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where $n\in0,1,2,\ldots$ is the Landau orbital quantum number. \req{kgp} differentiates between electrons and positrons which is to ensure the correct non-relativistic limit is reached; see \rf{tab:1}. The parameter $g$ is the gyro-magnetic ($g$-factor) of the particle. Following the conventions found in \cite{Tiesinga:2021myr}, we set $g\equiv g_{e^{+}}=-g_{e^{-}}>0$ such that electrons and positrons have opposite $g$-factors and opposite magnetic moments.
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where $n\in0,1,2,\ldots$ is the Landau orbital quantum number. \req{kgp} differentiates between electrons and positrons which is to ensure the correct non-relativistic limit is reached; see \rf{fig:schematic}. The parameter $g$ is the gyro-magnetic ($g$-factor) of the particle. Following the conventions found in \cite{Tiesinga:2021myr}, we set $g\equiv g_{e^{+}}=-g_{e^{-}}>0$ such that electrons and positrons have opposite $g$-factors and opposite magnetic moments which is schematically shown in \rf{fig:schematic}.
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As statistical properties depend on the characteristic Boltzmann factor $E/T$, another interpretation of \req{tbscale} in the context of energy eigenvalues (such as those given in \req{kgp}) is the preservation of magnetic moment energy relative to momentum under adiabatic cosmic expansion.
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@@ -250,7 +250,7 @@ \section{Theory of thermal matter-antimatter plasmas}
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\cline{2-3}
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\end{tabular}
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\caption{Organizational schematic of matter-antimatter $(\sigma)$ and polarization $(s)$ states with respect to the sign of the non-relativistic magnetic dipole energy $U_{\rm Mag}$ (obtainable from \req{kgp}) and the chemical $\mu$ and polarization $\eta$ potentials as seen in \req{partitionpower:2}.}
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\label{tab:1}
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\label{fig:schematic}
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\end{figure}
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@@ -283,22 +283,24 @@ \subsection{Spin and spin-orbit partition functions}
\req{partitionpower:3} allows us to reorganize the partition function with a new magnetization quantum number $s'$ which characterizes paramagnetic flux increasing states $(s'=+1)$ and diamagnetic flux decreasing states $(s'=-1)$. This recasts \req{partitionpower:2} as {\color{red}(maybe we should show $\epsilon_{s^\prime}=\epsilon_{++},\epsilon_{+-}$ clear )}
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\req{partitionpower:3} allows us to reorganize the partition function with a new magnetization quantum number $s'$ which characterizes paramagnetic flux increasing states $(s'=+1)$ and diamagnetic flux decreasing states $(s'=-1)$. This recasts \req{partitionpower:2} as
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