On Stein's method for multivariate normal approximation
Elizabeth S. Meckes
Introduction
for all for which the left-hand side exists and is finite. The operator defined on functions by
is called the characterizing operator of the standard normal distribution. The left-inverse to , denoted , is defined by the equation
where is a standard normal random variable; the boundedness properties of are an essential ingredient of Stein’s method.
with the random quantities being small compared to , then is indeed approximately Gaussian, and its distance to Gaussian (in some metric) can be bounded in terms of the and .
The addition of a random error to this equation was not needed in the applications in , but is a straightforward modification of the theorems proved there.
After the initial draft of appeared on the ArXiv, a preprint was posted by Reinert and Röllin which generalized one of the abstract normal approximation theorems of . Instead of condition (4) above, they required
where is a positive definite matrix and is a random error. This more general condition allowed them to estimate the distance to Gaussian random vectors with non-identity (even singular) covariance matrices. They then introduced an insightful new method, “the embedding method” for approximating real random variables by the normal distribution, by observing that in many cases in which the condition (1) does not hold, the random variable in question can be viewed as one component of a random vector which satisfies condition (5) with a non-diagonal . Many examples are given, both of the embedding method and the multivariate normal approximation theorem directly, including applications to runs on the line, statistics of Bernoulli random graphs, U-statistics, and doubly-indexed permutation statistics.
The approach taken in the published version of is to give smoothness conditions instead by requiring bounds on the quantities
The Wasserstein distance between the random variables and is defined by
where is the Lipschitz constant of . On the space of probability distributions with finite absolute first moment, Wasserstein distance induces a stronger topology than the usual one described by weak convergence, but not as strong as the topology induced by the total variation distance. See for detailed discussion of the various notions of distance between probability distributions.
The identity matrix is denoted and the matrix of all zeros is denoted .
that is, is the Lipschitz constant of the -st derivative of .
This general definition of is a departure from what was done by Raič in ; there, smoothness conditions on functions are also given in coordinate-independent ways, and and are defined as they are here, but in case , the quantity is defined as the Lipschitz constant of the Hessian with respect to the Hilbert-Schmidt norm as opposed to the operator norm.
Abstract Approximation Theorems
This section contains the basic lemmas giving the Stein characterization of the multivariate Gaussian distribution and bounds to the solution of the Stein equation, together with two multivariate abstract normal approximation theorems and their proofs. The first theorem is a reworking of the theorem of Reinert and Röllin on multivariate normal approximation with the method of exchangeable pairs for vectors with non-identity covariance. The second is an analogous result in the context of “continuous symmetries” of the underlying random variable, as has been previously studied by the author in , , and (jointly with S. Chatterjee) in .
is a solution to the differential equation
Part (1) follows from integration by parts.
and so since is dense in the class of bounded continuous functions, with respect to the supremum norm.
For part (3), first note that since is Lipschitz, if
which is integrable on , so the integral exists by the dominated convergence theorem.
To show that is indeed a solution to the differential equation (9), let
The next lemma gives useful bounds on and its derivatives in terms of and its derivatives. As in , bounds are most naturally given in terms of the quantities defined in the introduction.
If, in addition, is positive definite, then
Remark: Bounds (3), (4), and (5) are mainly of use when has a fairly simple form, since they require an estimate for . They are also of theoretical interest, since they show that if is non-singular, then the operator is smoothing; functions are typically one order smoother than . The bounds (1) and (2), while not showing the smoothing behavior of , are useful when is complicated (or singular) and an estimate of is infeasible or impossible.
Write and . Note that by the formula for ,
for unit vectors , and part (1) follows immediately.
For the second part, note that (10) implies that
For part (3), note that it follows by integration by parts on the Gaussian expectation that
For part (4), again using integration by parts on the Gaussian expectation,
For notational convenience, let . By the exchangeability of ,
where is the error in the Taylor approximation. By conditions (1) and (2), it follows that
that is (making use of the definition of ),
where the first line is by the Cauchy-Schwarz inequality, the second is by the standard bound and the third uses the bounds (2) and (4) from Lemma 2.
