# 4 The Normal PDF

## 4.1 Sampling from the standard normal distribution

The normal distribution - the familiar bell-shaped distribution - shows up all over the place. In the next chapter on the Central Limit Theorem we’ll see why this is the case but for now just realize that it’s a fundamental part of statistics. R has a set of functions that let you sample from and work with the normal distribution. We’ll start with `rnorm`

(*r* for random, *norm* for normal) which draws random numbers from the normal distribution.

The following code generates a huge sample from a normal distribution with mean 0 and standard deviation of 1, which is called the *standard normal*:

The command `set.seed`

sets the random number generator seed so that the following sequence will always be the same. This way my numbers will look like your numbers if you run this code.

With this huge sample size, hopefully the mean and standard deviation will be close to 0 and 1 respectively:

`## [1] -0.006537039`

`## [1] 1.012356`

Good.

To visualize the distribution of this sample we can plot a histogram after choosing the class intervals. Here’s how we did it in the last chapter on frequency distributions:

## 4.2 Density - the equivalent of relative frequency for continuous data

For discrete data, we calculated the relative frequency distribution by dividing by the sample size. If we do that here with continuous data we have the problem that we picked the class intervals ourselves. So, for example, doubling the width would roughly double the frequencies. To fix this, we divide the frequencies by the sample size but then multiply by the interval width.

The analogue of the relative frequency for continuous data is called the ‘density’, and the graph is called the ‘probability density function’, or ‘pdf’. You can plot the density instead of the frequency using ‘hist’ by setting ‘freq = FALSE’:

With such a large sample size, we can use a very small class interval with to get a better look at the distribution:

```
breaks = seq(-x.range,x.range,.1)
hist(x,main = "",breaks = breaks,xlab = "x",ylab = "Density",freq = FALSE)
```

Notice that even though the intervals are narrow, the height of the graph still peaks at around the same height of about 0.4. This is because the calculation of density takes into account the width of the intervals.

Remember, the relative frequency distribution for discrete data tells you the probability that a given sample will fall into a given category. There is a related relation between density and probability for the pdf: Since the heights of the bars are scaled by their width, the *area*, and not the height, of each bar represents the probability of drawing a sample from that class interval.

The useful thing about this is that you can use the pdf to find the probability of sampling a value within a certain range of class intervals we just sum the areas of the bars that cover that range.

Let’s use this to calculate the probability of obtaining a sample between the values of 0 and 0.5.

In the latest plot, the class interval width in the plot above was set to 0.1. There are 4 intervals that cover the range, and their heights add up to \(0.395+0.381+0.371+0.333 = 1.48\).

Multiplying this sum by the class interval width gives us \((1.48)(0.1) = 0.148\)

This means that about 15% of the scores fall between 0 and 0.5.

## 4.3 The normal pdf

Since we drew samples from the normal distribution, the pdf looks like the familiar bell-curve. With a finite sample we have to use a finite number of class intervals. We could use narrow class intervals because our sample size is large. In theory, with a big enough sample size we could get a smooth-looking pdf. This is a calculus thing: the sample sizes go to infinity but the widths go to zero. In the end, you get a smooth, continuous pdf that is the probability density function of the population that you’re drawing from.

Since it’s a smooth curve, we can describe it as a function of x. The standard normal distribution has a pdf of:

\[ y = \frac{e^{-x^{2}}}{\sqrt{2\pi}} \]

Where \(e\) is the basis of the natural logarithm (one of my favorite numbers). Like \(\pi\), it has a non-repeating decimal that goes on forever. You can use R’s ‘exp’ function to see \(e\) to the first 80 decimal places:

`## [1] "2.71828182845904509079559829842764884233474731445312"`

Sorry for the digression.

Let’s see how well the pdf for the standard normal fits the distribution of our sample by overlaying it on the histogram:

We’ll start plotting pdfs using the ‘ggplot’ function from the ‘ggplot2’ library. ggplot takes a little getting used to, but it’s a very flexible function that allows us to do things like overlay plots.

