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	<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?action=history&amp;feed=atom&amp;title=Black_Hole_Engineering</id>
	<title>Black Hole Engineering - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?action=history&amp;feed=atom&amp;title=Black_Hole_Engineering"/>
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	<updated>2026-05-02T14:12:52Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.41.1</generator>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3841&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3841&amp;oldid=prev"/>
		<updated>2026-04-19T03:44:16Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 20:44, 18 April 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l378&quot;&gt;Line 378:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 378:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But there is another issue to consider.  If e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;), for e the fundamental charge, is not much less than 1, you will get significant discharging from the hawking radiation emitting unbalanced numbers of electrons and positrons.  For e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) much larger than 1 and for T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) much larger than 1, the discharge rate is approximately e&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;amp;Vscr; / &amp;amp;hbar;&amp;lt;ref name=&amp;quot;Carter 1974&amp;quot;&amp;gt;&amp;lt;/ref&amp;gt;.  In our previous example with a 100 million ton black hole, e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) is about 10,000 and T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) is about 200.  Because these are much larger than 1 we can use our discharging estimate to find a discharge current of I = 24 million A.  In a tiny fraction of a second, our charged black hole would be neutral again.  Keeping it charged requires a power of P = I &amp;amp;Vscr; = 24 million terawatts from our particle accelerator.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But there is another issue to consider.  If e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;), for e the fundamental charge, is not much less than 1, you will get significant discharging from the hawking radiation emitting unbalanced numbers of electrons and positrons.  For e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) much larger than 1 and for T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) much larger than 1, the discharge rate is approximately e&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;amp;Vscr; / &amp;amp;hbar;&amp;lt;ref name=&amp;quot;Carter 1974&amp;quot;&amp;gt;&amp;lt;/ref&amp;gt;.  In our previous example with a 100 million ton black hole, e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) is about 10,000 and T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) is about 200.  Because these are much larger than 1 we can use our discharging estimate to find a discharge current of I = 24 million A.  In a tiny fraction of a second, our charged black hole would be neutral again.  Keeping it charged requires a power of P = I &amp;amp;Vscr; = 24 million terawatts from our particle accelerator.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But we have one more lever left to pull here.  Momentum is conserved, so if we can get our black hole to consume matter moving at high speed the momentum of the matter the black hole eats will be transferred to the black hole.  With a little bit of calculus you can find that for a Bondi-limited black hole, the optimum speed to shoot your mass stream at the black hole is &amp;amp;radic;2 c&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;.  The force on the black hole is v m&amp;amp;#775;&amp;lt;sub&amp;gt;BH&amp;lt;/sub&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But we have one more lever left to pull here.  Momentum is conserved, so if we can get our black hole to consume matter moving at high speed the momentum of the matter the black hole eats will be transferred to the black hole.  With a little bit of calculus you can find that for a Bondi-limited black hole, the optimum speed to shoot your mass stream at the black hole is &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;v = &lt;/ins&gt;&amp;amp;radic;2 c&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;.  The force on the black hole is v m&amp;amp;#775;&amp;lt;sub&amp;gt;BH&amp;lt;/sub&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Again for our example 100 million ton black hole, if we shoot it with a jet of thallium at 1157 m/s (the optimum for thallium&amp;#039;s speed of sound) the black hole will experience a force of 2.7 N and an acceleration of 2.7&amp;amp;times;10&amp;lt;sup&amp;gt;-11&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  This is still much less than the gravity tractor that was the first suggestion we floated for pulling a black hole; but at least it is much better than using electric or magnetic fields!  Again, this is just one example.  Black holes with different masses will get different results.  In particular, because the Bondi accretion rate increases proportionally to the square of the mass, the acceleration you can get from shooting your black hole with a mass jet will increase linearly with its mass and thus favor larger black holes for more reasonable accelerations.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Again for our example 100 million ton black hole, if we shoot it with a jet of thallium at 1157 m/s (the optimum for thallium&amp;#039;s speed of sound) the black hole will experience a force of 2.7 N and an acceleration of 2.7&amp;amp;times;10&amp;lt;sup&amp;gt;-11&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  This is still much less than the gravity tractor that was the first suggestion we floated for pulling a black hole; but at least it is much better than using electric or magnetic fields!  Again, this is just one example.  Black holes with different masses will get different results.  In particular, because the Bondi accretion rate increases proportionally to the square of the mass, the acceleration you can get from shooting your black hole with a mass jet will increase linearly with its mass and thus favor larger black holes for more reasonable accelerations.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3840&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3840&amp;oldid=prev"/>
