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In , a real interval is the set of all lying between two fixed endpoints with no "gaps". Each endpoint is either a real number or positive or negative , indicating the interval extends without a . A real interval can contain neither endpoint, either endpoint, or both endpoints, excluding any endpoint which is infinite.

For example, the set of real numbers consisting of , , and all numbers in between is an interval, denoted and called the ; the set of all positive real numbers is an interval, denoted ; the set of all real numbers is an interval, denoted ; and any single real number is an interval, denoted .

Intervals are ubiquitous in mathematical analysis. For example, they occur implicitly in the epsilon-delta definition of continuity; the intermediate value theorem asserts that the image of an interval by a continuous function is an interval; of are defined over an interval; etc.

Interval arithmetic consists of computing with intervals instead of real numbers for providing a guaranteed enclosure of the result of a numerical computation, even in the presence of uncertainties of and .

Intervals are likewise defined on an arbitrary set, such as or . The notation of integer intervals is considered in the special section below.


Definitions and terminology
An interval is a of the that contains all real numbers lying between any two numbers of the subset. In particular, the \varnothing and the entire set of real numbers \R are both intervals.

The endpoints of an interval are its , and its , if they exist as real numbers.

(1998). 9781886529021, Athena Scientific. .
If the infimum does not exist, one says often that the corresponding endpoint is -\infty. Similarly, if the supremum does not exist, one says that the corresponding endpoint is +\infty.

Intervals are completely determined by their endpoints and whether each endpoint belong to the interval. This is a consequence of the least-upper-bound property of the real numbers. This characterization is used to specify intervals by means of , which is described below.

An does not include any endpoint, and is indicated with parentheses.

(2025). 9780763714970, Jones & Bartlett Publishers. .
For example, (0, 1) = \{x \mid 0 < x < 1\} is the interval of all real numbers greater than and less than . (This interval can also be denoted by , see below). The open interval consists of real numbers greater than , i.e., positive real numbers. The open intervals have thus one of the forms
\begin{align}
(a,b)        &= \{x\in\mathbb R \mid a
\end{align}
where a and b are real numbers such that a< b. In the last case, the resulting interval is the  and does not depend on . The open intervals are those intervals that are  for the usual topology on the real numbers.
     

A is an interval that includes all its endpoints and is denoted with square brackets. For example, means greater than or equal to and less than or equal to . Closed intervals have one of the following forms in which and are real numbers such that a< b\colon

\begin{align}
 \;[a,b]        &= \{x\in\mathbb R \mid a\le x\le b\}, \\
\left(-\infty, b\right] &= \{x\in\mathbb R \mid x\le b\}, \\
\left[a, +\infty\right) &= \{x\in\mathbb R \mid a\le x\}, \\
(-\infty, +\infty) &= \R,\\
\left[a,a\right]&=\{a\}.
     
\end{align} The closed intervals are those intervals that are for the usual topology on the real numbers.

A has two endpoints and includes only one of them. It is said left-open or right-open depending on whether the excluded endpoint is on the left or on the right. These intervals are denoted by mixing notations for open and closed intervals. For example, means greater than and less than or equal to , while means greater than or equal to and less than . The half-open intervals have the form

\begin{align}
\left(a,b\right]       &= \{x\in\R \mid a
\end{align}
     

In summary, a set of the real numbers is an interval, if and only if it is an open interval, a closed interval, or a half-open interval. The only intervals that appear twice in the above classification are and that are both open and closed.

(2025). 9789811017896, Springer. .
See Definition 9.1.1.

A is any (i.e., an interval of the form ).

(1999). 9780691005478, Princeton University Press. .
Some authors include the empty set in this definition. A real interval that is neither empty nor degenerate is said to be proper, and has infinitely many elements.

An interval is said to be left-bounded or right-bounded, if there is some real number that is, respectively, smaller than or larger than all its elements. An interval is said to be bounded, if it is both left- and right-bounded; and is said to be unbounded otherwise. Intervals that are bounded at only one end are said to be half-bounded. The empty set is bounded, and the set of all reals is the only interval that is unbounded at both ends. Bounded intervals are also commonly known as finite intervals.

Bounded intervals are , in the sense that their (which is equal to the absolute difference between the endpoints) is finite. The diameter may be called the length, width, measure, range, or size of the interval. The size of unbounded intervals is usually defined as , and the size of the empty interval may be defined as (or left undefined).

