Published October 26, 2026 | Version v1

The Carbon–Silicon Symbiosis Equilibrium Regularity in Closed Planetary Civilizations: A Quantitative Validation Based on Century- Scale Simulation of a Million-Settler Settlement

Authors/Creators

Description

The long-term co-evolutionary regularity of carbon-based and silicon-based intelligence

in a closed planetary system holds urgency for both Mars settlement and Earth-side AI

governance, yet existing research lacks cross-scale quantitative criteria. This study, built

on the multi-scenario empirically validated Star Project ES-V2.0 kernel, constructs a

century-scale (120-year) system-dynamics simulation of a one-million-settler settlement,

covering a 32-run matrix formed by 6 governance scenarios × 4 supply-shock levels and

1,160 Monte Carlo envelope runs. The core finding is the Carbon–Silicon Symbiosis

Equilibrium Regularity (SSE-R): the carbon–silicon collaboration ratio φ ≈ 0.60

constitutes a Pareto optimum, the only interval in the present parameter space

simultaneously satisfying the dual objectives of "long-term internal stability" and "external

expansion redundancy"; carbon-dominated regimes (φ < 0.50) exhibit, at the century

scale, production stagnation and a civilization confined to its home soil, while silicon-

dominated regimes (φ > 0.80) exhibit irreversible decay of human–machine consensus

and elevated risk of chaotic collapse. A supply shock of−25% constitutes a systemic

phase-transition inflection point, and under a strong shock (−50%) all governance paths

collapse irreversibly. Through cross-scale comparison across four scales—the voyage

segment (6 persons/9 months), thousand-settler settlement (1,000 persons/10 years),

ten-thousand-settler town (10,000 persons/60 years), and million-settler settlement

(1,000,000 persons/120 years)—the equilibrium point converges toward φ ≈ 0.60 as scale

increases, preliminarily indicating the cross-scale convergence of this regularity. This

study provides quantitative decision support for Mars settlement engineering and a time-

scale-compressed reference framework for Earth-side AI governance.

Keywords: carbon–silicon symbiosis; civilization steady state; Mars settlement; century-

scale simulation; equilibrium regularity; system dynamics

Other

碳基智能与硅基智能在封闭⾏星系统内的⻓期协同演化规律,对⽕星定居与地球 AI 治理
均具有紧迫性,但现有研究缺乏跨尺度的量化判据。本研究基于经多场景实证校验的 Star
Project ES-V2.0内核,构建百万⼈⼝聚落的百年尺度(120年)系统动⼒学仿真,涵盖 6种治理
情景×4档供给冲击共 32组算例矩阵与 1160次蒙特卡洛包络。核⼼发现为碳硅共⽣均衡规律:
碳硅协作⽐值φ≈0.60构成 Pareto 最优点,在本仿真参数空间内唯⼀同时识别出可满⾜"内部⻓
期稳定"与"外部拓展冗余"双重⽬标的区间;碳基主导(φ<0.50)在百年尺度下表现为产能停滞
与⽂明困于本⼟,硅基主导(φ>0.80)表现为⼈机共识不可逆衰减与乱世崩溃⻛险⾼企。供给
冲击-25%构成系统性相变拐点,强冲击(-50%)下所有治理路径均不可逆崩溃。通过航⾏段
(6⼈/9⽉)、千⼈定居(1000⼈/10年)、万⼈城镇(10000⼈/60年)到百万聚落(100万⼈
/120年)四个尺度的对照,均衡点随尺度增⼤向φ≈0.60收敛,初步显示该规律具有跨尺度收敛
特征。本研究为⽕星定居⼯程提供量化决策依据,并为地球 AI 治理提供时间尺度压缩下的参
照框架。
关键词:碳硅共⽣;⽂明稳态;⽕星定居;百年仿真;均衡规律;系统动⼒学

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The Carbon–Silicon Symbiosis Equilibrium Regularity in Closed Planetary Civilizations A Quantitative Validation Based on Century Scale Simulation of a Million-Settler Settlement.pdf

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Alternative title
封闭⾏星⽂明碳硅共⽣均衡规律——基于百万级聚 落百年尺度仿真的量化验证