfrac{1}{ \sqrt{2}} x^{\frac{1}{2}1} e^{x}2dx=1\)
And simplifying, we get:
\(\dfrac{1}{ \sqrt{\pi}} \int_0^\infty x^{\frac{1}{2}1} e^{x} dx=1\)
Now, it's just a matter of recognizing that the integral is the gamma function of \(\frac{1}{2}\):
\(\dfrac{1}{ \sqrt{\pi}} \Gamma \left(\dfrac{1}{2}\right)=1\)
Our proof is complete.
So, now that we've taken care of the theoretical argument. Let's take a look at an example to see that the theorem is, in fact, believable in a practical sense.
Example 164
Find the probability that the standard normal random variable \(Z\) falls between −1.96 and 1.96 in two ways:
 using the standard normal distribution
 using the chisquare distribution
Solution
The standard normal table (Table V in the textbook) yields:
\(P(1.96<Z<1.96)=P(Z<1.96)P(Z>1.96)=0.9750.025=0.95\)
The chisquare table (Table IV in the textbook) yields the same answer:
\(P(1.96<Z<1.96)=P(Z<1.96)=P(Z^2<1.96^2)=P(\chi^2_{(1)})<3.8416)=0.95\)
16.6  Some Applications
16.6  Some ApplicationsInterpretation of Z
Note that the transformation from \(X\) to \(Z\):
\(Z=\dfrac{X\mu}{\sigma}\)
tells us the number of standard deviations above or below the mean that \(X\) falls. That is, if \(Z=2\), then we know that \(X\) falls 2 standard deviations below the mean. And if \(Z=+2\), then we know that \(X\) falls 2 standard deviations above the mean. As such, \(Z\)scores are sometimes used in medical fields to identify whether an individual exhibits extreme values with respect to some biological or physical measurement.
Example 165
Postmenopausal women are known to be susceptible to severe bone loss known as osteoporosis. In some cases, bone loss can be so extreme as to cause a woman to lose a few inches of height. The spines and hips of women who are suspected of having osteoporosis are therefore routinely scanned to ensure that their bone loss hasn't become so severe to warrant medical intervention.
The mean \(\mu\) and standard deviation \(\sigma\) of the density of the bones in the spine, for example, are known for a healthy population. A woman is scanned and \(x\), the bone density of her spine is determined. She and her doctor would then naturally want to know whether the woman's bone density \(x\) is extreme enough to warrant medical intervention. The most common way of evaluating whether a particular \(x\) is extreme is to use the mean \(\mu\), the standard deviation \(\sigma\), and the value \(x\) to calculate a \(Z\)score. The \(Z\)score can then be converted to a percentile to provide the doctor and the woman an indication of the severity of her bone loss.
Suppose the woman's \(Z\)score is −2.36, for example. The doctor then knows that the woman's bone density falls 2.36 standard deviations below the average bone density of a healthy population. The doctor, furthermore, knows that fewer than 1% of the population have a bone density more extreme than that of his/her patient.
The Empirical Rule Revisited
You might recall earlier in this section, when we investigated exploring continuous data, that we learned about the Empirical Rule. Specifically, we learned that if a histogram is at least approximately bellshaped, then:
 approximately 68% of the data fall within one standard deviation of the mean
 approximately 95% of the data fall within two standard deviations of the mean
 approximately 99.7% of the data fall within three standard deviations of the mean
Where did those numbers come from? Now, that we've got the normal distribution under our belt, we can see why the Empirical Rule holds true. The probability that a randomly selected data value from a normal distribution falls within one standard deviation of the mean is
\(P(1<Z<1)=P(Z<1)P(Z>1)=0.84130.1587=0.6826\)
That is, we should expect 68.26% (approximately 68%!) of the data values arising from a normal population to be within one standard deviation of the mean, that is, to fall in the interval:
\((\mu\sigma, \mu+\sigma)\)
The probability that a randomly selected data value from a normal distribution falls within two standard deviations of the mean is
\(P(2<Z<2)=P(Z<2)P(Z>2)=0.97720.0228=0.9544\)
That is, we should expect 95.44% (approximately 95%!) of the data values arising from a normal population to be within two standard deviations of the mean, that is, to fall in the interval:
\((\mu2\sigma, \mu+2\sigma)\)
And, the probability that a randomly selected data value from a normal distribution falls within three standard deviations of the mean is:
\(P(3<Z<3)=P(Z<3)P(Z>3)=0.99870.0013=0.9974\)
That is, we should expect 99.74% (almost all!) of the data values arising from a normal population to be within three standard deviations of the mean, that is, to fall in the interval:
\((\mu3\sigma, \mu+3\sigma)\)
Let's take a look at an example of the Empirical Rule in action.
Example 166
The left arm length, in inches, of 213 students were measured. Here's the resulting data, and a picture of a dot plot of the resulting arm lengths:
As you can see, the plot suggests that the distribution of the data is at least bellshaped enough to warrant the assumption that \(X\), the left arm lengths of students, is normally distributed. We can use the raw data to determine that the average arm length of the 213 students measured is 25.167 inches, while the standard deviation is 2.095 inches. We'll then use 25.167 as an estimate of \(\mu\), the average left arm length of all college students, and 2.095 as an estimate of \(\sigma\), the standard deviation of the left arm lengths of all college students.
The Empirical Rule tells us then that we should expect approximately 68% of all college students to have a left arm length between:
\(\bar{x}s=25.1672.095=23.072\) and \(\bar{x}+s=25.167+2.095=27.262\)
inches. We should also expect approximately 95% of all college students to have a left arm length between:
\(\bar{x}2s=25.1672(2.095)=20.977\) and \(\bar{x}+2s=25.167+2(2.095)=29.357\)
inches. And, we should also expect approximately 99.7% of all college students to have a left arm length between:
\(\bar{x}3s=25.1673(2.095)=18.882\) and \(\bar{x}+3s=25.167+3(2.095)=31.452\)
Let's see what percentage of our 213 arm lengths fall in each of these intervals! It takes some work if you try to do it by hand, but statistical software can quickly determine that:
 143, or 67.14%, of the 213 arm lengths fall in the first interval
 204, or 95.77%, of the 213 arm lengths fall in the second interval
 213, or 100%, of the 213 arm lengths fall in the third interval
The Empirical Rule didn't do too badly, eh?