The Spacetime Metric
Part IV · Mass, Inertia and Gravity

Gravity Control and Superconductors

Frame-dragging is measured — and Ning Li, Podkletnov and Tajmar are the programmes trying to make it big enough to use.

15 min read·gravitomagnetism · Ning Li · Podkletnov · Tajmar · Gravity Probe B

Superconductors are where people go looking for gravity control, and the instinct is good. A superconductor is the largest piece of coherent quantum matter you can hold in your hand. This chapter teaches three things: the real gravity effect relativity predicts, the programmes trying to amplify it, and what the measurements tell the next experiment to do.

Before any of that, watch the effect itself. Press play and watch what appears around the disc as it spins up: it is spacetime being dragged along with the mass. It is real, it is measured — and it is far too small to use. Closing that gap is what the rest of this chapter is about.

Before you move anything — what do you expect?

Optional, and there is no score. The instrument below works exactly the same whether you answer or not.

The scene below models what a spinning mass does to the spacetime around it. How do you expect that effect to be drawn?
A spinning superconducting disc winding up precessing rings of gravitomagnetic field around it.
Frame-dragging, modelled: a spinning mass winds spacetime slightly around with it, drawn as precessing field rings around a rotating disc. The effect is real and measured; making it large is the open problem. (Interactive 3D; degrades to the poster.)

The real effect: gravitomagnetism

Einstein's general relativity, in its weak-field form, says gravity has a "magnetic" side. A spinning mass drags spacetime slightly around with it. The effect is called gravitomagnetism, or frame-dragging. The formal name is gravitoelectromagnetism, GEM. None of this is fringe. It is textbook relativity, and it was measured. NASA's Gravity Probe B published results in 2011. It found Earth's frame-dragging at the size relativity predicts.

That is the winding you just watched, and here it is written down — with the factor that makes it so small in plain sight.

A gravitomagnetic field equation (GEM)(11.1)
∇×Bg  =  −16πGc2 j  +  1c2∂Eg∂t\nabla \times \mathbf{B}_g \;=\; -\dfrac{16\pi G}{c^2}\,\mathbf{j} \;+\; \dfrac{1}{c^2}\dfrac{\partial \mathbf{E}_g}{\partial t}
What this says
Written this way, gravity looks almost exactly like electromagnetism. Moving mass — the current j — makes a 'gravitomagnetic' field B_g. Moving charge makes a magnetic field the same way. This is real, confirmed physics. The catch is size. The 1/c² makes the field around a lab-scale spinning object tiny. It is about a hundred billion billion times weaker than a useful gravity effect needs. Closing that gap is the whole game. It is why every programme here reaches for coherent quantum matter.

Gravitomagnetism is real weak-field relativity, and frame-dragging is measured (Gravity Probe B, LAGEOS). It is also minuscule. That number is the yardstick for everything that follows.

The programmes: amplifying it with coherent matter

In the early 1990s Ning Li and Douglas Torr made a proposal with a mechanism. Inside a superconductor, they argued, the coherent spin of the lattice ions could amplify the gravitomagnetic field to useful levels. They called it "AC gravity."

Around the same time Eugene Podkletnov reported something more direct. Objects hung above a large, spinning YBCO superconductor seemed to lose a little weight. He called it gravitational shielding. He later described an "impulse gravity generator" that fired a force beam, using a high-voltage discharge through a superconductor.

A test mass hanging on a balance above a large spinning YBCO superconductor disc, with claimed weight loss marked.
Podkletnov's reported setup: a test mass suspended over a large rotating superconductor disc — the apparatus this whole thread is built around. (Precise vector schematic.)

What the measurements say

Three independent groups have run the weight-loss experiment. Woods, Helme, Cooke and Caldwell (2001) measured no change. Hathaway, Cleveland and Bao (2003) built a well-instrumented rig and measured no change either. NASA-funded evaluations at Marshall did not confirm an effect. The 1997 Podkletnov preprint was withdrawn; the peer-reviewed footprint is the 1992 Physica C paper.

Those runs are not the end of the thread. They are its specification. They fix the size any real effect has to beat. They also raise the obvious question: what did the different runs do differently? A 2026 stream put a specific answer on the table. Perhaps what matters is how fast the disc is spun up, not the speed it finally reaches. That turns a disagreement between laboratories into a number you can scan.

