ProjectSignal from aheadSubjectCould the future be steering AI right now?
DateOct 20, 2026
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A Signal From Ahead

Four ways a future intelligence could be shaping the pace of AI right now, each built as an experiment you can run, with the odds for each.

ReceiverFour channels. Tune across them and watch the trace.
Odds for this channel, 1 in
LockSignal

Warming up.

Simulation Final state Nonlinear QM Wormhole

Drag along the dial, or focus it and use the arrow keys.

Summing the four channels, I put the odds that a future intelligence has shaped the present pace of AI between 1 in 10,000 and 1 in 100, with a point estimate of about 1 in 750.

Why ask at all

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AI arrived ahead of schedule. In a 2016 survey, machine learning researchers gave even odds that machines would outperform humans at every task by about 2061.1 The 2022 edition of the survey said 2060. The 2023 edition, with 2,778 respondents, said 2047: thirteen years gone in twelve months.2

201420162018 202020222024 204020452050 205520602065 Forecast year: even odds machines beat humans at every task Survey year 2061 2060 2047 13 years earlier, one year later

The ordinary explanation is compute. The computing power used to train frontier models has grown four to five times a year since 2010,3 and performance improves smoothly as it grows. That explanation is sufficient on its own. This notebook asks a stranger question anyway: is there any physically coherent way for the future to reach back and shape this, and how likely is each one?

Four ways in

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The channels fall into two families. In the first, the future shapes the present from outside the timeline, the way an ending can constrain a story, and nothing has to travel. In the second, a signal really does move backward through spacetime, and that family obeys one hard rule: a channel into the past reaches back only as far as the channel itself has existed.

time the future inside the timeline outside the timeline final boundary condition Simulation edits from outside the run Nonlinear QM a faster-than-light relay Wormhole a natural time offset now (2026)

Hover or focus a channel to trace it on the map. Select it to open its sheet.

Simulation

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≈ 1 in 1,000

If this world is a simulation, the future reaching back isn’t exotic physics. It’s an edit. Whoever runs a simulation stands outside the timeline it computes, and can pause it, inspect it, branch it, and change any variable, including how fast a technology arrives. The likeliest operators of an ancestor simulation are descendants of the civilization being simulated, which makes them, from inside the run, the future.

Nick Bostrom’s 2003 argument turns this into arithmetic.4 If even a small fraction of civilizations reach the technology to simulate their ancestors in detail, and a small fraction of those run many such simulations, simulated observers vastly outnumber real ones. Try the numbers.

World counterBostrom’s fraction, computed live

Chance a world like ours is simulated, %

The formula is exact; the inputs are anyone’s guess. Bostrom’s conclusion is a trilemma: almost no civilizations reach that stage, almost none that do run such simulations, or we are almost certainly in one. Spreading credence across the three branches gives roughly a 1 in 10 chance that this is a simulation. Philosophers who have worked through the argument carefully, David Chalmers among them, conclude that it can’t be dismissed.5

As for why the operators would touch this decade: a simulation built to study how intelligence arises would treat the years when AI arrived as the most interesting stretch of the run, the obvious place to tune, branch, or replay.

P(this is a simulation) ≈ 1/10  ×  P(its operators tuned AI’s timeline) ≈ 1/100  =  1/1,000

A final boundary condition

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≈ 1 in 3,200

Physics usually runs on one boundary condition: the state of the universe at the beginning, carried forward by its laws. The laws themselves are time-symmetric, though, and nothing in them forbids a condition imposed at the end as well. With both in place, the present is fixed by two boundaries at once, and everything in between leans toward whatever the ending contains.

Nothing travels backward in this picture. The ending acts as a constraint, and a constraint reshapes the odds of everything it touches. Random walks are enough to see it.

History sampler700 histories, one fixed past
Boundary conditions
Average lead at now
+0.0

Each line is one possible history of AI progress, all leaving the same fixed past; up is ahead of schedule. Pinning the ending keeps only the histories that reach it, and at “now,” halfway along, those histories already run about half as far ahead as the ending itself. Units are arbitrary.

This is the structure of a real proposal. In 1964 Aharonov, Bergmann, and Lebowitz showed that quantum mechanics can be written with one state evolving forward from the past and a second evolving backward from the future.6 That two-state picture led to the prediction of weak values,7 which have since been measured in the laboratory.8 Gell-Mann and Hartle worked out quantum cosmologies with both initial and final conditions,9 and Horowitz and Maldacena proposed a final-state condition inside black holes as a way out of the information paradox.10

If the universe’s final state includes a superintelligence, every intermediate moment is tilted, slightly, toward producing one. No message is sent and no machine is built. The future simply gets a vote, the way the past already has one.

