In mathematical analysis, a null set is a Lebesgue measurable set of real numbers that has measure zero. This can be characterized as a set that can be covered by a countable union of intervals of arbitrarily small total length.
The notion of null set should not be confused with the empty set as defined in set theory. Although the empty set has Lebesgue measure zero, there are also non-empty sets which are null. For example, any non-empty countable set of real numbers has Lebesgue measure zero and therefore is null.
More generally, on a given measure space a null set is a set such that
Every finite or countably infinite subset of the real numbers is a null set. For example, the set of natural numbers , the set of rational numbers and the set of algebraic numbers are all countably infinite and therefore are null sets when considered as subsets of the real numbers.
The Cantor set is an example of an uncountable null set. It is uncountable because it contains all numbers between 0 and 1 whose ternary form contains only 0's and 2's in their decimal expansion, and it is null because it is constructed by beginning with the closed interval of real numbers from 0 to 1 and multiplying the length by 2/3 continuously.
Suppose is a subset of the real line such that for every there exists a sequence of open intervals (where interval has length such that then is a null set, [1] also known as a set of zero-content.
In terminology of mathematical analysis, this definition requires that there be a sequence of open covers of for which the limit of the lengths of the covers is zero.
Let be a measure space. We have:
Together, these facts show that the null sets of form a 𝜎-ideal of the 𝜎-algebra . Accordingly, null sets may be interpreted as negligible sets, yielding a measure-theoretic notion of "almost everywhere".
The Lebesgue measure is the standard way of assigning a length, area or volume to subsets of Euclidean space.
A subset of has null Lebesgue measure and is considered to be a null set in if and only if:
This condition can be generalised to using -cubes instead of intervals. In fact, the idea can be made to make sense on any manifold, even if there is no Lebesgue measure there.
For instance:
If is Lebesgue measure for and π is Lebesgue measure for , then the product measure In terms of null sets, the following equivalence has been styled a Fubini's theorem: [2]
Null sets play a key role in the definition of the Lebesgue integral: if functions and are equal except on a null set, then is integrable if and only if is, and their integrals are equal. This motivates the formal definition of spaces as sets of equivalence classes of functions which differ only on null sets.
A measure in which all subsets of null sets are measurable is complete . Any non-complete measure can be completed to form a complete measure by asserting that subsets of null sets have measure zero. Lebesgue measure is an example of a complete measure; in some constructions, it is defined as the completion of a non-complete Borel measure.
The Borel measure is not complete. One simple construction is to start with the standard Cantor set which is closed hence Borel measurable, and which has measure zero, and to find a subset of which is not Borel measurable. (Since the Lebesgue measure is complete, this is of course Lebesgue measurable.)
First, we have to know that every set of positive measure contains a nonmeasurable subset. Let be the Cantor function, a continuous function which is locally constant on and monotonically increasing on with and Obviously, is countable, since it contains one point per component of Hence has measure zero, so has measure one. We need a strictly monotonic function, so consider Since is strictly monotonic and continuous, it is a homeomorphism. Furthermore, has measure one. Let be non-measurable, and let Because is injective, we have that and so is a null set. However, if it were Borel measurable, then would also be Borel measurable (here we use the fact that the preimage of a Borel set by a continuous function is measurable; is the preimage of through the continuous function ). Therefore is a null, but non-Borel measurable set.
In a separable Banach space addition moves any subset to the translates for any When there is a probability measure μ on the σ-algebra of Borel subsets of such that for all then is a Haar null set. [3]
The term refers to the null invariance of the measures of translates, associating it with the complete invariance found with Haar measure.
Some algebraic properties of topological groups have been related to the size of subsets and Haar null sets. [4] Haar null sets have been used in Polish groups to show that when A is not a meagre set then contains an open neighborhood of the identity element. [5] This property is named for Hugo Steinhaus since it is the conclusion of the Steinhaus theorem.
In mathematics, specifically in measure theory, a Borel measure on a topological space is a measure that is defined on all open sets. Some authors require additional restrictions on the measure, as described below.
In measure theory, a branch of mathematics, the Lebesgue measure, named after French mathematician Henri Lebesgue, is the standard way of assigning a measure to subsets of higher dimensional Euclidean n-spaces. For lower dimensions n = 1, 2, or 3, it coincides with the standard measure of length, area, or volume. In general, it is also called n-dimensional volume, n-volume, hypervolume, or simply volume. It is used throughout real analysis, in particular to define Lebesgue integration. Sets that can be assigned a Lebesgue measure are called Lebesgue-measurable; the measure of the Lebesgue-measurable set A is here denoted by λ(A).