Spin-up, not spin

Thirty years of rotating-superconductor experiments varied one thing: how fast the disc finally turned. Nobody varied how fast it got there. Set the two independently — the angular acceleration of the ramp, and the steady rate at the end of it — and the ledger below says which published runs would have seen an effect that depends on the rate, and which would have been blind to one that depends on the ramp.

Spin-up, not spin
The ramp the reader sets, and the two candidate response laws drawn against itTwo panels. On the left, the rotation of the disc against time: a straight ramp whose slope is the angular acceleration you set, levelling off at the steady rate you set, with the balance reading marked both during the ramp and at the plateau. On the right, the two candidate laws side by side as bars against the same scale of weight change, with the range Podkletnov reported drawn as a band across both and the bound the Toronto rebuild published drawn as a line.
  • The range reported in 1992
  • The bound published in 2003
The two curves are models, not predictions from any paper. Each is anchored to the same published number — the largest weight change reported in 1992 — reached at the condition the original called for, and each rises in a straight line to it. They exist so that two hypotheses can be held against the same four runs, which is what has never been done.Nothing here moves on its own. The drawing changes only when you move a slider.
If it depends on the rate:
0.055 %
If it depends on the spin-up:
0.011 %
Time to reach that rate:
4.8 s

At this setting: A balance read only at the plateau is read at zero angular acceleration. Against a law of that kind such a run is not a null; it is blind, and its bound is a bound against the rate and nothing else. That is the whole argument: a bound constrains only the parameter that was varied.

What each published run would have seen

The runs, each on its own sheetIf the effect depends on the rateIf it depends on the spin-up
Podkletnov and Nieminen, 1992 — a 5.48-gram sample over a 14.5-centimetre YBCO disc, losing between 0.05 and about 0.3 per cent of its weight, varying with how fast the disc turned, with the original calling for several thousand revolutions per minutepublished no numerical bound, so it constrains neitherblind to it — the balance was read at the plateau, where the angular acceleration is zero
Woods, Helme, Cooke and Caldwell, 2001 — a careful null that states its own scope: the internal structure of the disc and the levitating and rotating system both fell short of the specified conditions, so what is published is a bound rather than a verdictpublished no numerical bound, so it constrains neitherblind to it — the balance was read at the plateau, where the angular acceleration is zero
Hathaway, Cleveland and Bao, 2003 — the most careful rebuild, with a disc the original author judged fit, seeing no weight change at the 0.001 per cent level; the disc never turned faster than 550 revolutions per minutewould have seen itblind to it — the balance was read at the plateau, where the angular acceleration is zero
Tajmar and colleagues, 2007 — a niobium ring in liquid helium read by a mirrored curl configuration of accelerometers plus laser gyroscopes, which corrected its own earlier figure downward and asked other laboratories to try; its accelerometers read acceleration while its gyroscopes read rotation ratepublished no numerical bound, so it constrains neitherpublished no numerical bound, so it constrains neither

The original claim is peer-reviewed, the published replications are nulls that name the conditions they did not reach, and the acceleration-rate hypothesis is a stated, testable refinement with no data either way. The settling measurement is the fractional weight change of the test mass plotted against angular acceleration at fixed final angular velocity, with the ramp reversed and with a non-superconducting disc of matched mass and moment of inertia as the control. If nothing appears, the bound is published against a parameter nobody had bounded, which is itself a real contribution.

Three steps down a rail: a reported anomaly, the group's own harder test of it, and the bound that survived.
The Tajmar arc: a small early signal that shrank as the shielding and controls improved. The bound it left behind is the number the next experiment has to beat.

The most instructive story is Martin Tajmar's. His 2006–07 experiments reported a small anomalous "gravitomagnetic London moment" around spinning superconductors. It was genuinely exciting. He did the right thing with it and improved his own controls. By 2007 his group was already setting its own numbers against Gravity Probe B, and reporting that the comparison ruled out every published model of the effect — their own earlier Cooper-pair hypothesis by five orders of magnitude. In better-shielded runs from 2009 to 2011 the signal shrank into the noise, and he published that. That is the field's roadmap, not a retreat. His bound is now the number a real effect has to clear.

Open question: does the spin-up rate set the size of the effect? What to watch next: a run that states its ramp rate in advance, and its predicted weight change, on a shielded balance.

Published measurements of superconductor gravity modification disagree. Comparing apparatus, shielding and operating conditions is necessary to identify the cause.

The objection · Woods 2001 / Hathaway 2003 / Tajmar's own later work

“Every careful independent attempt to replicate superconductor gravity modification has come back at or near zero, including the proponent's own better-controlled runs.”

The answer

That is a fair summary of the measurements, and this chapter reports them as they stand. Start with what is certain underneath. Gravitomagnetism is real, and Gravity Probe B watched Earth drag spacetime around by exactly the amount relativity predicts. So the question is never whether the effect exists. It is whether coherent matter can make it big enough to notice. The runs that came back at zero give that question a number to beat, and the tightest number in that comparison is Gravity Probe B's, which is the yardstick his group set every published model against — their own earlier one included. Two live variables are now on the table: the rate at which the disc is spun up, and, in the nuclear-spin line, the sample temperature that Stark, Grafe and Tajmar's 2024 test showed can imitate a weight change. Watch for a run that states its ramp rate and predicted effect size in advance. That is the experiment this chapter is waiting for.

What the field added — July to September 2026

Three gravity-control threads came back. One new result joined the chapter from an unexpected direction.

Mark Sokol presented Frederick Alzofon's 1981 idea. Polarise the nuclear spins in a sample, Alzofon said, and its weight should change. Sokol described his lab's work on it. The idea now has a modern test on record. Stark, Grafe and Tajmar ran it in 2024 with an NMR machine. They found that temperature is the thing the next experiment must control. A stream proposed a new variable for the spinning-superconductor effect: how fast the spin is ramped up, not the final speed. That turns a dispute between labs into a number to scan. Archival interviews with McDonnell Douglas engineers Robert Wood and Paul Czysz added a real 1968 memo proposing gravity experiments. A major aerospace company funded this line of thought sixty years ago.

The new result is the NbSe₂ cavity paper in Chapter 2. Reshape the vacuum around a superconductor and its critical temperature rises. That is a different quantity than weight. But it is the same family of physics this chapter is about, and it is peer-reviewed. Laithwaite's 1974 spinning-disk lift made a good classroom demonstration of how gyroscopes behave. Research log. Phase and coherence — the thread joining the London moment, flux quantisation and the junction arrays — have their own course: quantum phase and coherence. For the junction physics itself — the two Josephson relations, SQUIDs, qubits and junction arrays — take the Josephson-junction drill-down course.

The gaser: build the emitter, instead of amplifying the field

Every programme in this chapter so far tries to make a superconductor change the weight of something near it. There is a second way to spend the same coherence, and in January 2026 it arrived as a finished engineering proposal. Gary Stephenson, an engineer at Seculine Consulting, published "Stimulated Emission of Gravitational Waves via Dissimilar Superconducting Josephson Junctions" in the Journal of High Energy Physics, Gravitation and Cosmology. His device is a gaser — the gravitational counterpart of a laser. It does not nudge gravity. It radiates it: a wafer that makes gravitational waves on a laboratory bench, instead of waiting for two black holes to collide. Chapters 4 and 8 name it in passing. This is the chapter it belongs to, and this is where it gets built.

The lineage is three papers long. Halpern and Laurent worked out in 1964 how a quantum system radiates gravitationally, and found spontaneous graviton emission very small. Lawrence Ford returned to it in 1982 with a fully quantum treatment and found the result that makes a device possible: the radiated power goes as the square of the number of coherent emitters, and that number can be made arbitrarily large, so quantum-gravitational effects need not be confined to Planck dimensions. Giorgio Fontana turned that into a machine in 2012 — the HTSC gaser — as a bulk device, which meant fabricating bulk cuprate, among the most demanding materials anyone has tried to manufacture. Stephenson's contribution is the redesign that makes it buildable: thin films on a standard silicon wafer, laid out as a phased array.

The mechanism sits in the junction. A Josephson junction is a sandwich of two superconductors. Make the two halves deliberately unlike each other — a plain s-wave superconductor such as lead joined to a d-wave cuprate such as YBCO — and a Cooper pair crossing between those two pairing symmetries has to change its orbital angular momentum by two units. A spin-2 transition is exactly the transition that emits a graviton. In ordinary materials those s-to-d transitions are drowned out by far more probable electric and magnetic ones; Cooper pairs in a cuprate have nowhere else to go, because they support no states other than s-wave and d-wave. One junction is still a faint emitter — Fontana's figure is a graviton emission probability about 4.8 × 10⁻⁴³ of the photon's, for the same electron transition — which is why Ford's square law is the whole reason to build an array rather than a single junction.

