From a2bdaa0c75f904272dcad3bea6aae88f62dc0754 Mon Sep 17 00:00:00 2001
From: Andrew James Steinmetz <ajsteinmetz@arizona.edu>
Date: Tue, 7 Nov 2023 19:25:57 -0700
Subject: [PATCH] Black revised copy to be resubmitted to PRD.

---
 plasma-partition.tex | 4 ++--
 1 file changed, 2 insertions(+), 2 deletions(-)

diff --git a/plasma-partition.tex b/plasma-partition.tex
index c49744e..e935bac 100644
--- a/plasma-partition.tex
+++ b/plasma-partition.tex
@@ -59,7 +59,7 @@
 
 % Useful macros for annotation
 \newcommand*{\xred}{\color{red}}
-\newcommand*{\xblue}{\color{blue}}
+\newcommand*{\xblue}{\color{black}}
 \newcommand*{\xgreen}{\color{green}}
 
 \begin{document}
@@ -71,7 +71,7 @@
 \affiliation{Department of Physics, The University of Arizona, Tucson, AZ 85721, USA}
 
 %\date{\today}
-\date{August 28, 2023}
+\date{November 7, 2023}
 
 \begin{abstract}
 We explore the hypothesis that the abundant presence of relativistic antimatter (positrons) in the primordial universe is the source of the intergalactic magnetic fields we observe in the universe today. We evaluate both Landau diamagnetic and magnetic dipole moment paramagnetic properties of the very dense primordial electron-positron $e^{+}e^{-}$-plasma, and obtain in quantitative terms the relatively small magnitude of the $e^{+}e^{-}$ magnetic moment polarization asymmetry required to produce a consistent self-magnetization in the universe.