In mathematics, the concept of a measure is a generalization and formalization of geometrical measures and other common notions, such as magnitude, mass, and probability of events. These seemingly distinct concepts have many similarities and can often be treated together in a single mathematical context. Measures are foundational in probability theory, integration theory, and can be generalized to assume negative values, as with electrical charge. Far-reaching generalizations of measure are widely used in quantum physics and physics in general.
In mathematical analysis and in probability theory, a σ-algebra on a set X is a nonempty collection Σ of subsets of X closed under complement, countable unions, and countable intersections. The ordered pair is called a measurable space.
In mathematical analysis, the Haar measure assigns an "invariant volume" to subsets of locally compact topological groups, consequently defining an integral for functions on those groups.
In mathematics, a complete measure (or, more precisely, a complete measure space) is a measure space in which every subset of every null set is measurable (having measure zero). More formally, a measure space (X, Σ, μ) is complete if and only if
In the mathematical field of real analysis, the monotone convergence theorem is any of a number of related theorems proving the good convergence behaviour of monotonic sequences, i.e. sequences that are non-increasing, or non-decreasing. In its simplest form, it says that a non-decreasing bounded-above sequence of real numbers converges to its smallest upper bound, its supremum. Likewise, a non-increasing bounded-below sequence converges to its largest lower bound, its infimum. In particular, infinite sums of non-negative numbers converge to the supremum of the partial sums if and only if the partial sums are bounded.
In calculus and real analysis, absolute continuity is a smoothness property of functions that is stronger than continuity and uniform continuity. The notion of absolute continuity allows one to obtain generalizations of the relationship between the two central operations of calculus—differentiation and integration. This relationship is commonly characterized in the framework of Riemann integration, but with absolute continuity it may be formulated in terms of Lebesgue integration. For real-valued functions on the real line, two interrelated notions appear: absolute continuity of functions and absolute continuity of measures. These two notions are generalized in different directions. The usual derivative of a function is related to the Radon–Nikodym derivative, or density, of a measure. We have the following chains of inclusions for functions over a compact subset of the real line:
In mathematics, the ba space of an algebra of sets is the Banach space consisting of all bounded and finitely additive signed measures on . The norm is defined as the variation, that is
In mathematics, more precisely in measure theory, an atom is a measurable set that has positive measure and contains no set of smaller positive measures. A measure that has no atoms is called non-atomic or atomless.
In mathematics, a regular measure on a topological space is a measure for which every measurable set can be approximated from above by open measurable sets and from below by compact measurable sets.
In mathematics, a positive or a signed measure μ on a set X is called σ-finite if X equals the union of a sequence of measurable sets A1, A2, A3, … of finite measure μ(An) < ∞. Similarly, a subset of X is called σ-finite if it equals such a countable union. A measure being σ-finite is a weaker condition than being finite (i.e., weaker than μ(X) < ∞).
In mathematics, the support of a measure on a measurable topological space is a precise notion of where in the space the measure "lives". It is defined to be the largest (closed) subset of for which every open neighbourhood of every point of the set has positive measure.
In mathematics, strict positivity is a concept in measure theory. Intuitively, a strictly positive measure is one that is "nowhere zero", or that is zero "only on points".
In mathematics, an infinite-dimensional Lebesgue measure is a measure defined on infinite-dimensional normed vector spaces, such as Banach spaces, which resembles the Lebesgue measure used in finite-dimensional spaces.
In mathematics, more precisely in measure theory, a measure on the real line is called a discrete measure if it is concentrated on an at most countable set. The support need not be a discrete set. Geometrically, a discrete measure is a collection of point masses.
In probability theory, a standard probability space, also called Lebesgue–Rokhlin probability space or just Lebesgue space is a probability space satisfying certain assumptions introduced by Vladimir Rokhlin in 1940. Informally, it is a probability space consisting of an interval and/or a finite or countable number of atoms.
In mathematics, especially measure theory, a set function is a function whose domain is a family of subsets of some given set and that (usually) takes its values in the extended real number line which consists of the real numbers and
In mathematics, lifting theory was first introduced by John von Neumann in a pioneering paper from 1931, in which he answered a question raised by Alfréd Haar. The theory was further developed by Dorothy Maharam (1958) and by Alexandra Ionescu Tulcea and Cassius Ionescu Tulcea (1961). Lifting theory was motivated to a large extent by its striking applications. Its development up to 1969 was described in a monograph of the Ionescu Tulceas. Lifting theory continued to develop since then, yielding new results and applications.
This is a glossary of concepts and results in real analysis and complex analysis in mathematics.