Demography of galactic technosignatures

TL;DR

This paper develops a new framework for estimating the number and distribution of extraterrestrial technosignatures in the Milky Way, considering different emission types and their detectability, extending beyond traditional Drake equation metrics.

Contribution

It introduces new indicators for galactic technosignature demography, accounting for emission directionality and longevity, providing formulas to estimate their prevalence and observability.

Findings

$ar{k}$ equals $N_D$ for isotropic emissions

Highly directional signals have $ar{k}$ much smaller than $N_D$

$N_G$ depends on emission rate and longevity, unlike $N_D$ and $ar{k}$

Abstract

Probabilistic arguments about the existence of technological life beyond Earth traditionally refer to the Drake equation to draw possible estimates of the number of technologically advanced civilizations releasing, either intentionally or not, electromagnetic emissions in the Milky Way. Here, we introduce other indicators than Drake's number $N_D$ to develop a demography of artificial emissions populating the Galaxy. We focus on three main categories of statistically independent signals (isotropic, narrow beams, and rotating beacons) to calculate the average number $N_G$ of emission processes present in the Galaxy and the average number of them crossing Earth, $\bar{k}$, which is a quantity amenable to statistical estimation from direct observations. We show that $\bar{k}$ coincides with $N_D$ only for isotropic emissions, while $\bar{k}$ can be orders of magnitude smaller than $N_D$ in the case of highly directional signals. We further show that while $N_D$ gives the number of emissions being released at the present time, $N_G$ considers also the signals from no longer active emitters but whose emissions still occupy the Galaxy. We find that as long as the average longevity of the emissions is shorter than about $10^5$ yr, $N_G$ is fully determined by the rate of emissions alone, in contrast to $N_D$ and $\bar{k}$ which depend also on the emission longevity. Finally, using analytic formulas of $N_G$, $N_D$, and $\bar{k}$ determined for each type of emission processes here considered, we provide a comprehensive overview of the values these quantities can possibly achieve as functions of the emission birthrates, longevities, and directionality.