Update 2022-03-15 10:07
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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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@@ -1614,24 +1614,24 @@ Table of contents
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</svg></a><span class="headline-id">red.sr.4v</span></h4>
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<div class="outline-text-4" id="text-red_sr_4v">
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<p>
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\paragraph{Four-vectors.} Let's introduce the standard notations
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<b>Four-vectors</b>: let's introduce the standard notations
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\[
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x^0 \equiv ct, \hspace{10mm} \beta \equiv \frac{v}{c},
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\hspace{10mm} x^1 = x, ~~x^2 = y, ~~x^3 = z.
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\]
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The Lorentz transformation then reads
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</p>
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<div class="core div" id="org5cbcae9">
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<div class="core div" id="orgf4d6e6e">
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<p>
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{\bf Lorentz transformation (motion along \(x\) at velocity \(v\))}
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\[
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<b>Lorentz transformation</b> (motion along \(x\) at velocity \(v\))
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\[
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\bar{x}^0 = \gamma \left( x^0 - \beta x^1 \right),
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~~~~\bar{x}^1 = \gamma \left( x^1 - \beta x^0 \right),
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~~~~\bar{x}^2 = x^2,
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~~~~\bar{x}^3 = x^3
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\]
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or in matrix form
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\[
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or in matrix form
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\[
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\left( \begin{array}{c} \bar{x}^0 \\ \bar{x}^1 \\ \bar{x}^2 \\ \bar{x}^3
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\end{array} \right)
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= \left( \begin{array}{cccc}
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@@ -1647,17 +1647,17 @@ or in matrix form
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<p>
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This can be compactly written as
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\[
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\bar{x}^\mu = \sum_{\nu = 0}^3 \Lambda^\mu_\nu x^\nu.
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\bar{x}^\mu = \sum_{\nu = 0}^3 \Lambda^\mu{}_\nu x^\nu.
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\]
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</p>
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<p>
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\paragraph{Covariant and contravariant vectors.} Four-vectors with
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upper index are called {\it contravariant}. Their lower-index
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counterparts are called {\it covariant} vectors and are obtained by
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<b>Covariant and contravariant vectors</b>: four-vectors with
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upper index are called <b>contravariant</b>. Their lower-index
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counterparts are called <b>covariant</b> vectors and are obtained by
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using the Minkowski metric \(g_{\mu \nu}\) according to
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</p>
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<div class="main div" id="org6643ea5">
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<div class="main div" id="orge005c2f">
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<p>
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\[
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a_\mu = \sum_{\nu = 0}^3 g_{\mu \nu} a^\nu, \hspace{10mm}
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@@ -1671,9 +1671,9 @@ using the Minkowski metric \(g_{\mu \nu}\) according to
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</div>
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<p>
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\paragraph{Scalar products} are defined as the in-product of covariant/contravariant four-vectors,
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<b>Scalar products</b> are defined as the in-product of covariant/contravariant four-vectors,
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</p>
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<div class="main div" id="orge05e08a">
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<div class="main div" id="org411b956">
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<p>
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\[
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\sum_{\mu = 0}^3 a^\mu b_\mu \equiv a^\mu b_\mu
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@@ -1683,7 +1683,7 @@ using the Minkowski metric \(g_{\mu \nu}\) according to
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</div>
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<p>
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where in the right-hand side we have introduced the
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{\bf Einstein summation convention}, namely that any repeated index
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<b>Einstein summation convention</b>, namely that any repeated index
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is implicitly summed over. As you can trivially check, it doesn't matter
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which vector is co/contravariant: \(a^\mu b_\mu = a_\mu b^\mu\).
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Scalar products are Lorentz-invariant and thus take the same value in
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@@ -1691,25 +1691,45 @@ all inertial systems.
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</p>
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<p>
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\paragraph{Invariant intervals.} Generalizing the notion of the norm of
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<b>Invariant intervals</b>: generalizing the notion of the norm of
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a vector, the scalar product of a four-vector with itself is known as
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the invariant interval. Because of the geometry of spacetime, the invariant
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can take positive or negative values. The nomenclature goes as follows:
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</p>
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\begin{center}
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\begin{tabular}{cc}
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$a^\mu a_\mu > 0$ & $a^\mu$ is {\it spacelike} \\
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$a^\mu a_\mu < 0$ & $a^\mu$ is {\it timelike} \\
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$a^\mu a_\mu = 0$ & $a^\mu$ is {\it lightlike}
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\end{tabular}
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\end{center}
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<table>
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<colgroup>
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<col class="org-left">
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<col class="org-left">
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</colgroup>
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<tbody>
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<tr>
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<td class="org-left">\(a^\mu a_\mu > 0\)</td>
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<td class="org-left">\(a^\mu\) is {\it spacelike}</td>
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</tr>
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<tr>
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<td class="org-left">\(a^\mu a_\mu < 0\)</td>
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<td class="org-left">\(a^\mu\) is {\it timelike}</td>
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</tr>
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<tr>
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<td class="org-left">\(a^\mu a_\mu = 0\)</td>
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<td class="org-left">\(a^\mu\) is {\it lightlike}</td>
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</tr>
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</tbody>
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</table>
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<p>
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For two events \(A\) and \(B\), the difference
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\[
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\Delta x^\mu \equiv x_A^\mu - x_B^\mu
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\]
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is called the {\bf displacement four-vector} and its self-scalar product
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is the {\bf invariant interval} between the two events:
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is called the <b>displacement four-vector</b> and its self-scalar product
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is the <b>invariant interval</b> between the two events:
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\[
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I \equiv \Delta x^\mu \Delta x_\mu = -c^2 \Delta t^2 + |{\boldsymbol x}|^2
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\]
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@@ -1718,12 +1738,12 @@ is their spatial separation vector.
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</p>
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<p>
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\paragraph{Spacetime diagrams.} These are also know as
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{\it Minkowski diagrams}. Time is on the vertical axis, space on the
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<b>Spacetime diagrams</b>: these are also know as
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<b>Minkowski diagrams</b>. Time is on the vertical axis, space on the
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horizontal one. The trajectory of a particle is known as its
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{\bf world line}. Light is represented as propagating at lines at
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45 degrees, defining the {\bf forward} and
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{\bf backward light cones}. Lorentz transformations, which preserve
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<b>world line</b>. Light is represented as propagating at lines at
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45 degrees, defining the <i>forward</i> and
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<i>backward light cones</i>. Lorentz transformations, which preserve
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all invariant intervals, move spacetime points around but leave them
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on the same hyperboloid.
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</p>
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@@ -1746,7 +1766,7 @@ 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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