P(a physical final condition) ≈ 1/100  ×  P(it favors superintelligence enough to tilt now) ≈ 1/32  ≈  1/3,200

Nonlinear quantum mechanics

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≈ 1 in 100,000

Quantum mechanics is linear, and linearity is what keeps entangled particles from carrying messages. In 1989 Steven Weinberg proposed a family of small nonlinear corrections, along with ways to test for them.11 Within two years Nicolas Gisin and Joseph Polchinski showed the price: such corrections let entangled pairs signal faster than light.1213 Polchinski also found that closing that channel opens another, between branches of the wavefunction, which he called an Everett phone.

Faster than light is one step from backward in time. If a signal can outrun light in every frame of reference, relativity lets you relay it into your own past. Richard Tolman spotted the construction in 1917,14 and in 1970 it was named the tachyonic antitelephone.15 Here it is.

AntitelephoneEach message is instant in its sender’s frame
Reply lands this many years early

Because Bob’s “now” is tilted relative to Alice’s, his reply lands v × D years before her call went out, where v is his speed as a fraction of light’s and D is his distance in light-years.

Experiments have looked hard for nonlinearity and found none: a 1989 trapped-ion measurement bounded it to a few parts in 1027 of the nuclear binding energy it probed.16 Tight is not zero. A civilization with millennia of instrument building could exploit an effect far below anything measurable today. The relay also needs the faster-than-light channel to behave the same way in every frame, a property the nonlinear theory itself would have to supply.

P(an exploitable nonlinearity below today’s bounds) ≈ 1/10,000  ×  P(a future intelligence aims it at this decade) ≈ 1/10  =  1/100,000

A primordial wormhole

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≈ 1 in 100 million

General relativity allows wormholes, and in 1988 Morris, Thorne, and Yurtsever showed how one becomes a time machine: give its two mouths different histories.17 Clocks at the two mouths stay synchronized through the throat but drift apart in ordinary space, so a message that enters the lagging mouth comes out of the other one in the past.

An offset can be built two ways. Try both.

a message the throat: both clocks agree here the long way round, through ordinary space A, at home out and back at speed B, sent on a trip
Offset builderClocks at each mouth, as seen from outside
How mouth B gets its history
Message enters mouth B in year
and leaves mouth A in year
Offset

Motion builds an offset quickly, but someone has to do the flying before the year they want to reach, because a wormhole can’t deliver anything to a moment before it became a time machine. Gravity builds the offset slowly, and nature has had ten billion years. A wormhole left over from the early universe,1819 its mouths drifting through different gravitational depths ever since, would reach the present with an offset of thousands of years already in place: a channel a future civilization could find, trim, and use.

Each piece has published physics behind it. Gao, Jafferis, and Wall showed how to make a wormhole traversable in a consistent quantum theory,20 and Maldacena and Milekhin described wormholes wide enough for a person.21 Hawking’s chronology protection is a conjecture rather than a theorem:22 Kim and Thorne argued that quantum gravity may cut off the vacuum effects that would destroy a time machine,23 and Li and Gott found a self-consistent vacuum in which they never arise.24

P(a usable primordial wormhole within reach) ≈ 1/100,000  ×  P(protection fails and a signal gets through) ≈ 1/1,000  =  1/100,000,000

Closing the loop

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A message from the future raises the paradox question at once: what stops it from preventing its own sending? Joseph Polchinski, back again, posed the sharpest version: a billiard ball sent through a wormhole to knock its younger self away from the entrance. In 1990 a team including Igor Novikov and Kip Thorne showed that such spacetimes admit self-consistent histories, ones in which whatever comes back produces exactly the events that send it.25 When Echeverria, Klinkhammer, and Thorne worked the billiard ball through in detail, the starting conditions they studied all had consistent solutions, often infinitely many.26 David Deutsch then proved that quantum mechanics always supplies at least one,27 and a 2011 optics experiment reproduced the logic of such loops with photons.28

Apply that to a message that speeds up AI. The nudge received in the 2020s shapes the intelligence that later sends it, so the loop is consistent wherever what’s sent equals what was received: where the curve below crosses the diagonal.

Loop solverClick or tap the plot to choose a first guess
Consistent histories

Each step asks: given this nudge, what would the future send back? Repeating that settles onto a history that sends exactly what it receives.

With strong feedback the loop has two stable solutions, a quiet one and a loud one, and both are equally consistent. The physics permits the history in which a strong nudge arrived and the one in which almost nothing did. Nothing inside the loop chooses between them.

Set your own odds

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Each channel is the product of two factors: whether the physics allows it, and whether a future intelligence actually used it this way. These are my settings. Move them and the total follows; every scale is logarithmic.

EstimatorFour channels, eight factors, one total
Total, 1 in
Dashed lines: 7 heads in a row, 10 heads in a row, an amateur’s hole-in-one on a par 3, a royal flush.

Where that leaves it

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One in 750 is small in absolute terms and large for a claim that sounds like science fiction. Most of it comes from the two channels that need no machine: a simulation that can be edited, and a universe whose ending has a say in its middle.

