@@ -72,21 +72,21 @@ In all formulae given below, spin quantum numbers (e.g., $J$ ) are implicitly as
Let the angle-integrated cross sections from entrance channel $c$ to exit channel $c'$ with total angular momentum $J$ be represented by $\sigma_{cc'}$. This cross section is given in terms of the scattering matrix $U_{cc'}$ as
where $k_\alpha$ is the wave number (and $K_\alpha=\hbar k_\alpha=$ center-of-mass momentum) associated with incident particle pair $\alpha$, $g_{J\alpha}$ is the spin statistical factor, and $w_c$ is the Coulomb phase-shift difference. Note that $w_c$ is zero for non-Coulomb channels. (Details for the charged-particle case are presented in Section II.C.4.\ref{}) The spin statistical factor $g_{J\alpha}$ is given by
@@ -95,28 +95,28 @@ Here $E$ is the \textbf{laboratory} kinetic energy of the incident (moving) part
The scattering matrix $U$ can be written in terms of matrix $W$ as
\begin{equation}\label{eq:scat-matrix}
U_{cc'} = \Omega_cW_{cc'}\Omega_{c'}\:,
U_{cc'} = \Omega_cW_{cc'}\Omega_{c'}\:,
\end{equation}
\noindent
where $\Omega$ is given by
\begin{equation}\label{eq:omega}
\Omega_c = e^{i(w_c-\phi_c)}\:.
\Omega_c = e^{i(w_c-\phi_c)}\:.
\end{equation}
\noindent
Here again, $w_c$ is zero for non-Coulomb channels, and the potential scattering phase shifts for non-Coulomb interactions $\phi_c$ are defined in many references (e.g., \cite{lane_thomas_1958}) and shown in Table \ref{}. The matrix $W$ in Eq. \ref{eq:scat-matrix} is related to the R-matrix (in matrix notation with indices suppressed) via
\begin{equation}\label{eq:W-matrix}
W = P^{1/2}\left(I-RL\right)^{-1}\left(I-RL^*\right)P^{-1/2}\:.
W = P^{1/2}\left(I-RL\right)^{-1}\left(I-RL^*\right)P^{-1/2}\:.
\end{equation}
\noindent
The quantity $I$ in this equation represents the identity matrix, and superscript $*$ indicates a complex conjugate. The form of the R-matrix is given in Section IIA.1\ref{} in general Section II.B\ref{} for the versions used in SAMMY. The quantity $L$ in Eq. \ref{eq:W-matrix} is given by
\begin{equation}\label{eq:L-matrix}
L = (S-B) + iP \:,
L = (S-B) + iP \:,
\end{equation}
\noindent
...
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@@ -137,7 +137,7 @@ where $\rho$ is related to the center-of-mass momentum which in turn is related
as shown in Section II.C.2\ref{}. Here $\Xi_\alpha$ is the energy threshold for the particle pair $\alpha$, $m_\alpha$ and $M_\alpha$ are the masses of the two particles of particle pair $\alpha$, and $m$ and $M$ are the masses of the incident particle and target nuclide, respectively.
Appropriate formulae for $P$, $S$, and $\phi$ in the non-Coulomb case are shown in Table IIA.1. For two charged particles, formulae for the penetrabilities are given in Section II.C.4\ref{}.
Appropriate formulae for $P$, $S$, and $\phi$ in the non-Coulomb case are shown in Table IIA.1. For two charged particles, formulae for the penetrabilities are given in Section II.C.4\ref{tab:penetrabilities}.
The energy dependence of fission and capture widths is negligible over the energy range of these calculations. Therefore, a penetrability of unity may be used.
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...
@@ -160,10 +160,134 @@ The energy dependence of fission and capture widths is negligible over the energ
\end{tabular}
\begin{tablenotes}
\item[\textdagger]\footnotesize{The iterative formula for $\phi_l$ could also be defined by $B_l =(B_{l-1}+X_l)/(1-B_{l-1}X_l)$ where $B_l=tan(\rho-\phi_l)$ and $X_l=P_{l-1}/(l-S_l)$}
\item[\textdagger]\footnotesize{The iterative formula for $\phi_l$ could also be defined by $B_l =(B_{l-1}+X_l)/(1-B_{l-1}X_l)$ where $B_l=tan(\rho-\phi_l)$ and $X_l=P_{l-1}/(l-S_{l-1})$}
\end{tablenotes}
\end{threeparttable}
Formulae for a particular cross section type can be derived by summing over the terms in Eq. (II A.1)\ref{eq:sigma-ccprime}. For the total cross section, the sum over all possible exit channels and all spin groups gives
\begin{equation}\label{eq:sigma-tot}
\begin{aligned}
\sigma^{total}& = \sum_{\substack{incident \\ channels \\ c }}\sum_{\substack{all \\ channels \\ c' }}\sum_J \frac{\pi}{k_\alpha^2}g_\alpha|\delta_{cc'}-U_{cc'}|^2 \\
& = \frac{\pi}{k_\alpha^2}\sum_{J}g_J \sum_{\substack{incident \\ channels \\ c }}\sum_{\substack{all \\ channels \\ c' }}\left( \delta_{cc'}-U_{cc'}\delta_{cc'}-U^*_{cc'}\delta_{cc'}+\left|U_{cc'}\right|^2 \right) \\
The R-matrix was introduced in Eq. \ref{eq:W-matrix} as
\begin{equation}% don't ref, give \ref{eq:W-matrix}
W = P^{1/2}\left(I-RL\right)^{-1}\left(I-RL^*\right)P^{-1/2}\:,
\end{equation}
but the formula for the R-matrix was not given there. If $\lambda$ represents a particular resonance (or energy level), then the general form for the R-matrix is
\begin{equation}\label{eq:r-matrix}
R_{cc'} = \sum_\lambda\frac{\gamma_{\lambda c}\gamma_{\lambda c'}}{ E_\lambda - E }\delta_{J,J'}\:,
\end{equation}
where $E_\lambda$ represents the energy of the resonance, and the reduced width amplitude $\gamma$ is related to the partial width $\Gamma$ by
The sum in Eq. (II A1.2)\ref{eq:r-matrix} contains an infinite number of levels. All channels, including the ``gamma channel'' for which one of the particles is a photon, are represented by the channel indices.
The R-matrix is not the only possibility for parameterization of the scattering matrix. In the R-matrix formulation, equations are expressed in terms of channel-channel interactions. It is also possible to formulate scattering theory in terms of level-level interactions; this formulation uses what is called the A-matrix, which is defined as
Dividing by $(E_\mu- E)$, multiplying on the left by $\gamma_{\mu c'}$ and on the right by $\gamma_{\nu c''}$, and summing over $\mu$ puts this equation into the form