Approximate equality s of regular
n-sided
polygons that
circumscribe the
unit circle approximates 2\pi.
Numerical analysis is the study of
constructive methods and
algorithms to find numerical
approximations (as opposed to
symbolic manipulations) of solutions to problems in
mathematical analysis. Especially those which cannot be
solved analytically. Calculations are likely to involve
rounding errors and other
approximation errors.
Log tables, slide rules, and calculators produce approximate answers to all but the simplest calculations. The results of computer calculations are normally an approximation, expressed in a limited number of significant digits, although they can be programmed to produce more precise results. If approximate equality is viewed as a
binary relation (denoted by the symbol \approx) between
real numbers or other things, any rigorous definition of it will not be an equivalence relation, due to its not being transitive. This is the case even when it is modeled as a
fuzzy relation. In
computer science, equality is expressed using
relational operators. On computers, physical constraints fundamentally limit the level of precision with which numbers can be represented. Thus, the real numbers are often approximated by
floating-point numbers. Each floating-point number is represented as a
significand—comprising some fixed-length sequence of digits in a given base—which is scaled by some integer
exponent of said base, in effect enabling the
radix point to "float" between each possible location in the significand. This allows numbers spanning many orders of magnitude to be represented, but only as fuzzy ranges of values that become less precise as they increase in magnitude. In order to avoid losing precision, it is common to represent real numbers on computers in the form of an
expression that denotes the real number. However, the equality of two real numbers given by an expression is known to be
undecidable (specifically, real numbers defined by expressions involving the
integers, the basic
arithmetic operations, the
logarithm and the
exponential function). In other words, there cannot exist any
algorithm for deciding such an equality (see
Richardson's theorem).
Equivalence relation An
equivalence relation is a
mathematical relation that generalizes the idea of similarity or sameness. It is defined on a
set X as a
binary relation \sim that satisfies the three properties:
reflexivity,
symmetry, and
transitivity. Reflexivity means that every element in X is equivalent to itself (a \sim a for all a \in X). Symmetry requires that if one element is equivalent to another, the reverse also holds (a \sim b \implies b \sim a). Transitivity ensures that if one element is equivalent to a second, and the second to a third, then the first is equivalent to the third (a \sim b and b \sim c \implies a \sim c). These properties are enough to
partition a set into disjoint
equivalence classes. Conversely, every partition defines an equivalence class. The equivalence relation of equality is a special case, as, if restricted to a given set S, it is the strictest possible equivalence relation on S; specifically, equality partitions a set into equivalence classes consisting of all
singleton sets. Other equivalence relations, since they're less restrictive, generalize equality by identifying elements based on shared properties or transformations, such as
congruence in modular arithmetic or
similarity in geometry.
Congruence relation In
abstract algebra, a
congruence relation extends the idea of an equivalence relation to include the
function-application property. That is, given a set X, and a set of operations on X, then a congruence relation \sim has the property that a \sim b \implies f(a) \sim f(b) for all operations f (here, written as unary to avoid cumbersome notation, but f may be of any
arity). A congruence relation on an
algebraic structure such as a
group,
ring, or
module is an equivalence relation that respects the operations defined on that structure.
Isomorphism In mathematics, especially in
abstract algebra and
category theory, it is common to deal with objects that already have some internal
structure. An
isomorphism describes a kind of structure-preserving correspondence between two objects, establishing them as essentially identical in their structure or properties. More formally, an isomorphism is a bijective
mapping (or
morphism) f between two
sets or structures A and B such that f and its inverse f^{-1} preserve the
operations,
relations, or
functions defined on those structures. This means that any operation or relation valid in A corresponds precisely to the operation or relation in B under the mapping. For example, in
group theory, a
group isomorphism f: G \mapsto H satisfies f(a * b) = f(a) * f(b) for all elements a, b, where * denotes the group operation. When two objects or systems are isomorphic, they are considered indistinguishable in terms of their internal structure, even though their elements or representations may differ. For instance, all
cyclic groups of order \infty are isomorphic to the integers, \Z, with addition. Similarly, in
linear algebra, two
vector spaces are isomorphic if they have the same
dimension, as there exists a
linear bijection between their elements. The concept of isomorphism extends to numerous branches of mathematics, including
graph theory (
graph isomorphism),
topology (
homeomorphism), and algebra (group and
ring isomorphisms), among others. Isomorphisms facilitate the classification of mathematical entities and enable the transfer of results and techniques between similar systems. Bridging the gap between isomorphism and equality was one motivation for the development of
category theory, as well as for
homotopy type theory and
univalent foundations.
Geometry with one another, and are both
similar to the third triangle. The rightmost triangle is neither congruent nor similar to any of the others. In
geometry, formally, two figures are equal if they contain exactly the same
points. However, historically, geometric-equality has always been taken to be much broader.
Euclid and
Archimedes used "equal" ( ) often referring to figures with the same area or those that could be cut and rearranged to form one another. For example, Euclid stated the
Pythagorean theorem as "the square on the hypotenuse is equal to the squares on the sides, taken together", and Archimedes said that "a circle is equal to the rectangle whose sides are the radius and half the circumference." (See .) This notion persisted until
Adrien-Marie Legendre introduced the term "equivalent" in 1867 to describe figures of equal area, and reserved "equal" to mean "
congruent"the same
shape and
size, or if one has the same shape and size as the
mirror image of the other. Euclid's terminology continued in the work of
David Hilbert in his '''', who further refined Euclid's ideas by introducing the notions of polygons being "divisibly equal" () if they can be cut into finitely many triangles which are congruent, and "equal in content" () if one can add finitely many divisibly equal polygons to each such that the resulting polygons are divisibly equal. After the rise of set theory, around the 1960s, there was a push for a reform in
mathematics education called "
New Math", following
Andrey Kolmogorov, who, in an effort to restructure Russian geometry courses, proposed presenting geometry through the lens of
transformations and set theory. Since a figure was seen as a set of points, it could only be equal to itself, as a result of Kolmogorov, the term "congruent" became standard in schools for figures that were previously called "equal", which popularized the term. While Euclid addressed
proportionality and figures of the same shape, it was not until the 17th century that the concept of
similarity was formalized in the modern sense. Similar figures are those that have the same shape but can differ in size; they can be transformed into one another by
scaling and congruence. Later a concept of equality of
directed line segments,
equipollence, was advanced by
Giusto Bellavitis in 1835. == See also ==