Normal distribution
01 Theory
Theory 1
Normal distribution
A variable has a normal distribution, written or “ is Gaussian ,” when it has PDF given by:
The standard normal is and its PDF is usually denoted by :
The standard normal CDF is usually denoted by :
- To show that is a valid probability density, we must show that .
- This calculation is not trivial; it requires a double integral in polar coordinates!
- There is no explicit antiderivative of
- A computer is needed for numerical calculations.
- A chart of approximate values of is provided for exams.
- To check that :
- Observe that is an odd function, i.e. symmetric about the -axis.
- One must then simply verify that the improper integral converges.
- To check that :
- Since , we find:
- Use integration by parts to compute that . (Select and .)
General and standard normals
Assume that and are constants. Define . Then:
That is, has the distribution type .
Derivation of PDF of
Suppose that . Then:
Differentiate to find :
From this fact we can infer that and whenever .
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02 Illustration
Example - Basic generalized normal calculation
Basic generalized normal calculation
Suppose . Find .
Solution
First write as a linear transformation of :
Then:
Look in a table to find that and therefore:
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Example - Gaussian: interval of
Gaussian: interval of 2/3
Find the number such that .
Solution
First convert the question:
Solve for so that this value is :
Use a table to conclude .
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Example - Heights of American males
Heights of American males
Suppose that the height of an American male in inches follows the normal distribution .
(a) What percent of American males are over 6 feet, 2 inches tall?
(b) What percent of those over 6 feet tall are also over 6 feet, 5 inches tall?
Solution
(a) Let be a random variable measuring the height of American males in inches, so . Thus , and:
(b) We seek as the answer. Compute as follows:
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Example - Variance of normal from CDF table
Variance of normal from CDF table
Suppose , and suppose you know .
Find the approximate value of using a table.
Solution
So and thus . Then:
so .
Looking in the chart of for the nearest inverse of 0.8, we obtain , hence .
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