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	<id>https://wiki.fusiongirl.app:443/index.php?action=history&amp;feed=atom&amp;title=Tate_Experiment</id>
	<title>Tate Experiment - Revision history</title>
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		<title>JonoThora: Create Tate Experiment — Cooper pair mass anomaly (84 ppm), London moment measurement, competing interpretations, Magneto Speeder connection</title>
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		<updated>2026-03-14T06:00:11Z</updated>

		<summary type="html">&lt;p&gt;Create Tate Experiment — Cooper pair mass anomaly (84 ppm), London moment measurement, competing interpretations, Magneto Speeder connection&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Infobox&lt;br /&gt;
| title      = Tate Experiment&lt;br /&gt;
| image      =&lt;br /&gt;
| caption    = Precision measurement of Cooper pair mass via London moment&lt;br /&gt;
| header1    = Overview&lt;br /&gt;
| label2     = Principal Investigator&lt;br /&gt;
| data2      = Janet L. Tate (Stanford University)&lt;br /&gt;
| label3     = Supervisor&lt;br /&gt;
| data3      = Blas Cabrera&lt;br /&gt;
| label4     = Year&lt;br /&gt;
| data4      = 1989–1990&lt;br /&gt;
| label5     = Method&lt;br /&gt;
| data5      = SQUID measurement of London moment in spinning Nb&lt;br /&gt;
| label6     = Key Result&lt;br /&gt;
| data6      = Cooper pair mass excess: δ ≈ 8.4 × 10⁻⁵ (84 ppm)&lt;br /&gt;
| label7     = Publication&lt;br /&gt;
| data7      = Physical Review Letters 62, 845 (1989)&lt;br /&gt;
| label8     = Status&lt;br /&gt;
| data8      = Experimentally confirmed · Interpretation disputed&lt;br /&gt;
| below      = &amp;#039;&amp;#039;Only experimental anomaly supporting [[Ning Li|Li-Torr]] gravitomagnetic theory&amp;#039;&amp;#039;&lt;br /&gt;
}}&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+&lt;br /&gt;
| ⚡️ || [[Electrogravitics]] - [[Electrogravitic Tech]] || [[Electrokinetics]] - [[Electrokinetic Tech]]&lt;br /&gt;
|-&lt;br /&gt;
| 🧲 || [[Magnetogravitics]] - [[Magnetogravitic Tech]] || [[Magnetokinetics]] - [[Magnetokinetic Tech]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &amp;#039;&amp;#039;&amp;#039;Tate experiment&amp;#039;&amp;#039;&amp;#039; (1989–1990) was a precision measurement of the &amp;#039;&amp;#039;&amp;#039;Cooper pair mass&amp;#039;&amp;#039;&amp;#039; in a spinning niobium superconductor at Stanford University. By measuring the London moment — the magnetic field generated by a rotating superconductor — with SQUID magnetometers, Tate et al. determined the effective mass of the Cooper pairs with extraordinary precision and found a &amp;#039;&amp;#039;&amp;#039;statistically significant excess&amp;#039;&amp;#039;&amp;#039; of approximately 84 parts per million above the expected value of twice the electron mass.&lt;br /&gt;
&lt;br /&gt;
This anomaly is the &amp;#039;&amp;#039;&amp;#039;single most important experimental data point&amp;#039;&amp;#039;&amp;#039; in the gravitomagnetic superconductor debate. [[Ning Li]] interpreted the excess as evidence of gravitomagnetic coupling between the lattice ions and the Cooper pairs — the key prediction of the [[Gravitomagnetic London Moment]] theory.&lt;br /&gt;
&lt;br /&gt;
== Background: The London Moment ==&lt;br /&gt;
&lt;br /&gt;
