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Section Intervals

We will begin with one of the most basic type of set we will encounter β€” intervals. The open intervals will be important as they will form a basis for the standard topology on R. We are likely familiar with intervals from algebra and calculus, sets like (0,1), [2,3). To really understand intervals, we will need a rigorous definition.

Definition 1.1.

A subset I of R is an interval if for all a, b, and c in R (allowing for a or b to be ±∞) with a<c<b, if a and b are in I, then c is in I.
With this definition, the set of all real numbers x satisfying 0<x<1 is an interval that we denote by (0,1) (it is important to understand the context β€” we also use the notation (0,1) to denote an ordered pair). The general notation we use for intervals is the following:
  • (a,b)={t∈R∣a<t<b} (a or b could be ±∞)
  • [a,b)={t∈R∣a≀t<b} (b could be ±∞)
  • (a,b]={t∈R∣a<t≀b} (a could be ±∞)
  • [a,b]={t∈R∣a≀t≀b}.
In this notation, R=(βˆ’βˆž,∞). Intervals of the form (a,b) are called open intervals, intervals of the form [a,b] are called closed intervals, and intervals of the form [a,b) or (a,b] are half-open (or half-closed) intervals. The reason for this terminology should become more clear as we introduce open and closed sets later.
Note that nothing in the definition indicates that we must have a<b in the interval notation. This implies that (1,1) is an interval. Since there are no real numbers larger than 1 and less than 1, βˆ…=(1,1) is an interval. We could also have an interval of the form [a,a] where a is any real number. This means that {a}=[a,a], and any single point set is an interval. The intervals βˆ… and [a,a] for any real number a are called degenerate intervals.
One last note about intervals. Some require that a be less than b in the definition of an interval, with the result that there are no degenerate intervals. This is a matter of debate that we won’t get into. In almost all of our work, we will consider only non-degenerate intervals so this won’t be an issue for us.