English

SETI's blind spot: Technological Acceleration and fleeting technosignatures

Instrumentation and Methods for Astrophysics 2026-07-08 v1

Abstract

The search for extraterrestrial intelligence (SETI) has traditionally framed the detection challenge with a focus on the parameter LL in the Drake equation - the communicative lifetime of a civilisation. I argue that the more pertinent quantity is τd\tau_d, the duration during which a civilisation produces technosignatures that are \emph{actually detectable by us, now}. Modelling technological progress as an exponential process, we show that τd=α1ln(Kmax/Kmin)\tau_d = \alpha^{-1}\ln(K_{\rm max}/K_{\rm min}), where α\alpha is the rate of technological acceleration and [Kmin,Kmax][K_{\rm min},K_{\rm max}] brackets the technology levels accessible to our instruments. As α\alpha increases, τd\tau_d can shrink to mere decades, dramatically narrowing the window in which civilisations overlap technically. This ``technology mismatch'' has implications for future search strategies, emphasising broadband and technology-agnostic approaches, as well as anomaly detection across multi-wavelength/messenger survey data.

Cite

@article{arxiv.2607.07413,
  title  = {SETI's blind spot: Technological Acceleration and fleeting technosignatures},
  author = {Michael A. Garrett},
  journal= {arXiv preprint arXiv:2607.07413},
  year   = {2026}
}

Comments

4 pages, In Advancing the Search for Technosignatures, Proceedings of IAU Symposium #404 (forthcoming)