Definition
Measure theory
To define the Hellinger distance in terms of measure theory, let
and
denote two probability measures on a measure space
that are absolutely continuous with respect to an auxiliary measure
. Such a measure always exists, e.g
. The square of the Hellinger distance between
and
is defined as the quantity

Here,
and
, i.e.
and
are the Radon–Nikodym derivatives of P and Q respectively with respect to
. This definition does not depend on
, i.e. the Hellinger distance between P and Q does not change if
is replaced with a different probability measure with respect to which both P and Q are absolutely continuous. For compactness, the above formula is often written as

Probability theory using Lebesgue measure
To define the Hellinger distance in terms of elementary probability theory, we take λ to be the Lebesgue measure, so that dP / dλ and dQ / dλ are simply probability density functions. If we denote the densities as f and g, respectively, the squared Hellinger distance can be expressed as a standard calculus integral

where the second form can be obtained by expanding the square and using the fact that the integral of a probability density over its domain equals 1.
The Hellinger distance H(P, Q) satisfies the property (derivable from the Cauchy–Schwarz inequality)

Discrete distributions
For two discrete probability distributions
and
,
their Hellinger distance is defined as

which is directly related to the Euclidean norm of the difference of the square root vectors, i.e.

Also,
Proof |
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Properties
The Hellinger distance forms a bounded metric on the space of probability distributions over a given probability space.
The maximum distance 1 is achieved when P assigns probability zero to every set to which Q assigns a positive probability, and vice versa.
Sometimes the factor
in front of the integral is omitted, in which case the Hellinger distance ranges from zero to the square root of two.
The Hellinger distance is related to the Bhattacharyya coefficient
as it can be defined as

Hellinger distances are used in the theory of sequential and asymptotic statistics.
The squared Hellinger distance between two normal distributions
and
is:

The squared Hellinger distance between two multivariate normal distributions
and
is

The squared Hellinger distance between two exponential distributions
and
is:

The squared Hellinger distance between two Weibull distributions
and
(where
is a common shape parameter and
are the scale parameters respectively):

The squared Hellinger distance between two Poisson distributions with rate parameters
and
, so that
and
, is:

The squared Hellinger distance between two beta distributions
and
is:

where
is the beta function.
The squared Hellinger distance between two gamma distributions
and
is:

where
is the gamma function.