When a superconductor rotates, the Cooper pairs (which carry the supercurrent) cannot rotate with the lattice. This creates a charge imbalance that generates a magnetic field aligned with the rotation axis — the &amp;#039;&amp;#039;&amp;#039;London moment&amp;#039;&amp;#039;&amp;#039;: &amp;lt;ref&amp;gt;London, F. (1950). &amp;#039;&amp;#039;Superfluids&amp;#039;&amp;#039;, Vol. 1. Wiley, New York.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\vec{B}_L = -\frac{2m_e}{e}\vec{\omega}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;m_e&amp;lt;/math&amp;gt; is the electron mass, &amp;lt;math&amp;gt;e&amp;lt;/math&amp;gt; is the electron charge, and &amp;lt;math&amp;gt;\vec{\omega}&amp;lt;/math&amp;gt; is the angular velocity. The coefficient &amp;lt;math&amp;gt;2m_e/e&amp;lt;/math&amp;gt; is universal for any superconductor — it depends only on the electron mass and charge, not on the material.&lt;br /&gt;
&lt;br /&gt;
More precisely, the London moment measures the &amp;#039;&amp;#039;&amp;#039;effective mass of the Cooper pair&amp;#039;&amp;#039;&amp;#039;:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\vec{B}_L = -\frac{m^*}{e^*}\vec{\omega}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;m^* = 2m_e(1 + \delta)&amp;lt;/math&amp;gt; is the Cooper pair mass and &amp;lt;math&amp;gt;e^* = 2e&amp;lt;/math&amp;gt; is the Cooper pair charge. Any deviation &amp;lt;math&amp;gt;\delta \neq 0&amp;lt;/math&amp;gt; would indicate physics beyond the standard London theory.&lt;br /&gt;
&lt;br /&gt;
== Experimental Setup ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Tate Experiment Parameters&lt;br /&gt;
|-&lt;br /&gt;
! Component !! Specification&lt;br /&gt;
|-&lt;br /&gt;
| Sample || Niobium (Nb) superconducting cylinder&lt;br /&gt;
|-&lt;br /&gt;
| Temperature || ~4.2 K (liquid helium)&lt;br /&gt;
|-&lt;br /&gt;
| Rotation speeds || Various (up to ~100 rad/s)&lt;br /&gt;
|-&lt;br /&gt;
| Detector || DC SQUID magnetometer (superconducting quantum interference device)&lt;br /&gt;
|-&lt;br /&gt;
| Measurement || Ratio &amp;lt;math&amp;gt;B_L/\omega&amp;lt;/math&amp;gt; to extract &amp;lt;math&amp;gt;m^*/e^*&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| Shielding || Superconducting lead shield to eliminate external magnetic fields&lt;br /&gt;
|-&lt;br /&gt;
| Calibration || Earth&amp;#039;s field, applied coils, mechanical rotation system&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The experiment measured the London moment at multiple rotation speeds and extrapolated the slope &amp;lt;math&amp;gt;dB_L/d\omega&amp;lt;/math&amp;gt; to determine &amp;lt;math&amp;gt;m^*/e^*&amp;lt;/math&amp;gt; with high precision.&lt;br /&gt;
&lt;br /&gt;
== Results ==&lt;br /&gt;
&lt;br /&gt;
=== Key Measurement ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref&amp;gt;Tate, J.L., Cabrera, B., Felch, S.B. &amp;amp; Anderson, J.T. (1989). &amp;quot;Precise determination of the Cooper-pair mass.&amp;quot; &amp;#039;&amp;#039;Physical Review Letters&amp;#039;&amp;#039; 62, 845–848. doi:10.1103/PhysRevLett.62.845&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref&amp;gt;Tate, J.L., Cabrera, B., Felch, S.B. &amp;amp; Anderson, J.T. (1990). &amp;quot;Determination of the Cooper-pair mass in niobium.&amp;quot; &amp;#039;&amp;#039;Physical Review B&amp;#039;&amp;#039; 42, 7885–7893. doi:10.1103/PhysRevB.42.7885&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;m^* = 2m_e\left(1 + (8.4 \pm 0.2) \times 10^{-5}\right)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The measured Cooper pair mass is &amp;#039;&amp;#039;&amp;#039;84 ± 2 parts per million&amp;#039;&amp;#039;&amp;#039; higher than the theoretical value of &amp;lt;math&amp;gt;2m_e&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Tate Results Summary&lt;br /&gt;