		<updated>2026-04-18T16:18:10Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 09:18, 18 April 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l374&quot;&gt;Line 374:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 374:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For electric containment, it is interesting to note that because r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt; is proportional to the black hole mass, the capacitance is also proportional to the mass.  So for a given attainable voltage the charge on the black hole is proportional to the mass.  And consequently, for a given electric field the force on the black hole is proportional to the mass.  With the final result that for a fixed voltage and electric field strength, the acceleration of the black hole you can get with electric methods is entirely independent of its mass.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For electric containment, it is interesting to note that because r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt; is proportional to the black hole mass, the capacitance is also proportional to the mass.  So for a given attainable voltage the charge on the black hole is proportional to the mass.  And consequently, for a given electric field the force on the black hole is proportional to the mass.  With the final result that for a fixed voltage and electric field strength, the acceleration of the black hole you can get with electric methods is entirely independent of its mass.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;.  In particular, for a given voltage and magnetic field gradient, the acceleration should scale linearly with the black hole mass, thus favoring larger black holes&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But there is another issue to consider.  If e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;), for e the fundamental charge, is not much less than 1, you will get significant discharging from the hawking radiation emitting unbalanced numbers of electrons and positrons.  For e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) much larger than 1 and for T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) much larger than 1, the discharge rate is approximately e&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;amp;Vscr; / &amp;amp;hbar;&amp;lt;ref name=&amp;quot;Carter 1974&amp;quot;&amp;gt;&amp;lt;/ref&amp;gt;.  In our previous example with a 100 million ton black hole, e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) is about 10,000 and T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) is about 200.  Because these are much larger than 1 we can use our discharging estimate to find a discharge current of I = 24 million A.  In a tiny fraction of a second, our charged black hole would be neutral again.  Keeping it charged requires a power of P = I &amp;amp;Vscr; = 24 million terawatts from our particle accelerator.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But there is another issue to consider.  If e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;), for e the fundamental charge, is not much less than 1, you will get significant discharging from the hawking radiation emitting unbalanced numbers of electrons and positrons.  For e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) much larger than 1 and for T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) much larger than 1, the discharge rate is approximately e&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; &amp;amp;Vscr; / &amp;amp;hbar;&amp;lt;ref name=&amp;quot;Carter 1974&amp;quot;&amp;gt;&amp;lt;/ref&amp;gt;.  In our previous example with a 100 million ton black hole, e &amp;amp;Vscr; / (T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;) is about 10,000 and T&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; k&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; / (m&amp;lt;sub&amp;gt;e&amp;lt;/sub&amp;gt; c&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;) is about 200.  Because these are much larger than 1 we can use our discharging estimate to find a discharge current of I = 24 million A.  In a tiny fraction of a second, our charged black hole would be neutral again.  Keeping it charged requires a power of P = I &amp;amp;Vscr; = 24 million terawatts from our particle accelerator.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3839&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3839&amp;oldid=prev"/>
		<updated>2026-04-18T15:49:49Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 08:49, 18 April 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l370&quot;&gt;Line 370:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 370:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-17&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-18&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-17&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-18&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;.  &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;For electric containment, it is interesting to note that because r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt; is proportional to the black hole mass, the capacitance is also proportional to the mass.  So for a given attainable voltage the charge on the black hole is proportional to the mass.  And consequently, for a given electric field the force on the black hole is proportional to the mass.  With the final result that for a fixed voltage and electric field strength, the acceleration of the black hole you can get with electric methods is entirely independent of its mass&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3836&amp;oldid=prev</id>