The following code first runs the `'hist'`

function with `plot=FALSE`

which returns the frequencies without plotting. ‘plot’ also returns the $density. We then use `ggplot`

to plot the density. We’ll use the `geom_step()`

option which plots the bars without the vertical lines at the class intervals. This is cleaner for plots with lots of narrow class intervals. With a large sample size like this we can use narrow class intervals.

```
x.distribution <- hist(x,plot = FALSE,breaks = 200 )
big.data <- data.frame(x=x.distribution$mids,y=x.distribution$density)
p <- ggplot(big.data,aes(x=x,y=y)) + geom_step() + theme_bw() +
scale_x_continuous(breaks = seq(-4,4)) +
geom_hline(yintercept = 0) +
ylab("")
p
```

R has it’s own function, `dnorm`

, that calculates the pdf as a function of x. Here’s the smooth pdf for the standard normal on top of the sample pdf:

```
y <- dnorm(breaks,0,1)
norm.pdf <- data.frame(x=breaks,y=y)
p + geom_line(data =norm.pdf,aes(x=x,y=y),color = 'blue')
```

It’s a nice fit, which demonstrates that R’s random number generator is working well.

## 4.4 Probabilities for the standard normal

Given this smooth pdf, we can use the same trick to find probabilities that scores will fall within certain intervals by calculating the area under the pdf - which is integration in calculus. Frustratingly, although there is that function for the pdf, there is no closed-form integral for that function. But it doesn’t really matter because there are algorithms for approximating the integrals to any degree of precision. R has the `pnorm`

function for this. pnorm finds the area from minus infinity to a desired area. This result should make sense:

`## [1] 0.5`

Since the standard normal is symmetric around zero, half of the area falls below zero.

pnorm is all we need to find the area - and therefore the probability - between two values.

### 4.4.1 Example 1: Find the area above z=1 for the standard normal

We want to find the area of the shaded region:

The trick here is to find the area below 1 and subtract this from 1 since the total area is equal to 1:

`## [1] 0.1586553`

You can get the same answer using the ‘lower.tail’ option which is ‘TRUE’ by default. If set lower.tail=‘FALSE’ it finds the area above:

`## [1] 0.1586553`

### 4.4.2 Example 2: Find the area between -1 and 1

The trick here is to subtract the area below -1 from the area below 1:

`## [1] 0.6826895`

About 2/3 of the total area for the normal distribution falls within \(\pm\) 1 standard deviation from the mean.

### 4.4.3 Example 3: Find the area between 0 and 1/2

Just like the last one:

`## [1] 0.1914625`

Compare this number to 0.148, which is what we got when we added up the areas under the pdf from the sample. It’s pretty close. It’s not exact because our sample, although huge, is finite in size, so we didn’t get the exact number of samples between 0 and 0.5 that’s expected from the actual normal pdf.

### 4.4.4 Example 4: Find the z-score for which the area below is 0.75

This is the reverse of the previous examples: I gave you an area and you have to find the score. R does this with the `qnorm`

function, which is the inverse of the `pnorm`

function:

`## [1] 0.6744898`

So about 67% of the area under the standard normal falls below .75. We can verify this with pnorm:

`## [1] 0.75`

Or to get fancy:

`## [1] 0.75`

The shaded region has an area of 0.75:

### 4.4.5 Example 5: What z-scores bracket the middle 95% of the area under the standard normal?

This is a fun one. If the middle contains 95% of the area, then the two tails each contain a total of 5% of the area. Splitting each tail in half means that each tails contains a proportion of \(\frac{1-.95}{2} = 0.025\) of the area. The score for which the proportion of the area below is .025 is:

`## [1] -1.959964`

The boundary for the upper range is the score for which the proportion below is \(1-.025 = .975\):

`## [1] 1.959964`

You could have guessed that because the standard normal distribution is symmetric around zero.

Here’s the graph:

Remember this number - it’s very close to 2. About 95% of the area of the standard normal falls between -2 and 2. This means that if you were to draw a random sample from the standard normal, it’ll fall outside the range of -2 and 2 about 5% of the time. You’ll see this number, 5%, a lot in the future.

