Null set

Every finite or countably infinite subset of the real numbers is a null set. For example, the set of natural numbers and the set of rational numbers are both 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.

Suppose ${\displaystyle A}$ is a subset of the real line ${\displaystyle \mathbb {R} }$ such that for every ${\displaystyle \varepsilon >0,}$ there exists a sequence ${\displaystyle U_{1},U_{2},\ldots }$ of open intervals (where interval ${\displaystyle U_{n}=(a_{n},b_{n})\subseteq \mathbb {R} }$ has length ${\displaystyle \operatorname {length} (U_{n})=b_{n}-a_{n}}$) such that

$${\displaystyle A\subseteq \bigcup _{n=1}^{\infty }U_{n}\ ~{\textrm {and}}~\ \sum _{n=1}^{\infty }\operatorname {length} (U_{n})<\varepsilon \,,}$$

then ${\displaystyle A}$ 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 ${\displaystyle A}$ for which the limit of the lengths of the covers is zero.

The empty set is always a null set. More generally, any countable union of null sets is null. Any subset of a null set is itself a null set. Together, these facts show that the ${\displaystyle m}$-null sets of ${\displaystyle X}$ form a sigma-ideal on ${\displaystyle X.}$ Similarly, the measurable ${\displaystyle m}$-null sets form a sigma-ideal of the sigma-algebra of measurable sets. Thus, null sets may be interpreted as negligible sets, defining a 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 ${\displaystyle N}$ of ${\displaystyle \mathbb {R} }$ has null Lebesgue measure and is considered to be a null set in ${\displaystyle \mathbb {R} }$ if and only if:

Given any positive number ${\displaystyle \varepsilon ,}$ there is a sequence ${\displaystyle I_{1},I_{2},\ldots }$ of intervals in ${\displaystyle \mathbb {R} }$ such that ${\displaystyle N}$ is contained in the union of the ${\displaystyle I_{1},I_{2},\ldots }$ and the total length of the union is less than ${\displaystyle \varepsilon .}$

This condition can be generalised to ${\displaystyle \mathbb {R} ^{n},}$ using ${\displaystyle n}$-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:

• With respect to ${\displaystyle \mathbb {R} ^{n},}$ all singleton sets are null, and therefore all countable sets are null. In particular, the set ${\displaystyle \mathbb {Q} }$ of rational numbers is a null set, despite being dense in ${\displaystyle \mathbb {R} .}$
• The standard construction of the Cantor set is an example of a null uncountable set in ${\displaystyle \mathbb {R}$ ;} however other constructions are possible which assign the Cantor set any measure whatsoever.
• All the subsets of ${\displaystyle \mathbb {R} ^{n}}$ whose dimension is smaller than ${\displaystyle n}$ have null Lebesgue measure in ${\displaystyle \mathbb {R} ^{n}.}$ For instance straight lines or circles are null sets in ${\displaystyle \mathbb {R} ^{2}.}$
• Sard's lemma: the set of critical values of a smooth function has measure zero.

If ${\displaystyle \lambda }$ is Lebesgue measure for ${\displaystyle \mathbb {R} }$ and π is Lebesgue measure for ${\displaystyle \mathbb {R} ^{2}}$, then the product measure ${\displaystyle \lambda \times \lambda =\pi .}$ In terms of null sets, the following equivalence has been styled a Fubini's theorem:[2]

• For ${\displaystyle A\subset \mathbb {R} ^{2}}$ and ${\displaystyle A_{x}=\{y:(x,y)\in A\},}$
  $${\displaystyle \pi (A)=0\iff \lambda \left(\left\{x:\lambda \left(A_{x}\right)>0\right\}\right)=0.}$$

  

Null sets play a key role in the definition of the Lebesgue integral: if functions ${\displaystyle f}$ and ${\displaystyle g}$ are equal except on a null set, then ${\displaystyle f}$ is integrable if and only if ${\displaystyle g}$ is, and their integrals are equal. This motivates the formal definition of ${\displaystyle L^{p}}$ 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.

In a separable Banach space ${\displaystyle (X,+),}$ the group operation moves any subset ${\displaystyle A\subseteq X}$ to the translates ${\displaystyle A+x}$ for any ${\displaystyle x\in X.}$ When there is a probability measure μ on the σ-algebra of Borel subsets of ${\displaystyle X,}$ such that for all ${\displaystyle x,}$ ${\displaystyle \mu (A+x)=0,}$ then ${\displaystyle A}$ 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 ${\displaystyle A^{-1}A}$ 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.

• Cantor function – Continuous function that is not absolutely continuous
• Empty set – Mathematical set containing no elements
• Measure (mathematics) – Generalization of mass, length, area and volume
• Nothing – Complete absence of anything; the opposite of everything

• Capinski, Marek; Kopp, Ekkehard (2005). Measure, Integral and Probability. Springer. p. 16. ISBN 978-1-85233-781-0.
• Jones, Frank (1993). Lebesgue Integration on Euclidean Spaces. Jones & Bartlett. p. 107. ISBN 978-0-86720-203-8.
• Oxtoby, John C. (1971). Measure and Category. Springer-Verlag. p. 3. ISBN 978-0-387-05349-3.