Hellinger affinity 2026-10-06
The Hellinger affinity of dominated probability measures is the integral of the geometric mean of their probability density functions. It lies in by Cauchy-Schwarz inequality. The unnormalized squared Hellinger distance is times this affinity; this identity makes the relation with relative entropy particularly simple.
If is a measurable function into a separable Banach space and has finite second moments under probability measures , then their Bochner integral expected values satisfy
Here the Hellinger distance includes the factor in its square. For a proof, use , , and . Apply the norm bound for a Bochner integral and the Cauchy-Schwarz inequality to , then use . This explains why stability of a Bayesian posterior in Hellinger distance controls posterior expected values when the relevant second moments remain bounded.
With the convention , the Hellinger distance between two normal distributions with is
To prove it, integrate the geometric mean of their probability density functions. Completing the square makes that geometric mean the density of a normal distribution times the displayed prefactor and exponential. For example, writing , that normal distribution has mean and variance . The identity then proves the formula.
For equal unit variances, this becomes . More generally, put and . Then , , and , proving
Put and . Using natural logarithms, the Kullback-Leibler divergence is
The integrand is zero where , including where both densities vanish, and is where . Equivalently, when is absolutely continuous with respect to , and it is otherwise. This is a well-defined extended integral: on , writing gives , so its negative part is integrable.
For Pinsker's inequality, an infinite Kullback-Leibler divergence makes the conclusion immediate. Assume it is finite. Set
Since , the positive and negative parts of have equal integrals. Thus
This is the total variation distance with the convention .
We first prove the binary partition bound for relative entropy. For any measurable with , apply Jensen inequality to the convex function under the conditional probability measure . Absolute continuity of measures gives
If , both sides are zero; if , finiteness forces as well. Apply this bound to and its complement to obtain
For , regarding as a function of gives
Consequently is a convex function and has its minimum zero at . By continuity this also holds at . For , the finite case has and the remaining cases have infinite divergence. This proves the Bernoulli relative entropy lower bound in every case. Combining the bounds yields
For the Hellinger distance, retain the unnormalized convention in which
The integral is the Hellinger affinity. In the finite-divergence case, for -almost every point. Apply with to get
The affinity is finite by Cauchy-Schwarz inequality. Mass of on creates no difficulty, since the affinity vanishes there and both probability measures have mass one. The infinite-divergence case is again immediate. We obtain the relative entropy bound for the unnormalized Hellinger distance:
Let and be Radon-Nikodym derivatives. Use the following normalizations of the Kullback-Leibler divergence, total variation distance and unnormalized Hellinger distance:
We use and assign infinite Kullback-Leibler divergence if , where denotes absolute continuity of measures. Common domination alone also suffices for the inequalities with the extended-value convention. The negative part of the logarithmic integral is integrable: on , . Thus the extended-value integral defining the Kullback-Leibler divergence is well-defined. These expressions do not depend on which common dominating measure is chosen. The Kullback-Leibler divergence is generally asymmetric and therefore fails a defining property of a metric.
For completeness, the integral formula for total variation distance follows by taking : since , the positive and negative parts of have the same integral, and this set attains the supremum.
Put , by the Cauchy-Schwarz inequality. A second application gives
The logarithmic inequality in the hint implies for . Apply it to on :
Multiplying by and integrating proves
If on a set of positive -measure, the right side is finite but the Kullback-Leibler divergence is infinite, so the inequality is immediate. Thus
This total variation–Hellinger–relative entropy inequality requires the stated Hellinger distance normalization for its first constant. With the alternative convention , the correct comparison is and . In particular, and have .
Here is a testing form of the Le Cam two-point lemma. Suppose two parameter values in a metric space have separation , and let be the corresponding observation laws. Every estimator satisfies
To prove it, classify by the closer of the two parameters, breaking a tie in favour of one. Let . On , the triangle inequality implies , while on it implies . Hence the sum of the two probabilities in the display is at least
At least one is at least half the sum, proving the claim. It also gives a lower bound for the maximum expected metric loss.
For absolute-error loss, or any loss given by a metric, there is a stronger expectation form. Take densities relative to and use the triangle inequality under their overlap:
Therefore the Le Cam lower bound under absolute-error loss is
Both arguments are valid for randomized estimators as well, by adjoining the independent randomization to the observation; doing so does not change total variation distance.
For the normal distribution model, assume the usual nondegenerate convention and use the full product observation laws. Choose
For one observation, its Gaussian log likelihood ratio is
Under the first law, and . Thus the Kullback-Leibler divergence between normal distributions is
For the independent and identically distributed random variables, the joint log likelihood ratio is the sum of the individual ones, so the Kullback-Leibler divergence of the two full statistical samples is . The comparison just proved implies . Applying the expectation form of the Le Cam two-point lemma gives
This is a Gaussian location minimax lower bound under absolute-error loss. The constant may depend on the fixed known , but neither on the estimator nor on . If a signed nonzero scale were used, the same result holds with in place of . If zero noise were allowed, would estimate exactly, so a positive lower bound would be false; positive variance is necessary.
Use the Hellinger distance convention in the original PDF:
The TeX transcription incorrectly places the integral outside the outer square root in the definition; the displayed formula for the squared distance and the original PDF both use the convention above. Although Lebesgue measure is not a probability measure, we may use it as the common dominating measure: the integral is unchanged by replacing it with any equivalent dominating probability measure.
For unit-variance normal distributions, put and . The product of the square roots of their probability density functions is
The final factor integrates to one, so
For the bound at arbitrary , use the given formula for the Hellinger distance between normal distributions and write
Since for ,
Therefore one valid choice is . In particular this bound is uniform when the two standard deviations stay bounded away from zero.
Choose the common dominating probability measure and let , be the Radon-Nikodym derivatives. The assumed second moments imply first-moment integrability by the Cauchy-Schwarz inequality. Since is a separable Banach space, the measurable is a strongly measurable function, and both expected values exist as Bochner integrals.
The difference of these Bochner integrals satisfies
The first inequality is the norm bound for a Bochner integral, and the second is the scalar Cauchy-Schwarz inequality. Since , the first factor is at most
With the Hellinger distance convention of the original PDF, the second factor is . Multiplication proves the Hellinger bound for differences of expectations:
The proof uses only the two laws and their common dominating measure; no absolute continuity of measures assumption between and is needed.
Write and , whose existence follows from the Radon-Nikodym theorem. Since
we have
Thus the defining integral is finite and the Hellinger distance is well defined.
With the same , the squared Hellinger distance is
Since ,
The Gaussian Poincaré inequality and the derivative calculation in part (b) yield
The scalar inequality , applied to and integrated against , gives . The right side is the unnormalized squared Hellinger distance. Infinite divergence and zero density regions are handled by the usual extended-integral conventions.
A perturbation can have negligible Hellinger distance but a large integral of its density's fourth power. At the uniform density on , let on and zero elsewhere, and let . Then and , so the score function is zero. However . Thus the density fourth-power functional is not continuous along this differentiable-in-quadratic-mean path, despite a bounded baseline and individually bounded nearby densities.
The Hellinger distance convention , with no factor , for densities under a common dominating measure. Its range is . This convention makes hold with the displayed constants.
A Bayesian inverse problem is well posed in Hellinger distance when every datum determines a unique posterior and the posterior depends continuously on the data in Hellinger distance. Since posterior measures are dominated by the prior and squared Hellinger distance is at most twice total variation distance, total-variation well-posedness implies Hellinger well-posedness.