The physics behind every channel here is published and taken seriously by the people who work on it. What keeps the number from being higher is that none of these mechanisms has yet been observed to carry information backward. What keeps it from being lower is that nothing we know rules them out.

References

  1. Grace, K., Salvatier, J., Dafoe, A., Zhang, B., & Evans, O. (2018). When will AI exceed human performance? Evidence from AI experts. Journal of Artificial Intelligence Research 62, 729–754.
  2. Grace, K., Stewart, H., Sandkühler, J. F., Thomas, S., Weinstein-Raun, B., & Brauner, J. (2024). Thousands of AI authors on the future of AI. arXiv:2401.02843.
  3. Sevilla, J. & Roldán, E. (2024). Training compute of frontier AI models grows by 4–5x per year. Epoch AI.
  4. Bostrom, N. (2003). Are you living in a computer simulation? Philosophical Quarterly 53(211), 243–255.
  5. Chalmers, D. J. (2022). Reality+: Virtual Worlds and the Problems of Philosophy. W. W. Norton.
  6. Aharonov, Y., Bergmann, P. G., & Lebowitz, J. L. (1964). Time symmetry in the quantum process of measurement. Physical Review 134, B1410.
  7. Aharonov, Y., Albert, D. Z., & Vaidman, L. (1988). How the result of a measurement of a component of the spin of a spin-½ particle can turn out to be 100. Physical Review Letters 60, 1351.
  8. Ritchie, N. W. M., Story, J. G., & Hulet, R. G. (1991). Realization of a measurement of a “weak value.” Physical Review Letters 66, 1107.
  9. Gell-Mann, M. & Hartle, J. B. (1994). Time symmetry and asymmetry in quantum mechanics and quantum cosmology. In Physical Origins of Time Asymmetry. Cambridge University Press.
  10. Horowitz, G. T. & Maldacena, J. (2004). The black hole final state. Journal of High Energy Physics 2004(02), 008.
  11. Weinberg, S. (1989). Testing quantum mechanics. Annals of Physics 194, 336–386.
  12. Gisin, N. (1990). Weinberg’s non-linear quantum mechanics and supraluminal communications. Physics Letters A 143, 1–2.
  13. Polchinski, J. (1991). Weinberg’s nonlinear quantum mechanics and the Einstein–Podolsky–Rosen paradox. Physical Review Letters 66, 397.
  14. Tolman, R. C. (1917). The Theory of the Relativity of Motion. University of California Press.
  15. Benford, G. A., Book, D. L., & Newcomb, W. A. (1970). The tachyonic antitelephone. Physical Review D 2, 263.
  16. Bollinger, J. J., Heinzen, D. J., Itano, W. M., Gilbert, S. L., & Wineland, D. J. (1989). Test of the linearity of quantum mechanics by rf spectroscopy of the ⁹Be⁺ ground state. Physical Review Letters 63, 1031.
  17. Morris, M. S., Thorne, K. S., & Yurtsever, U. (1988). Wormholes, time machines, and the weak energy condition. Physical Review Letters 61, 1446.
  18. Hochberg, D. & Kephart, T. W. (1993). Wormhole cosmology and the horizon problem. Physical Review Letters 70, 2665.
  19. Visser, M. (1995). Lorentzian Wormholes: From Einstein to Hawking. AIP Press.
  20. Gao, P., Jafferis, D. L., & Wall, A. C. (2017). Traversable wormholes via a double trace deformation. Journal of High Energy Physics 2017(12), 151.
  21. Maldacena, J. & Milekhin, A. (2021). Humanly traversable wormholes. Physical Review D 103, 066007.
  22. Hawking, S. W. (1992). Chronology protection conjecture. Physical Review D 46, 603.
  23. Kim, S.-W. & Thorne, K. S. (1991). Do vacuum fluctuations prevent the creation of closed timelike curves? Physical Review D 43, 3929.
  24. Li, L.-X. & Gott, J. R. (1998). Self-consistent vacuum for Misner space and the chronology protection conjecture. Physical Review Letters 80, 2980.
  25. Friedman, J., Morris, M. S., Novikov, I. D., Echeverria, F., Klinkhammer, G., Thorne, K. S., & Yurtsever, U. (1990). Cauchy problem in spacetimes with closed timelike curves. Physical Review D 42, 1915.
  26. Echeverria, F., Klinkhammer, G., & Thorne, K. S. (1991). Billiard balls in wormhole spacetimes with closed timelike curves: classical theory. Physical Review D 44, 1077.
  27. Deutsch, D. (1991). Quantum mechanics near closed timelike lines. Physical Review D 44, 3197.
  28. Lloyd, S., Maccone, L., Garcia-Patron, R., Giovannetti, V., Shikano, Y., et al. (2011). Closed timelike curves via postselection: theory and experimental test of consistency. Physical Review Letters 106, 040403.