Pulse of Civilization: The Rhythm That Determines Survival express

Original: "Projections of Earth's Technosphere: Civilization Collapse-Recovery Dynamics and Detectability"
arXiv:2604.13774 · 2026-04-15 · CC BY 4.0 · 1 min
The fate of civilization is decided not by luck, but by resource consumption.

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The fate of a civilization isn't just a matter of luck or disasters. Scientists simulated a thousand years of history under ten different scenarios, accounting for resource consumption, governance, and random shocks. The key metric turned out to be the 'activity coefficient' – the fraction of time when a civilization is technologically alive. At best, this fraction nears 100%; at worst, it drops to 38%.

Every civilization beats like a heart, swinging from feverish growth to periods of stillness. This pulse sets the rhythm of its life.

The key levers are the speed at which we deplete resources and the ability to preserve knowledge for recovery. Even a slight shift in these parameters stretches active phases over centuries. Here lies the answer to the cosmic silence: civilizations on planets around other stars (exoplanets) might spend most of their time in sleep mode. Their beacons rarely light up, and by the time a signal reaches us at the speed of light, they may have gone dark again. Radiation analysis must account for this intermittent pulse, or we risk missing even the closest voices in the galaxy. Enrico Fermi might be surprised: perhaps space isn't empty, but simply sleeping peacefully.

If the active phase takes up only 38% of the time, the chance of randomly hearing such a civilization is no higher than winning at roulette by betting on a single number.

In Isaac Asimov's 'Foundation,' mathematicians calculated the fall of the galactic empire and sought to shorten the dark ages – a task almost copied from this scientific model.

D = \frac{T_{\text{актив}}}{T_{\text{общ}}}
D is the active time fraction (from 0 to 1), T_active is the time of technological activity, T_total is the total lifespan of the civilization.
Scientists
Fritz ZwickyLudwig BoltzmannJohn von NeumannJosiah Willard GibbsSubrahmanyan ChandrasekharAdam Riess
Concepts
reliability age of the universe ecological resilience charge cycle technosignature search annual cycle seti drought climate red dwarf habitability observable universe epidemic working memory redundancy stellar age escape velocity stellar collapse mechanism earth rotation period technosignatures