Update 2022-03-15 10:07
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@@ -1,7 +1,7 @@
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<!DOCTYPE html>
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<html lang="en">
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<head>
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<!-- 2022-03-07 Mon 20:38 -->
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<!-- 2022-03-15 Tue 08:10 -->
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<meta charset="utf-8">
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<meta name="viewport" content="width=device-width, initial-scale=1">
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<title>Pre-Quantum Electrodynamics</title>
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@@ -1310,10 +1310,6 @@ Table of contents
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</summary>
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<ul>
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<li>
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<a href="./d_m.html#d_m">Diagnostics: Mathematical Preliminaries</a><span class="headline-id">d.m</span>
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</li>
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<li>
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<a href="./d_ems.html#d_ems">Diagnostics: Electromagnetostatics</a><span class="headline-id">d.ems</span>
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</li>
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@@ -1352,6 +1348,10 @@ Table of contents
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<li>
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<a href="./d_red.html#d_red">Diagnostics: Relativistic Electrodynamics</a><span class="headline-id">d.red</span>
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</li>
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<li>
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<a href="./d_m.html#d_m">Diagnostics: Compendium - Mathematics</a><span class="headline-id">d.m</span>
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</li>
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</ul>
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@@ -1613,21 +1613,21 @@ Table of contents
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<path d="M9 5.5a3 3 0 0 0-2.83 4h1.098A2 2 0 0 1 9 6.5h3a2 2 0 1 1 0 4h-1.535a4.02 4.02 0 0 1-.82 1H12a3 3 0 1 0 0-6H9z"/>
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</svg></a><span class="headline-id">red.rm.rme</span></h4>
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<div class="outline-text-4" id="text-red_rm_rme">
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<div class="core div" id="org0915366">
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<div class="core div" id="org37554a5">
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<p>
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The {\bf relativistic momentum} \({\boldsymbol p}\) is defined as
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The <b>relativistic momentum</b> \({\boldsymbol p}\) is defined as
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\[
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{\boldsymbol p} \equiv m {\boldsymbol \eta} =
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\frac{m {\boldsymbol u}}{1 - u^2/c^2}.
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\]
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The {\bf relativistic energy} is defined as
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{\boldsymbol p} \equiv m {\boldsymbol \eta} =
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\frac{m {\boldsymbol u}}{1 - u^2/c^2}.
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\]
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The <b>relativistic energy</b> is defined as
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\[
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E \equiv \frac{m c^2}{\sqrt{1 - u^2/c^2}}.
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\]
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These can be combined into the {\bf energy-momentum four-vector}
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E \equiv \frac{m c^2}{\sqrt{1 - u^2/c^2}}.
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\]
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These can be combined into the <b>energy-momentum four-vector</b>
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\[
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p^\mu \equiv m \eta^\mu.
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\]
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p^\mu \equiv m \eta^\mu.
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\]
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</p>
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</div>
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@@ -1635,12 +1635,12 @@ These can be combined into the {\bf energy-momentum four-vector}
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<p>
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When the object is stationary, its energy is the
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</p>
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<div class="core div" id="orgb6d41ac">
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<div class="core div" id="orgf6b283a">
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<p>
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{\bf Rest energy}
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<b>Rest energy</b>
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\[
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E_{\mbox{\tiny rest}} \equiv m c^2.
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\]
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E_{\mbox{rest}} \equiv m c^2.
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\]
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</p>
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</div>
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@@ -1648,12 +1648,12 @@ When the object is stationary, its energy is the
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When moving, the difference between relativistic and rest energies
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is the
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</p>
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<div class="core div" id="org38aad5f">
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<div class="core div" id="org8d28e60">
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<p>
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{\bf Kinetic energy}
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<b>Kinetic energy</b>
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\[
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E_{\mbox{\tiny kin}} \equiv E - mc^2 = mc^2 \left( \frac{1}{\sqrt{1-u^2/c^2}} - 1 \right).
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\]
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E_{\mbox{kin}} \equiv E - mc^2 = mc^2 \left( \frac{1}{\sqrt{1-u^2/c^2}} - 1 \right).
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\]
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</p>
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</div>
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@@ -1661,25 +1661,25 @@ is the
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For velocities much smaller than the speed of light, we can expand
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this to
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\[
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E_{\mbox{\tiny kin}} = \frac{1}{2} mu^2 + \frac{3}{8} \frac{mu^2}{c^2} + ...
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E_{\mbox{kin}} = \frac{1}{2} mu^2 + \frac{3}{8} \frac{mu^2}{c^2} + ...
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\]
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</p>
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<p>
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In a closed system,
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</p>
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<div class="core div" id="org7f507cd">
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<div class="core div" id="org0b3cfe4">
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<p>
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{\bf Total relativistic energy and momentum is conserved}
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<b>Total relativistic energy and momentum is conserved</b>
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\[
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E^2 - c^2 p^2 = m^2 c^4
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\]
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E^2 - c^2 p^2 = m^2 c^4
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\]
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</p>
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</div>
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<p>
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N.B.: don't confuse an {\bf invariant} quantity with a {\bf conserved} quantity.
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N.B.: don't confuse an <i>invariant</i> quantity with a <i>conserved</i> quantity.
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</p>
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</div>
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</div>
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@@ -1702,7 +1702,7 @@ target="_blank">Creative Commons Attribution 4.0 International License</a>.
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</div>
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<div id="postamble" class="status">
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<p class="author">Author: Jean-Sébastien Caux</p>
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<p class="date">Created: 2022-03-07 Mon 20:38</p>
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<p class="date">Created: 2022-03-15 Tue 08:10</p>
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<p class="validation"></p>
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</div>
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