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		<title>JonoThora: Psionics expansion (01a + 01b): content authored / LaTeX-restored per local submodule; lint-clean.</title>
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		<summary type="html">&lt;p&gt;Psionics expansion (01a + 01b): content authored / LaTeX-restored per local submodule; lint-clean.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;= What is Frame Dragging? =&lt;br /&gt;
&lt;br /&gt;
{{Audience_Sidebar&lt;br /&gt;
| difficulty   = Beginner&lt;br /&gt;
| reading_time = 7 minutes&lt;br /&gt;
| prerequisites = High-school physics. Familiarity with the word &amp;quot;gravity&amp;quot;.&lt;br /&gt;
| if_too_basic_see = [[Lense-Thirring_Frame_Dragging]]&lt;br /&gt;
| if_you_want_the_math_see = [[Gravitoelectromagnetism]]&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
This page is the plain-language companion to [[Lense-Thirring_Frame_Dragging]]. It assumes no calculus and no relativity background.&lt;br /&gt;
&lt;br /&gt;
== The one-sentence version ==&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Frame dragging&amp;#039;&amp;#039;&amp;#039; is the prediction — confirmed by experiment — that a rotating massive object drags the very fabric of space and time around with it, just as a spinning ball in a pool of honey would drag the honey along.&lt;br /&gt;
&lt;br /&gt;
== The honey analogy ==&lt;br /&gt;
&lt;br /&gt;
Imagine a spinning ball in a thick, viscous fluid (honey, oil, glycerin). The ball doesn&amp;#039;t just sit there spinning — it pulls the fluid near it into rotation. Right at the surface, the fluid rotates almost as fast as the ball. A short distance away, slower. Far away, the fluid is barely affected.&lt;br /&gt;
&lt;br /&gt;
According to Einstein&amp;#039;s General Relativity, &amp;#039;&amp;#039;&amp;#039;spacetime itself behaves this way around a rotating mass&amp;#039;&amp;#039;&amp;#039;. The Earth, by rotating, drags spacetime around with it. An object falling freely near Earth doesn&amp;#039;t fall in a perfectly straight line as Newton would have it — its trajectory is twisted slightly by Earth&amp;#039;s rotation.&lt;br /&gt;
&lt;br /&gt;
The effect is tiny for Earth. For a rapidly-rotating black hole, the effect is so extreme that nothing — not even light — can stay still relative to the distant stars within a certain region around it (the &amp;quot;ergosphere&amp;quot;).&lt;br /&gt;
&lt;br /&gt;
== The gyroscope test ==&lt;br /&gt;
&lt;br /&gt;
How would you measure something this subtle?&lt;br /&gt;
&lt;br /&gt;
In ordinary space (Newton&amp;#039;s universe), a perfectly-balanced gyroscope keeps its spin axis pointed in the same direction forever, relative to the distant stars. Drop it in a free-fall orbit around Earth: same answer; the axis stays fixed.&lt;br /&gt;
&lt;br /&gt;
In Einstein&amp;#039;s universe, &amp;#039;&amp;#039;that&amp;#039;s wrong&amp;#039;&amp;#039;. The gyroscope&amp;#039;s axis precesses — drifts slowly in a predictable direction — for two reasons:&lt;br /&gt;
&lt;br /&gt;
# &amp;#039;&amp;#039;&amp;#039;Geodetic effect&amp;#039;&amp;#039;&amp;#039; (the curvature of spacetime around Earth&amp;#039;s mass) — the bigger of the two effects.&lt;br /&gt;
# &amp;#039;&amp;#039;&amp;#039;Frame-dragging&amp;#039;&amp;#039;&amp;#039; (the rotation of Earth pulling spacetime) — the smaller effect, and the one named after Lense and Thirring.&lt;br /&gt;
&lt;br /&gt;
In 2011, the [[Gravity_Probe_B]] satellite measured both effects directly using four fused-quartz superconducting gyroscopes in orbit. The numbers matched General Relativity:&lt;br /&gt;
&lt;br /&gt;
* Geodetic effect: &amp;#039;&amp;#039;&amp;#039;≈ 6,602 milliarcseconds per year&amp;#039;&amp;#039;&amp;#039; (out of 6,606 predicted).&lt;br /&gt;
* Frame-dragging: &amp;#039;&amp;#039;&amp;#039;≈ 37 milliarcseconds per year&amp;#039;&amp;#039;&amp;#039; (out of 39 predicted).&lt;br /&gt;
