The following calculations are based on Jeffreys’s (1961, p. 269) Theory of Probability and elaborates why he choose to use a symmetric proper weighting function
on the test relevant parameter the population effect size
.
First, to relate the observed
-value to the population effect size
within
, Jeffreys rewrote the likelihood of
in terms of the effect size
and
. To calculate the weighted likelihood of
he then choose to set
. By assigning the same weighting function to
as was done for
, we obtain:
(1) ![]()
The remaining task is to specify
, the weighting function for the test-relevant parameter. Jeffreys proposed his weighting function
based on desiderata obtained from hypothetical, extreme data.
Predictive matching: Symmetric 
The first “extreme” case Jeffreys discusses is when
; this automatically yields
regardless of the value of
. Jeffreys noted that a single datum cannot provide support for
, as any deviation of
from zero can also be attributed to our lack of knowledge of
. Hence, nothing is learned from only one observation and consequently the Bayes factor should equal 1 whenever
.
To ensure that
whenever
, Jeffreys (1961, p. 269) entered
, thus,
and
into Eq. 2 and noted that
equals
, if
is taken to be symmetric around zero. The proof assumes that
and uses the transformation
, thus,
and
. Hence, by symmetry of
we get
(2) ![Rendered by QuickLaTeX.com \begin{align*} (2 \pi)^{1 \over 2} p(d \, | \, \mathcal{M}_{1}) = & \int_{0}^{\infty} \sigma^{-1} \int_{-\infty}^{\infty} \exp \left ( - {1 \over 2} \left [ (\xi - \delta )^{2} \right ] \right ) \pi_{1}(\delta ) \, \text{d} \delta \, \sigma^{-1} \text{d} \sigma \\ = & {1 \over x} \int_{0}^{\infty} \int_{-\infty}^{\infty} \exp \left ( - {1 \over 2} \left [ (\xi - \delta )^{2} \right ] \right ) \pi_{1}(\delta ) \, \text{d} \delta \, \text{d} \xi \\ = & {1 \over x} \Big [ \int_{\xi=0}^{\xi=\infty} \int_{\delta=0}^{\delta=\infty} \exp \left ( - {1 \over 2} \left [ (\xi - \delta )^{2} \right ] \right ) \pi_{1}(\delta ) \, \text{d} \delta \, \text{d} \xi \\ & + \int_{\xi=0}^{\xi=\infty} \int_{\delta=0}^{\delta=\infty} \exp \left ( - {1 \over 2} \left [ (\xi + \delta )^{2} \right ] \right ) \pi_{1}(\delta ) \, \text{d} \delta \, \text{d} \xi \Big ] \end{align*}](https://www.alexander-ly.com/wp-content/ql-cache/quicklatex.com-4256de07e9c1895358ca21dfb90039f0_l3.png)
By swapping the order of integration (Fubini) then yields an integral in terms of
that yields the normalisation constant of a normal distribution, that is,
(3) ![Rendered by QuickLaTeX.com \begin{align*} p(d \, | \, \mathcal{M}_{1}) = & (2 \pi)^{-{1 \over 2}} {1 \over x} \Big [ \int_{\xi=-\infty}^{\xi=\infty} \exp \left ( - {1 \over 2} \left [ (\xi - \delta )^{2} \right ] \right ) \, \text{d} \xi \int_{\delta=0}^{\delta=\infty} \pi_{1}(\delta ) \, \text{d} \delta \Big ] \\ = & {1 \over x} \int_{0}^{\infty} \pi_{1}(\delta) \text{d} \delta = {1 \over 2 x}. \end{align*}](https://www.alexander-ly.com/wp-content/ql-cache/quicklatex.com-4ebcf5efad0bace319b359b160adac2e_l3.png)
Hence, for
symmetric around zero the weighted likelihood of
is then equal to that of the null model whenever
and
.