âApplication of the Thermodynamics of Radiation to Dyson Spheres As Work Extractors and Computational Engines, and Their Observational Consequencesâ, 2023-09-12 ()â :
[Twitter] I apply the thermodynamics of radiation to Dyson spheres as machines that do work or computation, and examine their observational consequences.
I identify 4 properties of Dyson spheres that complicate typical analyses: globally, they may do no work in the usual sense; they use radiation as the source and sink of energy; they accept radiation from a limited range of solid angle; and they conserve energy flux globally.
I consider 3 kinds of activities: computation at the Landauer limit; dissipative activities, in which the energy of a sphereâs activities cascades into waste heat, as for a biosphere; and âtraditionalâ work that leaves the sphere, such as radio emission. I apply the Landsberg formalism to derive efficiency limits in all 3 cases, and show that optical circulators provide an âexistence proofâ that greatly simplifies the problem and allows the Landsberg limit to be plausibly approached.
I find that for computation and traditional work, there is little to no advantage to nesting shells (as in a âMatrioshka Brainâ [1999]); that the optimal use of mass is generally to make very small and hot Dyson spheres; that for âcompleteâ Dyson spheres we expect optical depths of several; and that in all cases the Landsberg limit corresponds to a form of the Carnot limit.
I explore how these conclusions might change in the face of complications such as the sphere having practical efficiencies below the Landsberg limit (using the endoreversible limit as an example); no use of optical circulators; and swarms of materials instead of shells.