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	<id>https://www.conservapedia.com/index.php?action=history&amp;feed=atom&amp;title=Quantised_Inertia</id>
	<title>Quantised Inertia - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://www.conservapedia.com/index.php?action=history&amp;feed=atom&amp;title=Quantised_Inertia"/>
	<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;action=history"/>
	<updated>2026-11-06T06:00:35Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.35.14</generator>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763812&amp;oldid=prev</id>
		<title>Mark25: Layout</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763812&amp;oldid=prev"/>
		<updated>2021-06-01T21:56:39Z</updated>

		<summary type="html">&lt;p&gt;Layout&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&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 21:56, June 1, 2021&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-l8&quot; &gt;Line 8:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 8:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia combines these two predictions by saying that the horizon damps the Unruh waves on one side of the object—rather as sea defences damp ocean waves. The resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia combines these two predictions by saying that the horizon damps the Unruh waves on one side of the object—rather as sea defences damp ocean waves. The resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;Furthermore, &lt;/del&gt;Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon. As such, the waves of Unruh radiation are now damped equally all around, and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;further &lt;/ins&gt;predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon. As such, the waves of Unruh radiation are now damped equally all around, and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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='diff-marker'&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;/table&gt;</summary>
		<author><name>Mark25</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763800&amp;oldid=prev</id>
		<title>Mark25: Layout change</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763800&amp;oldid=prev"/>
		<updated>2021-06-01T21:14:40Z</updated>

		<summary type="html">&lt;p&gt;Layout change&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&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 21:14, June 1, 2021&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-l3&quot; &gt;Line 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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 phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass, for the first time, by combining two predictions:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass, for the first time, by combining two predictions:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;# From relativity, an accelerating object will see a Rindler horizon a certain distance &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;away, in &lt;/del&gt;the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light.  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;# From relativity, an accelerating object will see a Rindler horizon a certain distance &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;away—in &lt;/ins&gt;the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light.  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;# An accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation, as the horizon splits virtual particles, so that they become real.  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;# An accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation, as the horizon splits virtual particles, so that they become real.  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Mark25</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763799&amp;oldid=prev</id>
		<title>Mark25: Attempts at layout changes</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763799&amp;oldid=prev"/>
		<updated>2021-06-01T21:11:40Z</updated>

		<summary type="html">&lt;p&gt;Attempts at layout changes&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&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 21:11, June 1, 2021&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass for the first time by combining two predictions&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;. The first prediction is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;for the first time&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;by combining two predictions&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;:&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;Further&lt;/del&gt;, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;and so &lt;/del&gt;the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;# From relativity, an accelerating object will see a Rindler horizon a certain distance away, in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;# An accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation, as the horizon splits virtual particles, so that they become real. &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;Quantised Inertia combines these two predictions by saying that the horizon damps the Unruh waves on one side of the object—rather as sea defences damp ocean waves. The resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;Furthermore&lt;/ins&gt;, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. As such, &lt;/ins&gt;the waves of Unruh radiation are now damped equally all around&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, &lt;/ins&gt;and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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='diff-marker'&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;/table&gt;</summary>
		<author><name>Mark25</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763788&amp;oldid=prev</id>
		<title>Mark25: Typo: changed &quot;of&quot; to &quot;for&quot;</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763788&amp;oldid=prev"/>
		<updated>2021-06-01T20:42:45Z</updated>

