Do SETI Optimists Have a Fine-Tuning Problem?
David Kipping, Geraint Lewis

TL;DR
The paper models the population dynamics of extraterrestrial intelligences using ecological principles, revealing a fine-tuning problem for SETI optimism and connecting it to prior probability distributions like the Haldane prior.
Contribution
It introduces a novel ecological framework to analyze SETI population estimates and highlights a fine-tuning issue with optimistic assumptions about extraterrestrial life.
Findings
Occupation fraction versus birth-death ratio is S-shaped.
SETI optimism implies fine-tuning due to unbounded rates.
Prior distribution of population is bi-modal, resembling Haldane prior.
Abstract
In ecological systems, be it a petri dish or a galaxy, populations evolve from some initial value (say zero) up to a steady state equilibrium, when the mean number of births and deaths per unit time are equal. This equilibrium point is a function of the birth and death rates, as well as the carrying capacity of the ecological system itself. We show that the occupation fraction versus birth-to-death rate ratio is S-shaped, saturating at the carrying capacity for large birth-to-death rate ratios and tending to zero at the other end. We argue that our astronomical observations appear inconsistent with a cosmos saturated with ETIs, and thus SETI optimists are left presuming that the true population is somewhere along the transitional part of this S-curve. Since the birth and death rates are a-priori unbounded, we argue that this presents a fine-tuning problem. Further, we show that if the…
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Taxonomy
TopicsSpace Science and Extraterrestrial Life
