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Pulse of Civilization: The Rhythm That Determines Survival ⚡ экспресс

Original: "Projections of Earth's Technosphere: Civilization Collapse-Recovery Dynamics and Detectability"
The fate of civilization is decided not by luck, but by resource consumption.
Abstract

A civilization is like a lighthouse with intermittent power: it flickers on and off. Scientists modeled 10 future scenarios over 1000 years and found that the key to shining long is resource conservation, not just disaster protection. Perhaps alien signals go undetected because their lighthouses are more often dim.

Links in the knowledge graph 1

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
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
galaxy exoplanet entropy spectroscopy speed of light
Laws
second law of thermodynamicsDoppler effectprinciple of constancy of the speed of lightBekenstein-Hawking entropyKepler's third lawmass–energy equivalence
Original: arXiv:2604.13774 · CC BY 4.0 · bridge42worlds