|-&lt;br /&gt;
! Quantity !! Expected !! Measured !! Deviation&lt;br /&gt;
|-&lt;br /&gt;
| Cooper pair mass &amp;lt;math&amp;gt;m^*&amp;lt;/math&amp;gt; || &amp;lt;math&amp;gt;2m_e = 1.82189 \times 10^{-30}&amp;lt;/math&amp;gt; kg || &amp;lt;math&amp;gt;2m_e(1 + 8.4 \times 10^{-5})&amp;lt;/math&amp;gt; || +84 ppm&lt;br /&gt;
|-&lt;br /&gt;
| &amp;lt;math&amp;gt;B_L/\omega&amp;lt;/math&amp;gt; ratio || &amp;lt;math&amp;gt;-1.13460 \times 10^{-11}&amp;lt;/math&amp;gt; T/(rad/s) || &amp;lt;math&amp;gt;-1.13470 \times 10^{-11}&amp;lt;/math&amp;gt; T/(rad/s) || +84 ppm&lt;br /&gt;
|-&lt;br /&gt;
| Statistical significance || — || ~42σ || &amp;#039;&amp;#039;&amp;#039;Highly significant&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The anomaly is statistically very robust (~42 standard deviations). This is &amp;#039;&amp;#039;&amp;#039;not a measurement error&amp;#039;&amp;#039;&amp;#039;.&lt;br /&gt;
&lt;br /&gt;
== Competing Interpretations ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ Interpretations of the Tate Anomaly&lt;br /&gt;
|-&lt;br /&gt;
! Interpretation !! Proponent(s) !! Mechanism !! Implication&lt;br /&gt;
|-&lt;br /&gt;
| &amp;#039;&amp;#039;&amp;#039;Gravitomagnetic coupling&amp;#039;&amp;#039;&amp;#039; || [[Ning Li]] &amp;amp; Torr (1991) || Lattice ions contribute gravitomagnetic correction to Cooper pair effective mass || Superconductors amplify gravitomagnetic fields by ~10¹¹×&lt;br /&gt;
|-&lt;br /&gt;
| Band structure effects || Various || electron-phonon interaction modifies effective mass in Nb || No exotic physics needed&lt;br /&gt;
|-&lt;br /&gt;
| Relativistic correction || Verheijen et al. (1990) || Special relativistic mass enhancement from Fermi velocity || Accounts for ~50% of anomaly&lt;br /&gt;
|-&lt;br /&gt;
| Many-body correction || Hirsch (2014) || Electron-electron interaction within Cooper pair || Predicts material-dependent mass excess&lt;br /&gt;
|-&lt;br /&gt;
| Systematic error || Skeptics || Unknown systematic in rotation calibration || Requires explaining 42σ deviation&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== The Li-Torr Interpretation (Gravitomagnetic) ===&lt;br /&gt;
[[Ning Li]] argued that when a superconductor rotates, the &amp;#039;&amp;#039;&amp;#039;lattice ions&amp;#039;&amp;#039;&amp;#039; (which carry most of the mass) generate a gravitomagnetic field through the [[Gravitomagnetic London Moment]]. This field couples to the Cooper pairs, effectively adding a gravitomagnetic contribution to their inertial mass:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\delta m = m^* - 2m_e = \frac{2G}{c^2}\cdot\rho_{\text{lattice}}\cdot V_{\text{coherence}} \cdot f(\text{coupling})&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\rho_{\text{lattice}}&amp;lt;/math&amp;gt; is the lattice mass density and &amp;lt;math&amp;gt;V_{\text{coherence}}&amp;lt;/math&amp;gt; is the coherence volume. The 84 ppm excess, in this picture, directly measures the strength of the gravitomagnetic coupling.&lt;br /&gt;
&lt;br /&gt;
=== The Conventional Interpretation ===&lt;br /&gt;
Mainstream condensed matter physics attributes the mass excess to:&lt;br /&gt;
* Band-structure (effective mass) corrections specific to niobium&lt;br /&gt;
