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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Additional titles
- 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