## 4.5 Non-standard normal distributions

All normal distributions have the same shape - they only differ by their means and standard deviations.

Consider IQ scores, which are normalized to have a mean of 100 and a standard deviation of 15.

### 4.5.1 Example 6 What proportion of IQ’s area above 115?

I picked this score because it’s exactly one standard deviation above the mean. All normal distributions have the same shape, so the area is the same as the area above 1 for the standard normal, since the standard deviation of the standard normal is 1, which we calculated in Example 1 as 0.1586553.

It follows that probabilities for any IQ score can be found using the standard normal by converting the score into *standard deviation units*. If \(x\) is your score (IQ in this example), then the score in standard deviation units is:

\[ z = \frac{x-\mu}{\sigma} \]

You can see that the areas are the same in this figure:

You might have noticed that the y-axis scales for these two plots are different. That’s because the scales on the x-axis are different. Although the curves are smooth, you can think of the class interval width for IQs to be 15 times wider than for the z-scores. So in order for the bars to have the same heights, we need to divide the heights of the bars for the IQ scores by 15. That’s why the height in the z-score of 0.3 corresponds to a height in the IQ scores of \(\frac{.3}{15} = 0.02\).

The converted score is called *z-score*.

### 4.5.2 Example 7: What proportion of IQs fall between 100 and 118?

We need to convert the IQ scores to z-scores:

\[ z_1 = \frac{100-100}{15} = 0, z_2 = \frac{118-100}{15} = 1.2 \] So the answer is:

`## [1] 0.3849303`

There is a shortcut that bypasses the need to calculate the two z-scores. `pnorm`

let you pass in the means and standard deviations of your population as arguments. Without them they’re set to the default values of \(\mu = 0\) and \(\sigma = 1\). See how this gives you the same answer:

`## [1] 0.3849303`

Here’s what the areas look like for both the IQ and the standard normal distributions:

### 4.5.3 Example 8: What IQ marks the top 1% of all IQ’s?

Since you have a proportion (.01) we need to use `qnorm`

to find the z-score:

`## [1] 2.326348`

Then we need to find the IQ that is 2.3263479 standard deviations above the mean. This is \(IQ = 100 + (2.3263479)(15):\)

`## [1] 134.8952`

In general, if you have a z-score, we can rearrange the original formula for the z-score:

\[ z = \frac{x-\mu}{\sigma} \]

and solve for x:

\[ x = \mu + z\sigma \]
You might have guessed that `qnorm`

also allows for the shortcut. So the quick way to answer this problem is:

`## [1] 134.8952`

Here’s what that top 1% (above an IQ of about 135) looks like:

### 4.5.4 Example 9: What proportion of women in the world are taller than 70 inches?

For this we need to know something about the distribution of heights of women in the world. Digging around the world wide web, I’ve come up with the estimate that the average height of women in the world globally is 63 inches, with a standard deviation of 2.5 inches.

To solve this problem we’ll use the `pnorm`

function:

`## [1] 0.00255513`

This is a tiny proportion. To visualize this we need to zoom in on the upper tail of the distribution:

### 4.5.5 Example 9: What heights cover the middle 50% of the population of the women’s heights?

This can be done with the `qnorm`

function, since we’re given proportions. We know that the proportions in the two tails are 0.25:

`## [1] 61.31378`

`## [1] 64.68622`

The range between the upper 75% and upper 25%, divided by 2, is called the *semi-interquartile-range*, and has it’s own symbol, *Q*. Q for women’s heights is:

`## [1] 1.686224`

From example 2 we calculated that about 2/3 of the area under the normal distribution falls between \(\pm\) 1 standard deviation of the mean. Since \(\pm\) Q covers only the middle 50% it makes sense that Q is smaller than the standard deviation of 2.5 inches.

Here’s what the middle 50% looks like in blue overlaid on \(\pm\) one standard deviation in pink: