Rebuilding the Habitable Zone from the Bottom Up with Computational Zones

Fuente: arXiv
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Autori principali: Scharf, Caleb, Witkowski, Olaf
Natura: Preprint
Pubblicazione: 2023
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author Scharf, Caleb
Witkowski, Olaf
author_facet Scharf, Caleb
Witkowski, Olaf
contents Computation, if treated as a set of physical processes that act on information represented by states of matter, encompasses biological systems, digital systems, and other constructs, and may be a fundamental measure of living systems. The opportunity for biological computation, represented in the propagation and selection-driven evolution of information-carrying organic molecular structures, has been partially characterized in terms of planetary habitable zones based on primary conditions such as temperature and the presence of liquid water. A generalization of this concept to computational zones is proposed, with constraints set by three principal characteristics: capacity (including computation rates), energy, and instantiation (or substrate, including spatial extent). Computational zones naturally combine traditional habitability factors, including those associated with biological function that incorporate the chemical milieu, constraints on nutrients and free energy, as well as element availability. Two example applications are presented by examining the fundamental thermodynamic work efficiency and Landauer limit of photon-driven biological computation on planetary surfaces and of generalized computation in stellar energy capture structures (a.k.a. Dyson structures). It is suggested that computational zones involving nested structures or substellar objects could manifest unique observational signatures as cool far-infrared emitters. While these latter scenarios are entirely hypothetical, they offer a useful, complementary, introduction to the potential universality of computational zones.
format Preprint
id arxiv_https___arxiv_org_abs_2303_16111
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Rebuilding the Habitable Zone from the Bottom Up with Computational Zones
Scharf, Caleb
Witkowski, Olaf
Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
Biological Physics
Computation, if treated as a set of physical processes that act on information represented by states of matter, encompasses biological systems, digital systems, and other constructs, and may be a fundamental measure of living systems. The opportunity for biological computation, represented in the propagation and selection-driven evolution of information-carrying organic molecular structures, has been partially characterized in terms of planetary habitable zones based on primary conditions such as temperature and the presence of liquid water. A generalization of this concept to computational zones is proposed, with constraints set by three principal characteristics: capacity (including computation rates), energy, and instantiation (or substrate, including spatial extent). Computational zones naturally combine traditional habitability factors, including those associated with biological function that incorporate the chemical milieu, constraints on nutrients and free energy, as well as element availability. Two example applications are presented by examining the fundamental thermodynamic work efficiency and Landauer limit of photon-driven biological computation on planetary surfaces and of generalized computation in stellar energy capture structures (a.k.a. Dyson structures). It is suggested that computational zones involving nested structures or substellar objects could manifest unique observational signatures as cool far-infrared emitters. While these latter scenarios are entirely hypothetical, they offer a useful, complementary, introduction to the potential universality of computational zones.
title Rebuilding the Habitable Zone from the Bottom Up with Computational Zones
topic Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
Biological Physics
url https://arxiv.org/abs/2303.16111