Engineering an Interstellar Communications Network by Deploying Relay Probes

TL;DR

This paper models an interstellar communication network using relay probes with diffraction-limited photon beams, deriving a fundamental bit rate expression constrained by physics, and finds that larger optics and shorter node distances optimize the network.

Contribution

It introduces a theoretical physics-based model for interstellar relay networks, highlighting the importance of optics size and node spacing for efficient communication.

Findings

Bit rate under 1 Gbps for meter-scale probes over a light year.

Bit rate scales with the fourth power of optics size.

Optimal network involves nodes separated by sub-light-year distances.

Abstract

We develop a model for an interstellar communication network that is composed of relay nodes that transmit diffraction-limited beams of photons. We provide a multi-dimensional rationale for such a network of communication in lieu of interstellar beacons. We derive a theoretical expression for the bit rate of communication based on fundamental physics, constrained by the energy available for photons and the diffraction of the beam that dilutes the information by the inverse square law. We find that meter-scale probes are severely limited in their bit rate, under 1 Gbps, over distances of a light year. However, that bit rate is proportional to the 4th power of the size of the optics that transmit and receive the photons, and inversely proportional to the square of the distance between them, thus favoring large optics and short separations between nodes. The optimized architecture of interstellar communication consists of a network of nodes separated by sub-light-year distances and strung out between neighboring stars.