Hellinger distance

Hellinger distance

In probability theory, a branch of mathematics, given two probability measures "P" and "Q" that are absolutely continuous in respect to a third probability measure λ, the square of the Hellinger distance between "P" and "Q" is defined as the quantity

:H^2(P,Q) = frac{1}{2}displaystyle int left(sqrt{frac{dP}{dlambda - sqrt{frac{dQ}{dlambda ight)^2 dlambda.

Here, "dP" / "dλ" and "dQ" / "d"λ are the Radon-Nikodym derivatives of "P" and "Q" respectively. This definition does not depend on λ, so the Hellinger distance between "P" and "Q" does not change if λ is replaced with a different probability measure in respect to which both "P" and "Q" are absolutely continuous.

For compactness, the above formula is often written as

:H^2(P,Q) = frac{1}{2}int left(sqrt{dP} - sqrt{dQ} ight)^2.

Some authors omit the factor 1/2 in front of the integral.

The Hellinger distance "H"("P", "Q") thus defined satisfies the property

: 0le H(P,Q) le 1.

The Hellinger distance is related to the Bhattacharyya distance BC(P,Q) as it can be defined as

: H(P,Q) = frac{1}{2} sqrt{(2-2 BC(P,Q))}.

Example

The Hellinger distance "H"("P", "Q") between two normal distributions Psimmathcal{N}(x;mu_1,sigma_1^2) and Qsimmathcal{N}(x;mu_2,sigma_2^2) is: Hleft(P, Q ight)=sqrt{frac{1}{2}-sqrt{frac{sigma_1sigma_2}{2left(sigma_1^2+sigma_2^2 ight)}e^{-frac{1}{2}frac{left(mu_1-mu_2 ight)^2}{sigma_1^2+sigma_2^2

References

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