Finally, by Taylor’s theorem and Lemma 2,
The first bound of the theorem results from choosing the first term from each minimum; the second bound results from the second terms.
For notational convenience, let . Beginning as before,
where is the error in the Taylor approximation.
Now, by Taylor’s theorem, there exists a real number depending on , such that
Breaking up the expectation over the sets on which is larger and smaller than a fixed ,
The second term tends to zero as by condition 3; condition 2 implies that the first is bounded by for a constant depending on the distribution of . It follows that
is stronger than condition (3) of Theorem 4 and may be used instead; this is what is done in the application given in Section 3.
In , singular covariance matrices are treated by comparing to a nearby non-singular covariance matrix rather than directly. However, this is not necessary as all the proofs except those explicitly involving go through for non-negative definite .
Examples
The following example was treated by Reinert and Röllin as an example of the embedding method. It should be emphasized that showing that the number of -runs on the line is asymptotically Gaussian seems infeasible with Stein’s original method of exchangeable pairs because of the failure of condition (1) from the introduction, but in , the random variable of interest is embedded in a random vector whose components can be shown to be jointly Gaussian by making use of the more general condition (5) of the introduction. The example is reworked here making use of the analysis of together with Theorem 3, yielding an improved rate of convergence.
assuming the torus convention, namely that for any . For this example, we assume that . To make an exchangeable pair, sequential elements of are resampled. That is, let be a uniformly distributed element of and let be independent copies of the . Let be constructed from by replacing with . Then is an exhangeable pair, and, defining for , it is easy to see that
where sums are taken to be zero if . It follows that
Standard calculations show that, for
It then follows from (21) that, for ,
Condition (1) of Theorem 3 thus applies with and as above.
To apply Theorem 3, an estimate on is needed. Following Reinert and Röllin, we make use of known estimates of condition numbers for triangular matrices (see, e.g., the survey of Higham ). First, write , where is diagonal with the same diagonal entries as and is lower triangular with diagonal entries equal to one and for . Note that all non-diagonal entries of are bounded in absolute value by . From Lemeire , this implies the bounds
From Higham, thus
Trivially, , and thus
It was determined by Reinert and Röllin that
Using these bounds in inequality (13) from Theorem 3 yields the following.
where is a standard -dimensional Gaussian random vector.
Remarks: Compare this result to that obtained in :
where and .
2. Eigenfunctions of the Laplacian
Consider a compact Riemannian manifold with metric . Integration with respect to the normalized volume measure is denoted , thus For coordinates on , define
where the coefficient implicit in the depends on and and denotes the differential of at . Recall that for and the gradient defined as above. Now, for fixed, is distributed according to normalized Lebesgue measure on and is a linear functional on . It follows that
exists and is finite; we will take Indeed, it is well-known (see, e.g., Theorem 11.12 of ) that
For the second condition of Theorem 4, it is necessary to determine
Choose coordinates in a neighborhood of which are orthonormal at . Then
(As before, the convergence requirement is satisfied since the are smooth and is compact.)
(where the implicit constants depend on the and on ), thus condition (3) of Theorem 4 is satisfied.
All together, we have proved the following.
Let be a compact Riemannian manifold and an orthonormal (in ) sequence of eigenfunctions of the Laplacian on , with corresponding eigenvalues . Let be a uniformly distributed random point of . Then if ,
In this example, Theorem 6 is applied to the value distributions of eigenfunctions on flat tori. The class of functions considered here are random functions; that is, they are linear combinations of eigenfunctions with random coefficients.
Eigenfunctions of are given by the real and imaginary parts of functions of the form
Consider a collection of random eigenfunctions of on the torus which are linear combinations of eigenfunctions with random coefficients:
and, applying Theorem 6, we have shown that
Remarks: Note that if the elements of are mutually orthogonal, then the right-hand side becomes
Acknowledgements. The author thanks M. Meckes for many useful discussions. This research was supported by an American Institute of Mathematics five-year fellowship.