The centre () of a bounded interval with endpoints and is , and its radius is the half-length . These concepts are undefined for empty or unbounded intervals.

An interval is said to be left-open if and only if it contains no (an element that is smaller than all other elements); right-open if it contains no ; and open if it contains neither. The interval , for example, is left-closed and right-open. The empty set and the set of all reals are both open and closed intervals, while the set of non-negative reals, is a closed interval that is right-open but not left-open. The open intervals are of the real line in its standard topology, and form a base of the open sets.

An interval is said to be left-closed if it has a minimum element or is left-unbounded, right-closed if it has a maximum or is right unbounded; it is simply closed if it is both left-closed and right closed. So, the closed intervals coincide with the in that topology.

The interior of an interval is the largest open interval that is contained in ; it is also the set of points in which are not endpoints of . The closure of is the smallest closed interval that contains ; which is also the set augmented with its finite endpoints.

For any set of real numbers, the interval enclosure or interval span of is the unique interval that contains , and does not properly contain any other interval that also contains .

An interval is a subinterval of interval if is a of . An interval is a proper subinterval of if is a of .

However, there is conflicting terminology for the terms segment and interval, which have been employed in the literature in two essentially opposite ways, resulting in ambiguity when these terms are used. The Encyclopedia of Mathematics defines interval (without a qualifier) to exclude both endpoints (i.e., open interval) and segment to include both endpoints (i.e., closed interval), while Rudin's Principles of Mathematical Analysis

(1976). 007054235X, McGraw-Hill. . 007054235X
calls sets of the form a, intervals and sets of the form ( a, b) segments throughout. These terms tend to appear in older works; modern texts increasingly favor the term interval (qualified by open, closed, or half-open), regardless of whether endpoints are included.


Notations for intervals
The interval of numbers between and , including and , is often denoted . The two numbers are called the endpoints of the interval. In countries where numbers are written with a , a may be used as a separator to avoid ambiguity.


Including or excluding endpoints
To indicate that one of the endpoints is to be excluded from the set, the corresponding square bracket can be either replaced with a parenthesis, or reversed. Both notations are described in International standard ISO 31-11. Thus, in set builder notation,

\begin{align}
(a,b) = \mathopen{]}a,b\mathclose{} a,b) (a,b] = \mathopen{]}a,b\mathclose{]} &= \{x\in\R \mid a

Each interval , , and represents the , whereas denotes the singleton set }. When , all four notations are usually taken to represent the empty set.

Both notations may overlap with other uses of parentheses and brackets in mathematics. For instance, the notation is often used to denote an in set theory, the of a point or vector in analytic geometry and , or (sometimes) a in . That is why introduced the notation to denote the open interval. The notation too is occasionally used for ordered pairs, especially in .

Some authors such as Yves Tillé use to denote the complement of the interval ; namely, the set of all real numbers that are either less than or equal to , or greater than or equal to .


Infinite endpoints
In some contexts, an interval may be defined as a subset of the extended real numbers, the set of all real numbers augmented with and .

In this interpretation, the notations  ,  ,  , and are all meaningful and distinct. In particular, denotes the set of all ordinary real numbers, while denotes the extended reals.

Even in the context of the ordinary reals, one may use an infinite endpoint to indicate that there is no bound in that direction. For example, is the set of positive real numbers, also written as \mathbb{R}_+. The context affects some of the above definitions and terminology. For instance, the interval  = \R is closed in the realm of ordinary reals, but not in the realm of the extended reals.


Integer intervals
When and are , the notation ⟦ a, b⟧, or or } or just , is sometimes used to indicate the interval of all integers between and included. The notation is used in some programming languages; in Pascal, for example, it is used to formally define a subrange type, most frequently used to specify lower and upper bounds of valid of an array.

Another way to interpret integer intervals are as sets defined by enumeration, using notation.

An integer interval that has a finite lower or upper endpoint always includes that endpoint. Therefore, the exclusion of endpoints can be explicitly denoted by writing  ,  , or . Alternate-bracket notations like or are rarely used for integer intervals.


Properties
The intervals are precisely the subsets of \R. It follows that the image of an interval by any continuous function from \mathbb R to \mathbb R is also an interval. This is one formulation of the intermediate value theorem.

The intervals are also the of \R. The interval enclosure of a subset X\subseteq \R is also the of X.

