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Porter-Thomas fluctuations
Let's talk about Porter-Thomas (PT) fluctuations! To do that, we need to start talking about:
The Porter-Thomas distribution
Long story short: The PT distribution is the $\chi^2$ distribution with one degree of freedom ($k = 1$). In nuclear physics we have a central concept, namely the gamma strength function, which is a statistical property of atomic nuclei which describes the nuclei's gamma decay probabilities. The dipole ($L = 1$) strength function is given by
$$ f_{X1}(E_{\gamma}, E_i, j_i, \pi_i) = \dfrac{16 \pi}{9 \hbar^3 c^3}\langle B(X1;\downarrow) \rangle (E_{\gamma}, E_i, j_i, \pi_i) \rho (E_i, j_i, \pi_i).\qquad (0) $$
See p. 230 of Bartholomew et. al. for the general definition. We can re-arrange eq. (0) to get
$$ \langle B(Xj_{\gamma}) \rangle (E_{\gamma}, E_i, j_i, \pi_i) = \dfrac{9 \hbar^3 c^3}{16 \pi} \dfrac{f_{Xj_{\gamma}}(E_{\gamma}, E_i, j_i, \pi_i)}{\rho (E_i, j_i, \pi_i)}.\qquad (1) $$
From eq. (1) we see that the GSF $(f)$ is proportional to the mean $B$ value with a proportionality constant of $9 \hbar^3 c^3/(16 \pi \rho)$. The $B$ values deviate from the mean $B$ value by
$$ y = \dfrac{B}{\langle B \rangle} $$
and the distribution of $y$ values are hypothesised to follow the $\chi^2_1$ distribution, aka. the Porter-Thomas distribution.
Discussion