The gravitational-wave signal will be buried in the noise of the detector and the data from the detector will
be a random process. Consequently the problem of extracting the signal from the noise is a statistical one.
The basic idea behind the signal detection is that the presence of the signal changes the statistical
characteristics of the data , in particular its probability distribution. When the signal is absent the
data have probability density function (pdf)
, and when the signal is present the pdf is
.
A full exposition of the statistical theory of signal detection that is outlined here can be found in the
monographs [102, 56, 98, 96, 66, 44
, 77]. A general introduction to stochastic processes is given in [100].
Advanced treatment of the subject can be found in [64, 101].
The problem of detecting the signal in noise can be posed as a statistical hypothesis testing problem.
The null hypothesis is that the signal is absent from the data and the alternative hypothesis
is
that the signal is present. A hypothesis test (or decision rule)
is a partition of the observation set into
two sets,
and its complement
. If data are in
we accept the null hypothesis, otherwise we
reject it. There are two kinds of errors that we can make. A type I error is choosing hypothesis
when
is true and a type II error is choosing
when
is true. In signal detection theory the
probability of a type I error is called the false alarm probability, whereas the probability of a type II
error is called the false dismissal probability.
is the probability
of detection of the signal. In hypothesis testing the probability of a type I error is called the
significance of the test, whereas
is called the power of the
test.
The problem is to find a test that is in some way optimal. There are several approaches to find such a test. The subject is covered in detail in many books on statistics, for example see references [54, 41, 62].
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