What follows is a parts list, and that is what earns this proposal its place. The junction supplies its own oscillation through the AC Josephson effect: bias it, and it rings at a frequency the bias sets. Stephenson selects 24.048 GHz, a US amateur microwave band, because the bands below it give emitter features too large to fit an array onto a standard wafer. The Josephson relation then fixes the bias at 49.73 microvolts — not a free parameter, but the voltage that frequency demands. The wavelength there is 1.25 cm, so each emitter pad is a quarter wavelength across, 3.1 mm, and the pads sit a full wavelength apart so that every one of them emits in step. Eighty-one fit on a 150 mm silicon wafer. The films are lead over YBCO, with tantalum named as the substitute for a deposition chamber that must stay lead-free and BSCCO as the near-equivalent cuprate, and the wafer runs below 7 kelvin, set by lead's critical temperature. The estimate is about 1.5 milliwatts of gravitational-wave power per emitter, about 121.5 milliwatts from the 150 mm array, and about 193.5 milliwatts from a 200 mm wafer carrying 129 emitters.

The first experiment is self-contained, because the junctions work both ways. Reciprocity means the same junctions biased to emit can be used passively to detect, so one bench can make the signal and read it back. At a bandwidth of 10 kHz the noise equivalent power is about 600 picowatts, which puts the 150 mm array better than 83 decibels above its own noise floor. And the whole thing is meant to sit in an ordinary low-temperature cryogenic probe station of the kind that already tests quantum-computing wafers, which is the practical reason the thin-film redesign matters: the fabrication and the test rig both already exist.

This is designed, not yet built. Stephenson's conclusion says so in one line — the remaining work is for the described hardware to be built and tested — and he is equally direct about what is not yet known. The d-wave to s-wave conversion efficiency the device depends on is not well understood, and he recommends running a range of doping regimes to find the best one. Speaking about the design in July 2026 he put the remaining coupling shortfall at roughly twenty orders of magnitude, and said plainly that the device as specified generates gravitons rather than amplifying them. That candour is the point. A proposal that names its materials, its frequency, its bias voltage, its wafer, its predicted power, its detector and its own open question is a proposal a reader can check and an engineer can start — and the shortfall has a handle on it, because on the same broadcast he gave the scaling that governs it: strain rises with the square of the frequency, and radiated power with the fourth power.

What to watch: the first wafer. One array, biased to 49.73 microvolts, emitting at 24 GHz, with a second array of the same junctions listening.

A silicon wafer carrying a square grid of round thin-film emitter pads, with flat parallel sheets standing above it to show the wave leaving every pad in step, and a three-layer stack drawn to one side showing which superconductor sits on which.
Eighty-one emitters, spaced one wavelength apart so that they all emit in step — which is the whole reason to build an array, because the radiated power grows with the square of the number kept coherent. Designed, not yet built, and the author names the open problem himself: how efficiently one kind of superconductor converts into the other is not yet understood.

Two questions follow that wafer, and the axis below answers both from published figures alone. Is anything listening at 24 gigahertz? And how far short does the design still fall, by its own author's count? Switch between the two views to see where the gaser's band sits among the detectors that exist, and how many orders of magnitude separate it from being heard.

The gaser, measured against the instruments

Stephenson's wafer is specific enough to be measured, so measure it. Here is the megahertz-to-gigahertz band with the published detectors laid across it, and 24.048 gigahertz — the frequency the gaser is designed to emit at — drawn as a line through them. Then the distance the author names himself: roughly twenty orders of magnitude of coupling still to find. A zoomable scale would hide that, because above about a million readers stop reading a logarithmic axis logarithmically. So the orders are counted instead, one rung at a time, next to two distances of known size.

What to look at
The published detectors of the megahertz-to-gigahertz band, with the gaser's emission frequency drawn through them, and the shortfall its author states counted in rungsTwo views of one subject. The band view runs frequency from one megahertz to one hundred gigahertz on a logarithmic axis, one decade per step, with a horizontal bar for each published instrument at the strain figure its paper states, and a vertical line at 24.048 gigahertz where the gaser is designed to emit. The gap view is a ladder of counted rungs, one rung per order of magnitude: the gaser's published ideal case above the noise floor of its own reciprocal detector, the twenty orders of coupling its author says are still missing, where that leaves the device today, the six orders by which the whole band still falls short of the physics it is hunting, and the sixteen orders that separated a century-ago technology from the bands LIGO and LISA now cover.
  • Strain noise per root hertz
  • An upper limit already set on a background
  • The gaser
Every bar is the frequency range that paper states, at the strain figure that paper states. Nothing is interpolated between them, and no curve is drawn through a band its source does not cover.Two different rulers, on purpose. Frequency is a place, so it runs as a dial: one decade per step, left to right. The orders of magnitude are a size, and sizes above about a million stop being read logarithmically — so every order is drawn as its own counted rung and numbered, and the distance a reader sees is the distance there is.Three quantities, kept apart. Most of these figures are strain noise per root hertz, the number a running instrument quotes. ARCADE 2's is an upper limit on a stochastic background already excluded by radio data, not an instrument noise floor. The Li–Baker figure is a dimensionless monochromatic strain amplitude its authors state the design could resolve. Drawing all three as one curve is the ordinary way to get this picture wrong, so each is marked and named.
The published instruments
The gaser's emission frequency:
24.0 GHz
The published ideal case:
1.2E-1 W / 6E-10 W
The shortfall the author states:
20
Where that leaves the device today:
-11.7

