Continuous Distributions: The Uniform and the Standard Normal
These are the first two continuous distributions of the course, and both compute probabilities as areas under a density curve rather than by summing point masses. The continuous uniform distribution (Definition 12.11) spreads probability evenly over an interval : its density is the constant , so the chance of landing in a subinterval is just its length ratio, . The standard normal (Gaussian) distribution (Definition 12.12) is the famous bell curve, with density symmetric about . Its cumulative distribution function has no closed form, so we read from a standard-normal table or technology and assemble every probability from together with the symmetry rule . We close with Example 12.11, computing , and record the landmark values and .
Before you start — give these a try
Attempting first primes your brain for the lesson — even if you miss. Nothing is graded or saved; it's just a warm-up.
Let . Find . Give your answer as a decimal to places.
True or false: the standard normal distribution is symmetric about , and consequently .
What you’ll be able to do
- State Definition 12.11: a uniform variable has density for (and outside), with cumulative distribution function on .
- Compute uniform probabilities as length ratios, , and recognise that for any single value (so and give the same probability).
- State Definition 12.12: the standard normal has density , symmetric about , with c.d.f. .
- Use the standard-normal table to evaluate , applying the symmetry identity and the facts and as .
- Reproduce Example 12.11 () and the empirical values and .
In your course
· MATH2015 · Linear Algebra & Probability- Definition 12.11Uniform distribution(for ) is equally likely over : density on (else ), and c.d.f. on (with below and at or above ).
- Definition 12.12Standard normal (Gaussian) distributionhas density on and c.d.f. , with the symmetry .
- Example 12.11 via the standard-normal table.
The continuous uniform distribution on $[a,b]$
A uniform variable models a point dropped completely at random on , with no part of the interval favoured over any other (Definition 12.11). Because a continuous variable takes uncountably many values, we cannot give each a positive probability; instead probability is described by a density , and the probability of an event is the area under over that event. 'Equally likely across ' forces to be constant there, and for the total area to equal that constant must be the reciprocal of the width: The graph is a rectangle of width and height , whose area is exactly . This generalises the familiar (height on ) to any interval. Note that the density value is not a probability and may even exceed on a short interval; only areas are probabilities.
Uniform probabilities are length ratios, and single points have probability zero
For a uniform variable the area over a subinterval is a rectangle of height and width , so the fraction of the interval's length that occupies. The c.d.f. accumulates this area from the left: for , rises linearly as for , and equals for ; indeed . A defining feature of every continuous distribution appears here: a single point has zero width, so Consequently the endpoints never matter, , a convenience we exploit throughout.
The standard normal distribution $N(0,1)$
The standard normal (or Gaussian) variable (Definition 12.12) has the bell-shaped density Several features are visible in the formula. It is symmetric about , since (the exponent depends only on ); it peaks at with height ; and it decays extremely fast in both tails because of the factor, yet stays strictly positive for every real . The constant is the normalising factor that makes the total area equal . Unlike the uniform, the normal spreads probability over the whole real line, concentrating it near . The meaning of the parameters and (the mean and variance) is taken up in the next chapter; for now, is simply the standard bell curve.
The standard normal c.d.f. $\Phi$ and its symmetry
Probabilities for come from its cumulative distribution function the area under the bell curve to the left of . This integral has no closed-form antiderivative, so values of are obtained from a standard-normal table or from technology, never by elementary integration. Three facts make the table go a long way. First, any interval probability is a difference, . Second, by symmetry of about , so a table listing only positive covers negative arguments too; in particular , i.e. . Third, as and as . Together these yield the landmark values and .
Let . A random variable has the uniform distribution on , written , if it is equally likely to take any value in that interval. Its probability density function is for and otherwise, and its cumulative distribution function is
A random variable has the standard normal distribution, written , if it has density Its cumulative distribution function is , which has no closed-form expression and is evaluated from tables or technology.
For the c.d.f. satisfies for every real . In particular (so ), while as and as .
For a continuous random variable, for any single value , so and may be used interchangeably. For with , For , .
Worked examples
A uniform variable. Let . Find (a) the value of the density on the interval, (b) , and (c) .
- 1
Identify and . Here and , so the width of the interval is .
- 2
(a) Density value (Definition 12.11). On the density is the constant (and outside). This is a density, not a probability.
- 3
(b) Interval probability as a length ratio. . Equivalently, it is the rectangle of height and width .
- 4
(c) A single point. Since is continuous, a single value has zero width and hence zero area: . (So .)
Example 12.11. Let . Find using the standard-normal c.d.f. .
The one-sigma probability. Let . Express in terms of and give its decimal value.