Universe (mathematics)


Universe (mathematics)

: "In mathematical logic, the universe of a structure (or "model") is its domain.

In mathematics, and particularly in applications to set theory and the foundations of mathematics, a universe or universal class (or if a set, universal set – not to be confused with the universal set of some set theories that contains itself) is a class that contains (as elements or subsets) all of the elements and sets that one may wish to use in a given situation. There are several versions of this general idea, described in the following sections.

In a specific context

Perhaps the simplest version is that "any" set can be a universe, so long as the object of study is confined to that particular set.If the object of study is formed by the real numbers, then the real line R, which is the real number set, could be the universe under consideration.Implicitly, this is the universe that Georg Cantor was using when he first developed modern naive set theory and cardinality in the 1870s and 1880s in applications to real analysis.The only sets that Cantor was originally interested in were subsets of R.

This concept of a universe is reflected in the use of Venn diagrams.In a Venn diagram, the action traditionally takes place inside a large rectangle that represents the universe "U".One generally says that sets are represented by circles; but these sets can only be subsets of "U".The complement of a set "A" is then given by that portion of the rectangle outside of "A"'s circle.Strictly speaking, this is the relative complement "U" "A" of "A" relative to "U"; but in a context where "U" is the universe, it can be regarded as the absolute complement "A"C of "A".Similarly, there is a notion of the nullary intersection, that is the intersection of zero sets (meaning no sets, not null sets).Without a universe, the nullary intersection would be the set of absolutely everything, which is generally regarded as impossible; but with the universe in mind, the nullary intersection can be treated as the set of everything under consideration, which is simply "U".

These conventions are quite useful in the algebraic approach to basic set theory, based on Boolean lattices.Except in some non-standard forms of axiomatic set theory (such as New Foundations), the class of all sets is not a Boolean lattice (it is only a relatively complemented lattice).In contrast, the class of all subsets of "U", called the power set of "U", is a Boolean lattice.The absolute complement described above is the complement operation in the Boolean lattice; and "U", as the nullary intersection, serves as the top element (or nullary meet) in the Boolean lattice.Then De Morgan's laws, which deal with complements of meets and joins (which are unions in set theory) apply, and apply even to the nullary meet and the nullary join (which is the empty set).

In ordinary mathematics

However, once subsets of a given set "X" (in Cantor's case, "X" = R) are considered, the universe may need to be a set of subsets of "X".(For example, a topology on "X" is a set of subsets of "X".)The various sets of subsets of "X" will not themselves be subsets of "X" but will instead be subsets of P"X", the power set of "X".This may be continued; the object of study may next consist of such sets of subsets of "X", and so on, in which case the universe will be P(P"X").In another direction, the binary relations on "X" (subsets of the Cartesian product nowrap|"X" × "X") may be considered, or functions from "X" to itself, requiring universes like nowrap|P("X" × "X") or "X""X".

Thus, even if the primary interest is "X", the universe may need to be considerably larger than "X".Following the above ideas, one may want the superstructure over "X" as the universe.This can be defined by structural recursion as follows:
* Let S0"X" be "X" itself.
* Let S1"X" be the union of "X" and P"X".
* Let S2"X" be the union of S1"X" and P(S1"X").
* In general, let S"n"+1"X" be the union of Sn"X" and P(S"n""X").Then the superstructure over "X", written S"X", is the union of S0"X", S1"X", S2"X", and so on; or: mathbf{S}X := igcup_{i=0}^{infty} mathbf{S}_{i}X mbox{.} !

Note that no matter what set "X" is the starting point, the empty set {} will belong to S1"X".The empty set is the von Neumann ordinal [0] .Then { [0] }, the set whose only element is the empty set, will belong to S2"X"; this is the von Neumann ordinal [1] .Similarly, { [1] } will belong to S3"X", and thus so will { [0] , [1] }, as the union of { [0] } and { [1] }; this is the von Neumann ordinal [2] .Continuing this process, every natural number is represented in the superstructure by its von Neumann ordinal.Next, if "x" and "y" belong to the superstructure, then so does "x"},{"x","y", which represents the ordered pair ("x","y").Thus the superstructure will contain the various desired Cartesian products.Then the superstructure also contains functions and relations, since these may be represented as subsets of Cartesian products.The process also gives ordered "n"-tuples, represented as functions whose domain is the von Neumann ordinal ["n"] .And so on.

So if the starting point is just "X" = {}, a great deal of the sets needed for mathematics appear as elements of the superstructure over {}.But each of the elements of S{} will be finite sets!Each of the natural numbers belongs to it, but the set N of "all" natural numbers does not (although it is a "subset" of S{}).In fact, the superstructure over "X" consists of all of the hereditarily finite sets.As such, it can be considered the "universe of finitist mathematics".Speaking anachronistically, one could suggest that the 19th-century finitist Leopold Kronecker was working in this universe; he believed that each natural number existed but that the set N (a "completed infinity") did not.