		<summary type="html">&lt;p&gt;Typo: changed &amp;quot;of&amp;quot; to &amp;quot;for&amp;quot;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&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 20:42, June 1, 2021&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;of &lt;/del&gt;the first time by combining two predictions. The first prediction is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;for &lt;/ins&gt;the first time by combining two predictions. The first prediction is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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='diff-marker'&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;/table&gt;</summary>
		<author><name>Mark25</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763761&amp;oldid=prev</id>
		<title>DeepHorizon at 19:24, June 1, 2021</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763761&amp;oldid=prev"/>
		<updated>2021-06-01T19:24:57Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
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				&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 19:24, June 1, 2021&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass of the first time by combining two predictions. The first prediction is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;|arxiv = 0612599 &lt;/del&gt;}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;|arxiv = 1302.2775 |bibcode=2012Ap&amp;amp;SS.342..575M. &lt;/del&gt;}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law: &amp;quot;Objects move in straight lines at constant speed unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass of the first time by combining two predictions. The first prediction is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration vector. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum pushes the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;|arxiv = 1207.7007 |bibcode=2012Ap&amp;amp;SS.342..575M. &lt;/del&gt;}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound to the galaxy. As a result, Quantised Inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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='diff-marker'&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;/table&gt;</summary>
		<author><name>DeepHorizon</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763758&amp;oldid=prev</id>
		<title>DeepHorizon at 19:23, June 1, 2021</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763758&amp;oldid=prev"/>
		<updated>2021-06-01T19:23:07Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&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 19:23, June 1, 2021&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch, from the University of Plymouth in the UK.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law &amp;quot;Objects move in straight lines unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass of the first time by combining two predictions. The first is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;push &lt;/del&gt;the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x |arxiv = 0612599 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 |arxiv = 1302.2775 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;The phenomenon of inertial mass is defined in Newton's First Law&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;: &lt;/ins&gt;&amp;quot;Objects move in straight lines &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;at constant speed &lt;/ins&gt;unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass of the first time by combining two predictions. The first &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;prediction &lt;/ins&gt;is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;vector&lt;/ins&gt;. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;pushes &lt;/ins&gt;the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x |arxiv = 0612599 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 |arxiv = 1302.2775 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;td class='diff-marker'&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;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;ot &lt;/del&gt;the galaxy. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Therefore &lt;/del&gt;Quantised &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;inertia &lt;/del&gt;predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 |arxiv = 1207.7007 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;to &lt;/ins&gt;the galaxy. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;As a result, &lt;/ins&gt;Quantised &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Inertia &lt;/ins&gt;predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 |arxiv = 1207.7007 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;==References==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>DeepHorizon</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763757&amp;oldid=prev</id>
		<title>DeepHorizon: Added two paragraphs of explanation and references.</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763757&amp;oldid=prev"/>
		<updated>2021-06-01T19:20:12Z</updated>

		<summary type="html">&lt;p&gt;Added two paragraphs of explanation and references.&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 19:20, June 1, 2021&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&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;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, from the University of Plymouth in the UK&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;The phenomenon of inertial mass is defined in Newton's First Law &amp;quot;Objects move in straight lines unless pushed on&amp;quot; but it has never been explained. Quantised inertia explains inertial mass of the first time by combining two predictions. The first is from relativity and states that an accelerating object will see a Rindler horizon a certain distance away in the direction opposite to that of its acceleration. This is because information is limited to travelling at the speed of light. The second prediction is that an accelerating object will see itself surrounded by a thermal bath of so-called Unruh radiation as the horizon splits virtual particles so that they become real. Quantised Inertia combines these by saying that the horizon damps the Unruh waves on one side of the object rather as sea defences would damp ocean waves and the resulting gradient in the quantum vacuum push the object back against it acceleration, explaining inertia.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2007|title=Modelling the Pioneer anomaly as modified inertia |journal=Monthly Notices of the Royal Astronomical Society |volume=376 |pages=338-342|doi=10.1111/j.1365-2966.2007.11433.x |arxiv = 0612599 }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2013|title=Inertia from an asymmetric Casimir effect |journal=EPL |volume=101 |pages=59001|doi=10.1209/0295-5075/101/59001 |arxiv = 1302.2775 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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;&gt; &lt;/td&gt;&lt;td class='diff-marker'&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 class=&quot;diffchange diffchange-inline&quot;&gt;Further, Quantised Inertia predicts that for objects with very low accelerations, such as stars at the edges of galaxies, the Rindler horizon moves so far back that it is close to the cosmic horizon and so the waves of Unruh radiation are now damped equally all around and the mechanism of inertia collapses. This explains why stars at the edge of galaxies can orbit faster than expected but still remain bound ot the galaxy. Therefore Quantised inertia predicts galaxy rotation perfectly without the need for dark matter or any adjustment.&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2012|title=Testing quantised inertia on galactic scales |journal=Astrophysics &amp;amp; Space Science |volume=342 |pages=575–578|doi=10.1007/s10509-012-1197-0 |arxiv = 1207.7007 |bibcode=2012Ap&amp;amp;SS.342..575M. }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt; {{cite journal|last=McCulloch |first=M.E. |year=2017|title=Galaxy rotations from quantised inertia and visible matter only |journal=Astrophysics &amp;amp; Space Science |volume=362 |pages=149|doi=10.1007/s10509-017-3128-6}}&amp;lt;/ref&amp;gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>DeepHorizon</name></author>
	</entry>
	<entry>
		<id>https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763217&amp;oldid=prev</id>
		<title>Mark25: Initial post</title>
		<link rel="alternate" type="text/html" href="https://www.conservapedia.com/index.php?title=Quantised_Inertia&amp;diff=1763217&amp;oldid=prev"/>
		<updated>2021-05-31T13:43:33Z</updated>

		<summary type="html">&lt;p&gt;Initial post&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Quantised Inertia (QI) is a theory of inertia first proposed in 2007 by physicist Mike McCulloch.&lt;/div&gt;</summary>
		<author><name>Mark25</name></author>
	</entry>
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