The closure of an interval is the union of the interval and the set of its finite endpoints, and hence is also an interval. (The latter also follows from the fact that the closure of every of a topological space is a connected subset.) In other words, we have

\operatorname{cl}(a,b)=\operatorname{cl}(a,b]=\operatorname{cl}a,b)=\operatorname{cl}[a,b=a,b,
\operatorname{cl}(a,+\infty)=\operatorname{cl}[a,+\infty)=[a,+\infty),
\operatorname{cl}(-\infty,a)=\operatorname{cl}(-\infty,a]=(-\infty,a],
\operatorname{cl}(-\infty,+\infty)=(-\infty,\infty).

The intersection of any collection of intervals is always an interval. The union of two intervals is an interval if and only if they have a non-empty intersection or an open end-point of one interval is a closed end-point of the other, for example (a,b) \cup b,c = (a,c].

If \R is viewed as a , its are the open bounded intervals , and its are the closed bounded intervals . In particular, the and topologies in the real line coincide, which is the standard topology of the real line.

Any element  of an interval  defines a partition of  into three disjoint intervals 1, 2, 3: respectively, the elements of  that are less than , the singleton x,x = \{x\}, and the elements that are greater than . The parts 1 and 3 are both non-empty (and have non-empty interiors), if and only if is in the interior of . This is an interval version of the trichotomy principle.


Dyadic intervals
A dyadic interval is a bounded real interval whose endpoints are \tfrac{j}{2^n} and \tfrac{j+1}{2^n}, where j and n are integers. Depending on the context, either endpoint may or may not be included in the interval.

Dyadic intervals have the following properties:

  • The length of a dyadic interval is always an integer power of two.
  • Each dyadic interval is contained in exactly one dyadic interval of twice the length.
  • Each dyadic interval is spanned by two dyadic intervals of half the length.
  • If two open dyadic intervals overlap, then one of them is a subset of the other.

The dyadic intervals consequently have a structure that reflects that of an infinite .

Dyadic intervals are relevant to several areas of numerical analysis, including adaptive mesh refinement, multigrid methods and . Another way to represent such a structure is (for ).


Generalizations

Balls
An open finite interval (a, b) is a 1-dimensional open ball with a center at \tfrac12(a + b) and a of \tfrac12(b - a). The closed finite interval a, is the corresponding closed ball, and the interval's two endpoints \{a, b\} form a 0-dimensional . Generalized to n-dimensional , a ball is the set of points whose distance from the center is less than the radius. In the 2-dimensional case, a ball is called a disk.

If a half-space is taken as a kind of degenerate ball (without a well-defined center or radius), a half-space can be taken as analogous to a half-bounded interval, with its boundary plane as the (degenerate) sphere corresponding to the finite endpoint.


Multi-dimensional intervals
A finite interval is (the interior of) a 1-dimensional . Generalized to real coordinate space \R^n, an axis-aligned hyperrectangle (or box) is the Cartesian product of n finite intervals. For n=2 this is a ; for n=3 this is a rectangular cuboid (also called a "box").

Allowing for a mix of open, closed, and infinite endpoints, the Cartesian product of any n intervals, I = I_1\times I_2 \times \cdots \times I_n is sometimes called an n-dimensional interval.

A facet of such an interval I is the result of replacing any non-degenerate interval factor I_k by a degenerate interval consisting of a finite endpoint of I_k. The faces of I comprise I itself and all faces of its facets. The corners of I are the faces that consist of a single point of \R^n.


Convex polytopes
Any finite interval can be constructed as the intersection of half-bounded intervals (with an empty intersection taken to mean the whole real line), and the intersection of any number of half-bounded intervals is a (possibly empty) interval. Generalized to n-dimensional , an intersection of half-spaces (of arbitrary orientation) is (the interior of) a , or in the 2-dimensional case a .


Domains
An open interval is a connected open set of real numbers. Generalized to topological spaces in general, a non-empty connected open set is called a domain.