		<title>Lwcamp: /* Hawking radiation */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3836&amp;oldid=prev"/>
		<updated>2026-04-13T14:19:59Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Hawking radiation&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 07:19, 13 April 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l128&quot;&gt;Line 128:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 128:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Temperature (K) &amp;lt;td&amp;gt; &amp;amp;lt;&amp;amp;lt; 1200 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 1200 &amp;amp; &amp;amp;lt;&amp;amp;lt; 6 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt; &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 6 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt; &amp;amp; &amp;amp;lt;&amp;amp;lt; 1.2 &amp;amp;times; 10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Temperature (K) &amp;lt;td&amp;gt; &amp;amp;lt;&amp;amp;lt; 1200 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 1200 &amp;amp; &amp;amp;lt;&amp;amp;lt; 6 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt; &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 6 &amp;amp;times; 10&amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt; &amp;amp; &amp;amp;lt;&amp;amp;lt; 1.2 &amp;amp;times; 10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Temperature (eV) &amp;lt;td&amp;gt; &amp;amp;lt;&amp;amp;lt; 0.1 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 0.1 &amp;amp; &amp;amp;lt;&amp;amp;lt; 500,000 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 500,000 &amp;amp; &amp;amp;lt;&amp;amp;lt; 100,000,000&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Temperature (eV) &amp;lt;td&amp;gt; &amp;amp;lt;&amp;amp;lt; 0.1 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 0.1 &amp;amp; &amp;amp;lt;&amp;amp;lt; 500,000 &amp;lt;td&amp;gt; &amp;amp;gt;&amp;amp;gt; 500,000 &amp;amp; &amp;amp;lt;&amp;amp;lt; 100,000,000&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Electromagnetic fraction &amp;lt;td&amp;gt; 90% &amp;lt;td&amp;gt; &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;17&lt;/del&gt;% &amp;lt;td&amp;gt; 7.6%&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Electromagnetic fraction &amp;lt;td&amp;gt; 90% &amp;lt;td&amp;gt; &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;11.8&lt;/ins&gt;% &amp;lt;td&amp;gt; 7.6%&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Gravitational fraction &amp;lt;td&amp;gt; 10% &amp;lt;td&amp;gt; &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;2&lt;/del&gt;% &amp;lt;td&amp;gt; 0.9%&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Gravitational fraction &amp;lt;td&amp;gt; 10% &amp;lt;td&amp;gt; &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;1.4&lt;/ins&gt;% &amp;lt;td&amp;gt; 0.9%&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Neutrino fraction &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;81&lt;/del&gt;% &amp;lt;td&amp;gt; 55.7%  &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Neutrino fraction &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;86.8&lt;/ins&gt;% &amp;lt;td&amp;gt; 55.7%  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Electron &amp;amp; Positron fraction &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; 35.8%&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;tr&amp;gt;&amp;lt;td&amp;gt;Electron &amp;amp; Positron fraction &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; 0 &amp;lt;td&amp;gt; 35.8%&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;/table&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;/table&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3780&amp;oldid=prev</id>
		<title>Lwcamp at 18:59, 7 March 2026</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3780&amp;oldid=prev"/>
		<updated>2026-03-07T18:59:13Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 11:59, 7 March 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l385&quot;&gt;Line 385:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 385:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== References ==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Engineering‏‎]][[Category:Physics &amp;amp; Engineering‏‎]][[Category:Physics]][[Category:Astronomy &amp;amp; Cosmology]][[Category:Infrastructure]][[Category:Propulsion]]&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Engineering‏‎]][[Category:Physics &amp;amp; Engineering‏‎&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;]][[Category:Physics &amp;amp; Math &amp;amp; Engineering&lt;/ins&gt;]][[Category:Physics]][[Category:Astronomy &amp;amp; Cosmology]][[Category:Infrastructure]][[Category:Propulsion]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3640&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3640&amp;oldid=prev"/>
		<updated>2026-02-28T05:31:20Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:31, 27 February 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l363&quot;&gt;Line 363:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 363:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;where &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; = 8.8541878188&amp;amp;times;10&amp;lt;sup&amp;gt;−12&amp;lt;/sup&amp;gt; F/m is the vacuum permittivity.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;where &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; = 8.8541878188&amp;amp;times;10&amp;lt;sup&amp;gt;−12&amp;lt;/sup&amp;gt; F/m is the vacuum permittivity.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The potential &amp;amp;Vscr;, in volts, for a black hole with a charge Q in coulombs, is&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The potential &amp;amp;Vscr;, in volts, for a black hole with a charge Q in coulombs, is&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div class=&quot;center&quot; style=&quot;width: auto; margin-left: auto; margin-right: auto;&quot;&amp;gt; &amp;amp;Vscr; = Q / C&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div class=&quot;center&quot; style=&quot;width: auto; margin-left: auto; margin-right: auto;&quot;&amp;gt; &amp;amp;Vscr; = Q / C &lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&amp;lt;/div&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;and the energy to charge the black hole up is&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;and the energy to charge the black hole up is&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; W = (1/2) C &amp;amp;Vscr;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; W = (1/2) C &amp;amp;Vscr;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3639&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3639&amp;oldid=prev"/>
