The Hellinger distance is the square root of a constant multiple of . Common conventions use either the factor or .
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.
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.
For the unnormalized Hellinger distance, . Factor and use the Cauchy-Schwarz inequality to bound the total variation distance. For the other bound, gives , whose integral is the squared unnormalized Hellinger distance. Infinite Kullback-Leibler divergence is allowed.
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.
If is a measurable function into a separable Banach space and has finite second moments under probability measures , then their Bochner integral expected values satisfyHere 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 isTo 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.
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