1. Introduction
The classical procedure in multivariate stochastic models assumes the existence of a suitable (joint) probability distribution, expressed in terms of the univariate marginals and the copula, that provides an accurate description of the phenomenon under consideration, and all subsequent computations (i.e., risk calculations) are based on this model. However, in most practical cases, the joint distribution is only partially known, and this model uncertainty should be taken into consideration. In particular, various investigations have considered that we only know the marginal distributions, but do not know the dependence structure, i.e., we do not know the copula.
These latter studies typically provide dependence uncertainty bounds for the copula and/or for related functionals of the multivariate distributions. Their origin has a long history going back to earlier works by Hoeffding and Fréchet (see, for instance, [
1] and the references therein), but they have been extended to many kinds of functionals of the joint distribution, especially related to quantile estimation and risk calculation in finance and insurance (see, e.g., [
2,
3] and the references therein). As a matter of fact, these bounds are in general not copulas, but quasi-copulas. Such objects were introduced in [
4,
5] and characterized in analytical terms in [
6,
7] (for a complete overview, we refer to [
8,
9]). Noticeably, the suprema and infima of copulas are actually quasi-copulas, although not all quasi-copulas can be expressed in terms of lattice operations on copulas in dimensions greater than three (see [
10,
11]).
Quasi-copulas have recently appeared in the study of the model-free procedure for pricing financial instruments (see [
3,
12,
13,
14]). In fact, as underlined in [
3], since the bounds on the dependence structure of a given random vector
may not be copulas, then the results from stochastic order theory that translate the bounds on the copula of
into the bounds on the expectation of
do not apply directly, and some concepts need to be extended into the quasi-copula framework.
Motivated by the study of bounds for special classes of (quasi-)copulas, here, we focus our attention on copulas, supermodular quasi-copulas (see, for instance, [
15]), as well as their Dedekind–MacNeille completion. In fact, these sets may represent natural frameworks where lattice operations on copulas naturally lie. Our purpose is, hence, to study the relative size of these sets by using the concept of the Baire category as considered, for instance, in [
16,
17,
18,
19]. Specifically, we will determine the size of the Dedekind–MacNeille completion of the sets of copulas and supermodular quasi-copulas with respect to the topology induced by the distance (or metric)
, i.e., the uniform convergence in the set of quasi-copulas.
The paper is organized as follows. After recalling some preliminary definitions and notations (
Section 2), in
Section 3, we present some properties related to supermodular quasi-copulas and show that the set of supermodular quasi-copulas is compact under the metric
. In
Section 4, we show that the Dedekind–MacNeille completion of the set of copulas is small, in terms of the Baire category, in the Dedekind–MacNeille completion of the set of the supermodular quasi-copulas, and in turn, this set and the set of copulas are small in the set of quasi-copulas. Finally,
Section 5 concludes.
2. Preliminaries
First, we recall some basic aspects about copulas and quasi-copulas (see, e.g., [
20,
21]).
Let be a natural number. We recall that an n-dimensional quasi-copula (briefly, n-quasi-copula) is a function Q from to satisfying:
- (Q1)
Boundary conditions: For every , if at least one coordinate of is equal to zero; and whenever all coordinates of are equal to one, except maybe .
- (Q2)
Monotonicity: Q is nondecreasing in each variable.
- (Q3)
Lipschitz condition: For every , it holds that .
The set of n-quasi-copulas will be denoted by .
Quasi-copulas are generalizations of the concept of a copula, which is recalled here. An n-copula is a function C from to that satisfies the condition (Q1) for n-quasi-copulas and, in place of (Q2) and (Q3), the stronger condition:
- (Q4)
n-increasing property: for every n-box in , where the sum is taken over all the vertices of B (i.e., each is equal to either or ), and is the number of indices k’s such that .
The set of n-copulas will be denoted by .
Every n-copula is an n-quasi-copula, and a proper n-quasi-copula is an n-quasi-copula, which is not an n-copula—the set of proper n-quasi-copulas will be denoted by .
If we consider the standard partial order among real-valued functions in the space of quasi-copulas, then we can provide upper and lower bounds in
. In fact, every
n-quasi-copula
Q satisfies the following condition:
It is known that: (a)
is an
n-copula for every
, (b)
is a two-copula, and (c)
is a proper
n-quasi-copula for every
. For several interesting similarities and differences between copulas and proper quasi-copulas, see, for example, [
22,
23,
24,
25,
26,
27].
In the following, we will also consider some notions from lattice theory (see, e.g., [
28]), which are recalled here.
Given two elements x and y of a partially ordered set (i.e., poset) , let denote the join (or the least upper bound) of x and y (when it exists); similarly for , where S is a subset of P; denotes the meet (or the greatest lower bound) of x and y (when it exists); and similarly for . If the join or meet is found within a particular poset P, we subscript . Given two posets A and B, we say that A is join-dense (respectively, meet-dense) in B if, for every d in B, there exists a set such that (respectively, ). A poset is a lattice if for every in P, and are in P; and P is a complete lattice if, for every , and are in P.
