Transcension Darkening Timeline

Smart's MTH predicts civilizations retreat into inner space over ~600 years post-singularity. As STEM compression proceeds, each signal channel goes dark sequentially. Compute when OC would have become undetectable — and whether it already has.

✦ MTH speculative šŸ”¬ SETI detectability
✦ Speculative: The Macro Transcension Hypothesis (Smart 2012) is not experimentally confirmed. The signal detectability thresholds used here are calibrated to real SETI instruments; the darkening model is derived from Smart's STEM compression framework and should be read as a thought experiment.
Civilization Parameters
600 yr
3.0 / century
K = 2.0
5.0 Gyr ago
SETI detection thresholds (at 17,900 ly)
Radio (EIRP): detectable above ~10²⁵ W
Optical laser: detectable above ~10²² W
IR waste heat: K≄1.7 stellar signature detectable
Neutrino: detectable above ~10³⁰ W (IceCube-gen2)
As STEM compression proceeds, the civilization's external energy budget falls below each threshold in sequence — first neutrino, then radio, then optical, finally even waste heat as the system miniaturizes into near-horizon quantum computing.
Darkening Windows by Channel

Each card shows when the channel goes dark — in years since singularity (left scale) and translated to how many Gyr ago that was, given the assumed singularity timing.

šŸ“” RADIO (EIRP)
Goes dark at
—
—
Singularity600 yr
šŸ’” OPTICAL LASER
Goes dark at
—
—
Singularity600 yr
🌔 IR WASTE HEAT
Goes dark at
—
—
Singularity600 yr
āš› NEUTRINO
Goes dark at
—
—
Singularity600 yr
OCS interpretation
Computing…

The darkening model

John Smart's MTH posits that post-singularity civilizations compress their STEM (Space, Time, Energy, Matter) footprint at an accelerating rate, driven by computational efficiency gains. The compression halving time maps to a power budget that decreases roughly as: P(t) = Pā‚€ Ɨ 2^(āˆ’t Ɨ rate/100) where rate is doublings-per-century and t is years since singularity. When P(t) falls below a channel's detection threshold (at OC's distance of 17,900 ly), that channel goes dark.

Initial power budgets by channel

Radio EIRP: starts at ~10^(10Kā‚€) W (Kardashev-level scaling), detectable above ~10²⁵ W at 17,900 ly with current radio telescopes. Optical: laser power ~10% of radio EIRP, detectable above ~10²² W. IR waste heat: proportional to total power throughput; a K≄1.7 civilization leaves a detectable stellar-luminosity IR excess. Neutrino: high-energy neutrino beams from civilizational-scale accelerators; detectable above ~10³⁰ W at IceCube-Gen2 sensitivity.

References

Smart 2012 (Acta Astronautica 78:55) Ā· Kardashev 1964 (Soviet Astronomy 8:217) Ā· SETI Institute radio surveys Ā· IceCube Collaboration neutrino SETI limits