Complex intervals
Intervals of can be defined as regions of the , either or circular. Complex interval arithmetic and its applications, Miodrag Petković, Ljiljana Petković, Wiley-VCH, 1998,


Intervals in posets and preordered sets

Definitions
The concept of intervals can be defined in arbitrary partially ordered sets or more generally, in arbitrary . For a (X,\lesssim) and two elements a,b\in X, one similarly defines the intervals
(2025). 9783540416838, Springer.
(a,b) =\{x\in X \mid a
a,b =\{x\in X \mid a\lesssim x\lesssim b\},
(a,b] =\{x\in X \mid a
[a,b) =\{x\in X \mid a\lesssim x
(a,\infty) =\{x\in X \mid a
[a,\infty) =\{x\in X \mid a\lesssim x\},
(-\infty,b) =\{x\in X \mid x
(-\infty,b] =\{x\in X \mid x\lesssim b\},
(-\infty,\infty) =X,
where x means x\lesssim y\not\lesssim x. Actually, the intervals with single or no endpoints are the same as the intervals with two endpoints in the larger preordered set
\bar X=X\sqcup\{-\infty,\infty\}
-\infty
defined by adding new smallest and greatest elements (even if there were ones), which are subsets of X. In the case of X=\mathbb R one may take \bar\mathbb R to be the extended real line.


Convex sets and convex components in order theory
A subset A\subseteq X of the (X,\lesssim) is (order-)convex if for every x,y\in A and every x\lesssim z\lesssim y we have z\in A. Unlike in the case of the real line, a convex set of a preordered set need not be an interval. For example, in the totally ordered set (\mathbb Q,\le) of , the set
\mathbb Q=\{x\in\mathbb Q \mid x^2<2\}
is convex, but not an interval of \mathbb Q, since there is no square root of two in \mathbb Q.

Let (X,\lesssim) be a and let Y\subseteq X. The convex sets of X contained in Y form a under inclusion. A of this poset is called a convex component of Y. By the , any convex set of X contained in Y is contained in some convex component of Y, but such components need not be unique. In a totally ordered set, such a component is always unique. That is, the convex components of a subset of a totally ordered set form a partition.


Properties
A generalization of the characterizations of the real intervals follows. For a non-empty subset I of a (L,\le), the following conditions are equivalent.
(2025). 9780131816299, Prentice Hall. .
  • The set I is an interval.
  • The set I is order-convex.
  • The set I is a connected subset when L is endowed with the .

For a S of a lattice L, the following conditions are equivalent.

  • The set S is a and an (order-)convex set.
  • There is an ideal I\subseteq L and a filter F\subseteq L such that S=I\cap F.


Applications

In general topology
Every is embeddable into a of the closed unit intervals 0,1. Actually, every Tychonoff space that has a base of \kappa is embeddable into the product 0,1^\kappa of \kappa copies of the intervals.
(1989). 9783885380061, Heldermann Verlag.

The concepts of convex sets and convex components are used in a proof that every totally ordered set endowed with the is completely normal or moreover, monotonically normal.


Topological algebra
Intervals can be associated with points of the plane, and hence regions of intervals can be associated with regions of the plane. Generally, an interval in mathematics corresponds to an ordered pair taken from the \R \times \R of real numbers with itself, where it is often assumed that . For purposes of mathematical structure, this restriction is discarded,Kaj Madsen (1979), Review of "Interval analysis in the extended interval space" by Edgar Kaucher, and "reversed intervals" where are allowed. Then, the collection of all intervals can be identified with the formed by the direct sum of \R with itself, where addition and multiplication are defined component-wise.

The direct sum algebra ( \R \oplus \R, +, \times) has two ideals, { x,0 : x ∈ R } and { 0, y : y ∈ R }. The of this algebra is the condensed interval . If interval is not in one of the ideals, then it has multiplicative inverse . Endowed with the usual , the algebra of intervals forms a . The group of units of this ring consists of four quadrants determined by the axes, or ideals in this case. The identity component of this group is quadrant I.

Every interval can be considered a symmetric interval around its . In a reconfiguration published in 1956 by M Warmus, the axis of "balanced intervals" is used along with the axis of intervals that reduce to a point. Instead of the direct sum R \oplus R, the ring of intervals has been identifiedD. H. Lehmer (1956) Review of "Calculus of Approximations", with the hyperbolic numbers by M. Warmus and D. H. Lehmer through the identification

z = \tfrac12(x + y) + \tfrac12(x - y)j,
where j^2 = 1.

This linear mapping of the plane, which amounts of a , provides the plane with a multiplicative structure having some analogies to ordinary complex arithmetic, such as polar decomposition.


See also


Bibliography


External links

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