If
is an order-embedding (i.e., order-preserving injection) of a poset
P into a complete lattice
L, then we say that
L is a completion of
P. Moreover, if
maps
P onto
L, then
is referred to as an order-isomorphism (i.e., order-preserving bijection). We also have the following definition (see [
28]).
Definition 1. A completion P of a lattice L is called a Dedekind–MacNeille completion of L if P is join-dense and meet-dense in L.
3. Quasi-Copulas and Related Subclasses
Now, we consider the class of quasi-copulas
equipped with the standard partial order among real-valued functions. For any pair
and
of quasi-copulas (or copulas),
and
. As is known (see [
10,
11]),
is a complete lattice; however,
(respectively,
) is not even a lattice. We denote by
the Dedekind–MacNeille completion of the set of
n-copulas in
.
It is known that:
the set of two-quasi-copulas
is order-isomorphic to the Dedekind–MacNeille completion of the set of two-copulas
(see [
11]);
for
,
is not order-isomorphic to
(see [
10]).
In the quest for a suitable subset of quasi-copulas that may be order-isomorphic to
, supermodular quasi-copulas were considered in [
15]. Here, we recall the definition of this concept (see, e.g., [
29]).
Definition 2. A function is called supermodular if, for all , it holds that
The following result is a useful characterization of supermodular functions (see [
30,
31]). We recall that for any
and any set of indices
with
, the
k-dimensional section of a function
with fixed values given by
at the positions not in
A is the function
defined by
, where
if
and
if
.
Proposition 1. A function is supermodular if, and only if, all of its two-dimensional sections are supermodular.
For
, supermodularity and two-increasingness are equivalent. However, this is no longer true for
(see [
22]). Furthermore, supermodularity together with the boundary conditions (Q1) implies increasingness and one-Lipschitz continuity, whence the following result is obtained (see [
22]).
Proposition 2. If is a supermodular function satisfying the condition (Q1) of an n-quasi-copula, then S is an n-quasi-copula.
Let
denote the set of supermodular
n-quasi-copulas. As can be easily seen, for
,
(see [
22]). Moreover,
. A relevant subset of
is formed by all Archimedean
n-quasi-copulas (see [
22]), as introduced in [
32]. In particular,
is supermodular. For other examples of supermodular
n-quasi-copulas, see [
33].
Now, we consider the lattice structure of
and its related Dedekind–MacNeille completion, denoted by
. The following result follows from [
15].
Proposition 3. For , the following results hold:
- (a)
is join-dense in ;
- (b)
is not meet-dense in , i.e., there exists an n-quasi-copula such that for any , .
Thus, is not a complete lattice.
As a consequence of Proposition 3, for , is not order-isomorphic to . Furthermore, in the following example, we show that neither nor hold.
Example 1. Let . We know that ; however, since there does not exist an n-copula C such that .
On the other hand, consider the following two n-copulas: for and for all , where and are the two-copulas given by and , respectively. Then, we have that is a proper n-quasi-copula such that (see [10]); furthermore, Q is not supermodular, since is a proper two-quasi-copula [11], i.e., it is not supermodular. We conclude this section with two additional properties about the structure of the set .
It is known that the sets
and
are compact under the metric
(see [
20,
34]). This is also the case for the set
, as the next result shows.
Proposition 4. The set is compact under the metric .
Proof. Let
be a sequence in
that converges pointwise to an
n-quasi-copula
. Since
for every
and for all
, taking the limits on both sides of the inequality, we have:
i.e.,
is closed in
. Since
is compact under the metric
, the set
is also compact, which completes the proof. □
For the next result, we need to recall the concept of an ordinal sum for quasi-copulas. Let
be a finite or countably infinite subset of
, and let
,
, be a collection of functions. The ordinal sum
F of
with respect to the family of pairwise disjoint intervals
is defined, for all
, by:
The sets
and
are closed under ordinal sums (see [
20,
35,
36]). In the next result, we study the ordinal sum of two supermodular
n-quasi-copulas in intervals of the form
and
, with
.
Proposition 5. The ordinal sum of two n-quasi-copulas of with respect to the intervals and , with , is in .
Proof. Let
Q be the ordinal sum of
with respect to the intervals
. Let
be a fixed point in
, with
, and define the function
on
. We check that
G is two-increasing (note that, as a consequence of Proposition 1, we would have
). Observe that, for all
such that
and
, we have:
Note also that the rectangle
can be decomposed into a union of rectangles, namely
, of disjoint interiors so that, if
(respectively,
), then
(respectively,
). We consider three cases:
. We consider two subcases:
- 1a.
. Then, we have
; thus:
with
, whence
.
- 1b.
. In this case, we have
; thus:
with
, whence
.
. We need to consider two subcases:
- 2a.
. Then, we have:
with
. Therefore,
, where:
- 2b.