		<updated>2026-02-28T05:30:23Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:30, 27 February 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l358&quot;&gt;Line 358:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 358:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;You can also electrically charge the black hole.  This will give it an electric field.  If the black hole is also spinning, the combination of spin and charge will give it a magnetic field.  You can then push or pull on the black hole with beefy capacitor plates or electromagnets.  However, it can be challenging to give a black hole a large charge, or to have it keep its charge for long.   &lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;You can also electrically charge the black hole.  This will give it an electric field.  If the black hole is also spinning, the combination of spin and charge will give it a magnetic field.  You can then push or pull on the black hole with beefy capacitor plates or electromagnets.  However, it can be challenging to give a black hole a large charge, or to have it keep its charge for long.   &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One problem is the electrical potential of the hole. &lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt; The potential &amp;amp;Vscr;, in volts, for a black hole with a charge Q in coulombs, is&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One problem is the electrical potential of the hole.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&amp;lt;div class=&quot;center&quot; style=&quot;width: auto; margin-left: auto; margin-right: auto;&quot;&amp;gt; &amp;amp;Vscr; = (1/(4 &amp;amp;pi; &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt;)) Q / r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A black hole will have a capacitance of  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;where &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; = 8.8541878188&amp;amp;times;10&amp;lt;sup&amp;gt;−12&amp;lt;/sup&amp;gt; F/m is the vacuum permittivity.  &lt;/del&gt;A black hole will have a capacitance of  &lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-added&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; C = 4 &amp;amp;pi; &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; C = 4 &amp;amp;pi; &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; r&amp;lt;sub&amp;gt;S&amp;lt;/sub&amp;gt;&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;where &amp;amp;epsilon;&amp;lt;sub&amp;gt;0&amp;lt;/sub&amp;gt; = 8.8541878188&amp;amp;times;10&amp;lt;sup&amp;gt;−12&amp;lt;/sup&amp;gt; F/m is the vacuum permittivity.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;The potential &amp;amp;Vscr;, in volts, for a black hole with a charge Q in coulombs, is&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-side-deleted&quot;&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&amp;lt;div class=&quot;center&quot; style=&quot;width: auto; margin-left: auto; margin-right: auto;&quot;&amp;gt; &amp;amp;Vscr; = Q / C&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;and the energy to charge the black hole up is&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;and the energy to charge the black hole up is&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; W = (1/2) C &amp;amp;Vscr;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&amp;lt;div align=center&amp;gt; W = (1/2) C &amp;amp;Vscr;&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.&amp;lt;/div&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3638&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3638&amp;oldid=prev"/>
		<updated>2026-02-28T05:25:56Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:25, 27 February 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l376&quot;&gt;Line 376:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 376:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But we have one more lever left to pull here.  Momentum is conserved, so if we can get our black hole to consume matter moving at high speed the momentum of the matter the black hole eats will be transferred to the black hole.  With a little bit of calculus you can find that for a Bondi-limited black hole, the optimum speed to shoot your mass stream at the black hole is &amp;amp;radic;2 c&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;.  The force on the black hole is v m&amp;amp;#775;&amp;lt;sub&amp;gt;BH&amp;lt;/sub&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;But we have one more lever left to pull here.  Momentum is conserved, so if we can get our black hole to consume matter moving at high speed the momentum of the matter the black hole eats will be transferred to the black hole.  With a little bit of calculus you can find that for a Bondi-limited black hole, the optimum speed to shoot your mass stream at the black hole is &amp;amp;radic;2 c&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;.  The force on the black hole is v m&amp;amp;#775;&amp;lt;sub&amp;gt;BH&amp;lt;/sub&amp;gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Again for our example 100 million ton black hole, if we shoot it with a jet of thallium at 1157 m/s (the optimum for thallium&#039;s speed of sound) the black hole will experience a force of 2.7 N and an acceleration of 2.7&amp;amp;times;10&amp;lt;sup&amp;gt;-11&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  This is still much less than the gravity tractor that was the first suggestion we floated for pulling a black hole; but at least it is much better than using electric or magnetic fields!  