&lt;br /&gt;
A milliarcsecond is one three-millionth of a degree. The detection is exquisite, but the effect is real.&lt;br /&gt;
&lt;br /&gt;
== Why does this matter? ==&lt;br /&gt;
&lt;br /&gt;
Frame-dragging is one of the cleanest confirmations of General Relativity — and a stark reminder that gravity, in Einstein&amp;#039;s framework, is not a force in the Newtonian sense. It is the geometry of spacetime itself. Rotating mass twists that geometry. A spinning gyroscope, falling freely, traces out the twisted geometry.&lt;br /&gt;
&lt;br /&gt;
For [[Psionics|psionic-framework]] purposes, frame-dragging is the cleanest test of the &amp;quot;ψ → 0&amp;quot; limit. In the regime where the ψ field is negligible — which Earth-orbit certainly is — the framework predicts standard GR. [[Gravity_Probe_B]] confirms that standard GR is correct in this regime. Any deviation from GR in regions with &amp;#039;&amp;#039;strong&amp;#039;&amp;#039; ψ-field activity (rotating superconductors; high-coherence biological systems) would then constitute evidence for ψ-coupling.&lt;br /&gt;
&lt;br /&gt;
== The amplified version ==&lt;br /&gt;
&lt;br /&gt;
The framework predicts that in &amp;#039;&amp;#039;rotating superconductors&amp;#039;&amp;#039; — where the Cooper-pair condensate produces a coherent quantum state — frame-dragging-like effects can be &amp;#039;&amp;#039;&amp;#039;dramatically amplified&amp;#039;&amp;#039;&amp;#039; over the standard GR prediction. The [[Gravitomagnetic_London_Moment|Tajmar 2007 measurement]] found a signal &amp;#039;&amp;#039;&amp;#039;28 orders of magnitude&amp;#039;&amp;#039;&amp;#039; larger than GR would predict for the rotating-superconductor case — consistent with strong ψ-coupling inside the condensate.&lt;br /&gt;
&lt;br /&gt;
This is one of the most striking empirical hints in modern physics — but it is not yet conclusively confirmed across multiple labs. See [[Famous_Experiments]] and [[Open_Questions_in_Psionics]].&lt;br /&gt;
&lt;br /&gt;
== A brief history ==&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;1918&amp;#039;&amp;#039;&amp;#039; — Josef Lense and Hans Thirring derive the rotating-mass frame-dragging effect from Einstein&amp;#039;s GR.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;1959&amp;#039;&amp;#039;&amp;#039; — Leonard Schiff at Stanford proposes a satellite-based gyroscope test.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;1976&amp;#039;&amp;#039;&amp;#039; — LAGEOS satellite launched; later used for indirect frame-dragging measurements.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;2004&amp;#039;&amp;#039;&amp;#039; — [[Gravity_Probe_B]] launched.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;2011&amp;#039;&amp;#039;&amp;#039; — GP-B publishes the direct confirmation.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;2007–present&amp;#039;&amp;#039;&amp;#039; — [[Tajmar_Experiments|Tajmar&amp;#039;s rotating-superconductor experiments]] suggest very large frame-dragging-like signals; status remains contested.&lt;br /&gt;
&lt;br /&gt;
== Where to go next ==&lt;br /&gt;
&lt;br /&gt;
* For the math: [[Lense-Thirring_Frame_Dragging]] → [[Gravitoelectromagnetism]].&lt;br /&gt;
* For the experimental confirmation: [[Gravity_Probe_B]].&lt;br /&gt;
* For the anomalous superconductor case: [[Gravitomagnetic_London_Moment]]; [[Tajmar_Experiments]].&lt;br /&gt;
* For the ψ-coupling: [[Modified_Einstein_Equations_with_Psi]].&lt;br /&gt;
&lt;br /&gt;
== See Also ==&lt;br /&gt;
&lt;br /&gt;
* [[Lense-Thirring_Frame_Dragging]]&lt;br /&gt;
* [[Gravity_Probe_B]]&lt;br /&gt;
* [[Gravitoelectromagnetism]]&lt;br /&gt;
* [[Famous_Experiments]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Psionics]]&lt;br /&gt;
[[Category:Plain language]]&lt;br /&gt;
[[Category:Gravity]]&lt;/div&gt;</summary>
		<author><name>JonoThora</name></author>
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