. We separately study the values:
where
. Unless
for all
j, all the cases correspond to Case 2a; thus, their
Q-volumes are non-negative, and:
. We have two subcases.
- 3a.
. Then, we have:
with
. Therefore,
.
- 3b.
. This case is similar to Case 2b.
Therefore, we have that G is two-increasing, and the result follows. □
Notice that the previous result can be extended to the ordinal sum of a finite (or countable) set of copulas by using a similar procedure as in [
36]. Specifically, the ordinal sum of
k copulas, namely
, can be interpreted as the ordinal sum of two copulas,
and
, where
is an ordinal sum of the copulas
(with respect to suitable intervals).
4. Baire Category Results for Subclasses of Quasi-Copulas
In this section, we check that the “size” of the set
is “small”—in terms of the Baire category—in
and, in turn,
is “small” in
. We recall that a subset of a (complete) metric space is called nowhere dense if it is not dense in any open ball
of centre
and radius
(equivalently, if its closure has an empty interior). Thus, for example, the set
is nowhere dense in the class
(see [
18]). Using the same techniques as those used in [
18], it can be proven that, for
,
is nowhere dense
.
To study the Baire category results for the set in , we need some preliminary results.
Lemma 1. Let . Then, if, and only if, for every , there exist and in such that and for all .
Proof. Suppose in . Then, there exists a set such that, for all , . Fixing , there exists a sequence in such that for all and for every , and converges to as k goes to ∞.
Since is compact with the topology induced by the metric (recall Proposition 4), there exists a subsequence of convergent to . The n-quasi-copula satisfies that and for all . Analogously, we can obtain that and for all .
Conversely, note that , so that Q belongs to , and this completes the proof. □
Proposition 6. The set is compact in with respect to the metric .
Proof. Let Q be an n-quasi-copula in the closure of . Then, there exists a sequence in such that for every . Let be fixed. From Lemma 1, for every , there exists an n-quasi-copula such that and for all . Then, there exists a subsequence that converges to such that and for all . Therefore, we have , and since , then for all . Since is closed, then is supermodular. From Lemma 1, we conclude that . □
In what follows, we will need additional notation. For any , let denote the ordinal sum of Q and the n-quasi-copula given in Proposition 3, with intervals and , where , .
Lemma 2. For any , we have . Moreover, converges pointwise to Q as k goes to ∞.
Proof. Suppose
. Then, from Lemma 1, for every
, there exists
such that
and
for all
. This implies:
i.e.,
is an ordinal sum. Thus, the bijection from
on
defined by:
provides a family
of supermodular
n-quasi-copulas such that, for a fixed
, we have
and
for all
. Therefore, we obtain a contradiction and, hence,
.
On the other hand, from the definition of
, we have:
This guarantees that
converges pointwise to
Q as
k goes to
∞. □
We are now in a position to provide the main result about the “size” of the set in .
Theorem 1. The set is nowhere dense in .
Proof. Suppose the set is not nowhere dense in . Since, from Proposition 6, is closed in , it must contain an open ball B, and the n-quasi-copula Q is in its interior. For a sufficiently large k, we have that . However, this is a contradiction since, from Lemma 2, we have . Therefore, is nowhere dense in . □
Since , it follows that is nowhere dense in .
In the sequel, we show that is nowhere dense in . In order to prove it, we need some preliminary results.
Lemma 3. Let . Then, if, and only if, for every , there exist and in such that and for all .
The proof of Lemma 3 is similar to the proof of Lemma 1, and we omit it.
As a consequence of Lemma 3, we have the following result, whose proof is similar to the proof of Proposition 6, and we omit it.
Proposition 7. The set is closed in with respect to the metric , and hence, it is also compact.
For any , let denote the ordinal sum of Q and with respect to the intervals and , where , .
Lemma 4. For any , we have . Moreover, converges pointwise to Q as k goes to ∞.
Proof. Suppose
. Then, from Lemma 3, there exists
such that:
and
for all
, i.e.,
is an ordinal sum. Thus, there exists
n-copulas
such that
can be represented as the ordinal sum of
with respect to the intervals
and
. Since
, it follows that
, which is absurd for
. Therefore,
.
In order to prove the convergence of , we just have to follow the same steps as the ones given in the proof of Lemma 2, which completes the proof. □
We are now in a position to check the “size” of the set in . As a consequence of Proposition 7 and Lemma 4, we have the following result, whose proof is similar to the proof of Theorem 1, and we omit it.
Theorem 2. The set is nowhere dense in .
From the results presented here and mimicking the same arguments used in their proofs, it is possible to show the following two results, whose proofs are omitted.
Theorem 3. The set is nowhere dense in .
For the next result, we recall that a function
is called
k-dimensionally-increasing, with
, if any of its
k-dimensional sections is
k-increasing. Let
denote the class of all
k-dimensionally-increasing
n-quasi-copulas. In [
22], it was shown that
. Then, we have:
Theorem 4. For every , the set is nowhere dense in .