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This article is about intervals of real numbers. For intervals in general, see partially ordered set. In mathematics, a (real) interval is a set of real numbers with the property that any number that lies between two numbers in the set is also included in the set. For example, the set of all numbers x satisfying In fact, intervals are meaningful in any (totally or partially) ordered set, not just in the reals; so one can have intervals of rational numbers, integers, computer-representable floating point numbers, or subsets of a set (ordered by inclusion), for example. Real intervals play an important role in the theory of integration, because they are the simplest sets whose "size" or "measure" or "length" is easy to define. The concept of measure can then be extended to more complicated sets of real numbers, leading to the Borel measure and eventually to the Lebesgue measure. Intervals are central to interval arithmetic, a general numerical computing technique that automatically provides guaranteed enclosures for arbitrary formulas, even in the presence of uncertainties, mathematical approximations, and arithmetic roundoff.
[edit] Notations for intervalsThe interval of numbers between a and b, including a and b, is often denoted [a,b]. The two numbers are called the endpoints of the interval. [edit] Excluding the endpointsTo indicate that one of the endpoints is to be excluded from the set, many writers substitute a parenthesis for the corresponding square bracket. Thus, in set builder notation, Note that (a,a), [a,a), and (a,a] denote the empty set, whereas [a,a] denotes the set {a}. When a > b, all four notations are usually assumed to represent the empty set. [edit] The ISO notationInternational standard ISO 31-11 also defines another notation for intervals, which seems to be more commonly taught in Europe[citation needed] and South America. It uses an inwards pointing bracket to indicate inclusion of the endpoint, and outwards-pointing bracket for exclusion: Both notations may overlap with other uses of parentheses and brackets in mathematics. For instance, the notation (a,b) is often used to denote an ordered pair in set theory, the coordinates of a point or vector in analytic geometry and linear algebra, or (sometimes) a complex number in algebra. The notation [a,b] too is occasionally used for ordered pairs, especially in computer science. Some authors use ]a,b[ to denote the complement of the interval (a,b); namely, the set of all real numbers that are either less than or equal to a, or greater than or equal to b. In countries where numbers are written with a decimal comma, a semicolon may be used as a separator, to avoid ambiguity. [edit] Infinite endpointsIn both styles of notation, one may use an infinite endpoint to indicate that there is no bound in that direction. Specifically, one may use The notations [edit] Integer intervalsWhen a and b are integers, the 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 [edit] TerminologyAn open interval does not include its endpoints, and is indicated with parentheses. For example (0,1) means greater than 0 and less than 1. Conversely, a closed interval includes its endpoints, and is denoted with square brackets. For example [0,1] means greater than or equal to 0 and less than or equal to 1. A degenerate interval is any set consisting of a single real number. Some authors include the empty set in this definitions. An 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 bounded sets, in the sense that their diameter (which is equal to the absolute difference between the endpoints) is finite. The diameter may be called the length, width, measure, or size of the interval. The size of unbounded intervals is usually defined as The centre of bounded interval with endpoints a and b is (a + b) / 2, and its radius is the half-length An interval is said to be left-open if and only if it has no minimum (an element that is smaller than all other elements); right-open if it has no maximum; and open if it has both properties. The interval An interval is said to be left-closed if it has a minimum element, right-closed if it has a maximum, and simply closed if it has both. These definitions are usually extended to include the empty set and to the (left- or right-) unbounded intervals, so that the closed intervals coincide with closed sets in that topology. The interior of an interval I is the largest open interval that is contained in I; it is also the set of points in I which are not endpoints of I. The closure of I is the smallest closed interval that contains I; which is also the set I augmented with its finite endpoints. For any set X of real numbers, the interval enclosure or interval span of X is the unique interval that contains X and does not properly contain any other interval that also contains X. [edit] Classification of intervalsThe intervals of real rumbers can be classified into eleven different types, listed below; where a and b are real numbers, with a < b:
[edit] Intervals of the extended real lineIn some contexts, an interval may be defined as a subset of the extended real numbers, the set of all real numbers augmented with In this interpretation, the notations This choice affects some of the above definitions and terminology. For instance, the interval [edit] Properties of intervalsThe intervals are precisely the connected subsets of The intervals are also the convex subsets of 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 (e.g., If Any element x of an interval I defines a partition of I into three disjoint intervals I1,I2,I3: respectively, the elements of I that are less than x, the singleton [x,x] = {x}, and the elements that are greater than x. The parts I1 and I3 are both non-empty (and have non-empty interiors) if and only if x is in the interior of I. This is an interval version of the trichotomy principle. [edit] Dyadic intervalsA dyadic interval is a bounded real interval whose endpoints are Dyadic intervals have some nice properties, such as the following:
The dyadic intervals thus have a structure very similar to an infinite binary tree. Dyadic intervals are relevant to several areas of numerical analysis, including adaptive mesh refinement, multigrid methods, and wavelet analysis. [edit] Multi-dimensional intervalsIn many contexts, an n-dimensional interval is defined as a subset of For n = 2, this generally defines a rectangle whose sides are parallel to the coordinate axes; for n = 3, it defines an axis-aligned rectangular box. A facet of such an interval I is the result of replacing any non-degenerate interval factor Ik by a degenerate interval consisting of a finite endpoint of Ik. 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 [edit] See also[edit] References[edit] External links
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