Reading: A microwave cavity on ADMX parameters. 3E-22 — strain per root hertz. Its published band stops short of 24.048 gigahertz.

Berlin and colleagues show that an axion haloscope is already most of a gravitational-wave detector: an eight-tesla field, a tenth of a cubic metre of cavity, a quality factor of 100,000, one kelvin and a minute of integration reaches about 3 × 10⁻²² at a gigahertz, and a phase-sensitive matched filter takes it to about 10⁻²³. The hardware exists; what changes is what it is asked.

The published ideal case assumes nearly perfect conversion, and the author is explicit that the conversion is the open problem. Subtract the shortfall he states and the ledger closes where the drawing shows it.

This is what taking a proposal seriously looks like. A programme that names no frequency and no output cannot appear on these axes at all; the gaser can, because it names a wafer, a bias voltage, an emitter count, a predicted power, a detector and its own missing number. The distance is real, and so is the fact that it is stated rather than discovered by a critic.

Three things would move the line. The frequency scaling Stephenson gives on the same broadcast: strain rises with the square of the frequency and radiated power with the fourth, so the whole ledger moves with the band a future wafer is designed for. The coherence law the array exists for: radiated power grows with the square of the number of emitters kept in step, so 81 pads on a 150 mm wafer is the smallest version of the device, not the largest. And the conversion efficiency itself — the doping sweep across d-wave and s-wave regimes that the paper recommends as the first experiment is the measurement that would put a real number where twenty orders of magnitude currently stand.

Read the source sheets. The 100-megahertz recycling interferometerA microwave cavity on ADMX parametersARCADE 2, recastThe Li–Baker detectorThe gaser


Measurements to make next

A spin-up test should state its ramp rate and predicted weight change in advance. For the nuclear-spin proposal, use an Alzofon-style experiment with temperature controlled to determine whether a weight shift persists.

Sources

Primary - the programmes

  • G. V. Stephenson (2026), "Stimulated Emission of Gravitational Waves via Dissimilar Superconducting Josephson Junctions," J. High Energy Phys. Gravit. Cosmol. 12(1), 585-605, doi:10.4236/jhepgc.2026.121029 - the gaser, with materials, frequency, bias and a first test. Full text on the source sheet. (Open licence, CC BY 4.0.)
  • N. Li & D. Torr (1991), "Effects of a gravitomagnetic field on pure superconductors," Phys. Rev. D 43, 457; (1992) Phys. Rev. B 46, 5489 - the amplification proposal.
  • E. Podkletnov & R. Nieminen (1992), "A possibility of gravitational force shielding by bulk YBa2Cu3O7-x superconductor," Physica C 203, 441 - the peer-reviewed origin (the later 1997 preprint was withdrawn).
  • E. Podkletnov & G. Modanese (2001), "Impulse gravity generator...," arXiv:physics/0108005 / physics/0209051. Full text on the source sheet. (Downloaded.)

Real gravitomagnetism - the yardstick (beyond the source corpus)

  • B. Mashhoon (2003), "Gravitoelectromagnetism: a brief review," arXiv:gr-qc/0311030 - GEM is real weak-field relativity; the lab-scale field is ~1e-20 of the claimed effects.
  • C. Everitt et al. (2011), "Gravity Probe B: Final Results...," Phys. Rev. Lett. 106, 221101 - measured frame-dragging at its tiny predicted size.

Where the physics is worked out

Where the replication stands: the positive reports are a thin cluster, and the best-instrumented runs measured nothing. The 2026 threads answer with a variable nobody scanned - the spin-up rate - which is what makes a disputed effect testable again.