However, S{} is unsatisfactory for ordinary mathematicians (who are not finitists), because even though N may be available as a subset of S{}, still the power set of N is not.In particular, arbitrary sets of real numbers are not available.So it may be necessary to start the process all over again and form S(S{}).However, to keep things simple, one can take the set N of natural numbers as given and form SN, the superstructure over N.This is often considered the "universe of ordinary mathematics".The idea is that all of the mathematics that is ordinarily studied refers to elements of this universe.For example, any of the usual constructions of the real numbers (say by Dedekind cuts) belongs to SN.Even non-standard analysis can be done in the superstructure over a non-standard model of the natural numbers.

One should note a slight shift in philosophy from the previous section, where the universe was any set "U" of interest.There, the sets being studied were "subset"s of the universe; now, they are "members" of the universe.Thus although P(S"X") is a Boolean lattice, what is relevant is that S"X" itself is not.Consequently, it is rare to apply the notions of Boolean lattices and Venn diagrams directly to the superstructure universe as they were to the power-set universes of the previous section.Instead, one can work with the individual Boolean lattices P"A", where "A" is any relevant set belonging to S"X"; then P"A" is a subset of S"X" (and in fact belongs to S"X"). In Cantor's case "X" = R in particular, arbitrary sets of real numbers are not available, so there it may indeed be necessary to start the process all over again.

In set theory

It is possible to give a precise meaning to the claim that SN is the universe of ordinary mathematics; it is a model of Zermelo set theory, the axiomatic set theory originally developed by Ernst Zermelo in 1908.Zermelo set theory was successful precisely because it was capable of axiomatising "ordinary" mathematics, fulfilling the programme begun by Cantor over 30 years earlier.But Zermelo set theory proved insufficient for the further development of axiomatic set theory and other work in the foundations of mathematics, especially model theory.For a dramatic example, the description of the superstructure process above cannot itself be carried out in Zermelo set theory!The final step, forming S as an infinitary union, requires the axiom of replacement, which was added to Zermelo set theory in 1922 to form Zermelo-Fraenkel set theory, the set of axioms most widely accepted today.So while ordinary mathematics may be done "in" SN, discussion "of" SN goes beyond the "ordinary", into metamathematics.

But if high-powered set theory is brought in, the superstructure process above reveals itself to be merely the beginning of a transfinite recursion.Going back to "X" = {}, the empty set, and introducing the (standard) notation "V""i" for S"i"{}, "V"0 = {}, "V"1 = P{}, and so on as before.But what used to be called "superstructure" is now just the next item on the list: "V"ω, where ω is the first infinite ordinal number.This can be extended to arbitrary ordinal numbers:: V_{i} := igcup_{jdefines "V""i" for "any" ordinal number "i".The union of all of the "V""i" is the von Neumann universe "V":: V := igcup_{i} V_{i} ! .Note that every individual "V""i" is a set, but their union "V" is a proper class.The axiom of foundation, which was added to ZF set theory at around the same time as the axiom of replacement, says that "every" set belongs to "V".

: "Kurt Gödel's constructible universe "L" and the axiom of constructibility": "Inaccessible cardinals yield models of ZF and sometimes additional axioms, and are equivalent to the existence of the Grothendieck universe set"

In category theory

There is another approach to universes which is historically connected with category theory. This is the idea of a Grothendieck universe. Conceptually, a Grothendieck universe is a set inside which all the usual operations of set theory can be performed. For example, the union of any two sets in a Grothendieck universe "U" is still in "U". Similarly, intersections, unordered pairs, power sets, and so on are also in "U". This is similar to the idea of a superstructure above. The advantage of a Grothendieck universe is that it is actually a "set", and never a proper class; the disadvantage is that if one tries hard enough, one can leave a Grothendieck universe.

The most common use of a Grothendieck universe "U" is to take "U" as a replacement for the category of all sets. One says that a set "S" is "U"-small if "S" ∈"U", and "U"-large otherwise. The category "U"-Set of all "U"-small sets has as objects all "U"-small sets and as morphisms all functions between these sets. Both the object set and the morphism set are sets, so it becomes possible to discuss the category of "all" sets without invoking proper classes. Then it becomes possible to define other categories in terms of this new category. For example, the category of all "U"-small categories is the category of all categories whose object set and whose morphism set are in "U". Then the usual arguments of set theory are applicable to the category of all categories, and one does not have to worry about accidentally talking about proper classes. Because Grothendieck universes are extremely large, this suffices in almost all applications.

Often when working with Grothendieck universes, there is an axiom hiding in the background: "For all sets "x", there exists a universe "U" such that "x" ∈"U"." The point of this axiom is that any set one encounters is then "U"-small for some "U", so any argument done in a general Grothendieck universe can be applied. This axiom is closely related to the existence of strongly inaccessible cardinals.

: "Set-like toposes"

See also

* Herbrand universe
* Free object


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