* Relativistic corrections of order &amp;lt;math&amp;gt;(v_F/c)^2 \sim 10^{-5}&amp;lt;/math&amp;gt;&lt;br /&gt;
* Many-body interactions within the Cooper pair&lt;br /&gt;
&lt;br /&gt;
The debate has never been conclusively resolved because:&lt;br /&gt;
# The anomaly has only been measured in &amp;#039;&amp;#039;&amp;#039;niobium&amp;#039;&amp;#039;&amp;#039; — no systematic comparison across different superconducting materials has been published&lt;br /&gt;
# The predicted gravitomagnetic effect is too small to detect by any method other than the London moment (making independent verification extremely difficult)&lt;br /&gt;
&lt;br /&gt;
== Connection to Gravity Probe B ==&lt;br /&gt;
&lt;br /&gt;
[[Gravity Probe B]] also relied on the London moment of spinning niobium spheres (coated gyroscope rotors) for its readout system. GP-B calibrated its SQUID readout using the &amp;#039;&amp;#039;&amp;#039;expected&amp;#039;&amp;#039;&amp;#039; value of &amp;lt;math&amp;gt;2m_e/e&amp;lt;/math&amp;gt;. The Tate anomaly implies that GPB&amp;#039;s London moment readout carried a systematic offset of 84 ppm — small enough to be within their systematic error budget but potentially significant for ultra-precision measurements.&lt;br /&gt;
&lt;br /&gt;
This creates an interesting cross-check: GP-B confirmed gravitomagnetic frame-dragging (validating [[Gravitoelectromagnetism|GEM]]) while simultaneously relying on a readout mechanism that may itself be affected by gravitomagnetic coupling.&lt;br /&gt;
&lt;br /&gt;
== Significance for Magneto Speeder ==&lt;br /&gt;
&lt;br /&gt;
The Tate anomaly matters for the [[Magneto Speeder]] because:&lt;br /&gt;
&lt;br /&gt;
# It is &amp;#039;&amp;#039;&amp;#039;experimentally real&amp;#039;&amp;#039;&amp;#039; (42σ significance, published in Phys. Rev. Lett.)&lt;br /&gt;
# If the Li-Torr interpretation is correct, it directly measures the gravitomagnetic coupling strength in superconductors&lt;br /&gt;
# The magnitude (84 ppm) is consistent with Li-Torr&amp;#039;s predicted amplification factor&lt;br /&gt;
# It motivates the search for stronger gravitomagnetic effects in rapidly rotating superconductors — exactly what [[Martin Tajmar]] attempted&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|+ From Tate to Magneto Speeder&lt;br /&gt;
|-&lt;br /&gt;
! Link !! Connection&lt;br /&gt;
|-&lt;br /&gt;
| Tate → [[Ning Li|Li-Torr]] || Mass anomaly motivates gravitomagnetic coupling theory&lt;br /&gt;
|-&lt;br /&gt;
| Li-Torr → [[Gravitomagnetic London Moment]] || Theory predicts controllable gravitomagnetic field generation&lt;br /&gt;
|-&lt;br /&gt;
| London Moment → [[Martin Tajmar|Tajmar]] || Tajmar attempts to detect the predicted field&lt;br /&gt;
|-&lt;br /&gt;
| Tajmar → [[Magneto Speeder]] || If confirmed, provides engineering basis for magnetogravitic drive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== See Also ==&lt;br /&gt;
* [[Ning Li]]&lt;br /&gt;
* [[Gravitomagnetic London Moment]]&lt;br /&gt;
* [[Martin Tajmar]]&lt;br /&gt;
* [[Gravity Probe B]]&lt;br /&gt;
* [[Gravitoelectromagnetism]]&lt;br /&gt;
* [[Magnetogravitics]]&lt;br /&gt;
* [[Magneto Speeder]]&lt;br /&gt;
* [[Magnetogravitic Tech]]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Physics]]&lt;br /&gt;
[[Category:Technology]]&lt;br /&gt;
[[Category:Magnetogravitic Tech]]&lt;br /&gt;
[[Category:Clan Tho&amp;#039;ra]]&lt;/div&gt;</summary>
		<author><name>JonoThora</name></author>
	</entry>
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