Again, this is just one example.  Black holes with different masses will get different results.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;Again for our example 100 million ton black hole, if we shoot it with a jet of thallium at 1157 m/s (the optimum for thallium&#039;s speed of sound) the black hole will experience a force of 2.7 N and an acceleration of 2.7&amp;amp;times;10&amp;lt;sup&amp;gt;-11&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  This is still much less than the gravity tractor that was the first suggestion we floated for pulling a black hole; but at least it is much better than using electric or magnetic fields!  Again, this is just one example.  Black holes with different masses will get different results&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;.  In particular, because the Bondi accretion rate increases proportionally to the square of the mass, the acceleration you can get from shooting your black hole with a mass jet will increase linearly with its mass and thus favor larger black holes for more reasonable accelerations&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== Credit ==&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;== Credit ==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3637&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3637&amp;oldid=prev"/>
		<updated>2026-02-28T05:20:02Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:20, 27 February 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l368&quot;&gt;Line 368:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 368:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;15&lt;/del&gt;&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;16&lt;/del&gt;&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;17&lt;/ins&gt;&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;18&lt;/ins&gt;&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
	<entry>
		<id>https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3636&amp;oldid=prev</id>
		<title>Lwcamp: /* Containment */</title>
		<link rel="alternate" type="text/html" href="https://www.galacticlibrary.net/mediawiki-1.41.1/index.php?title=Black_Hole_Engineering&amp;diff=3636&amp;oldid=prev"/>
		<updated>2026-02-28T05:18:04Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Containment&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 22:18, 27 February 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l368&quot;&gt;Line 368:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 368:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;With modern accelerators, we might get electrons up to an energy of 1 TeV (1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; eV), for a potential of &amp;amp;Vscr; = 1&amp;amp;times;10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; V.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;25&lt;/del&gt;&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;25&lt;/del&gt;&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;For our example 100 million ton black hole, this gives a charge of Q = 1.65&amp;amp;times;10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; C with a negligible charging energy.  We can put this next to a highly charged capacitor plate to accelerate it.  You can generate fields as high as the vacuum breakdown limit for the materials used to make your plate, which is typically about &amp;amp;#120020; ~= 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; V/m.  The force is F = Q &amp;amp;#120020;, or about (very roughly) 1 &amp;amp;mu;N.  Using F = M a, the acceleration a produced is a rather pathetic a ~= 10&amp;lt;sup&amp;gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;15&lt;/ins&gt;&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, or about 10&amp;lt;sup&amp;gt;-&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;16&lt;/ins&gt;&amp;lt;/sup&amp;gt; g&amp;lt;sub&amp;gt;&amp;amp;oplus;&amp;lt;/sub&amp;gt;.  This is not going to get anyone anywhere in a reasonable time!  But you can at least see the math needed to figure out how to move the hole so you can work other examples for yourself.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;br&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;If you have a charged rotating black hole, as described earlier it will have a magnetic moment.  If you put a magnetic moment in a magnetic field gradient dB/dx the magnetic moment will experience a force F = m dB/dx.  If we take our 100 million ton black hole charged up to a trillion volts from above, and give it enough spin that it becomes extremal, you will have an angular momentum of J = 2.2&amp;amp;times;10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; kg m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;/s.  This gives it a magnetic dipole moment of m = 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-33&amp;lt;/sup&amp;gt; A m&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.  The highest magnetic field gradients we have managed to achieve have been about a GT/m&amp;lt;ref&amp;gt;[Zablotskii, V., Polyakova, T., Lunov, O. et al. How a High-Gradient Magnetic Field Could Affect Cell Life. Sci Rep 6, 37407 (2016). https://doi.org/10.1038/srep37407&amp;lt;/ref&amp;gt;.  Thus, we have a force of approximately 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-21&amp;lt;/sup&amp;gt; N and an acceleration of about 3.7&amp;amp;times;10&amp;lt;sup&amp;gt;-32&amp;lt;/sup&amp;gt; m/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, which is many orders of magnitude worse than the already pathetic electric field case.  But again, using these tools you can work out for yourself the best way to move your black hole if your black hole is not 100 million tons or is charged to a different potential.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Lwcamp</name></author>
	</entry>
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