Quantitative Nonequilibrium Pathway from Fundamental Physics to the Emergence and Persistence of Exoplanetary Biospheres
arXiv:2606.02648 · doi:10.1007/s11084-026-09727-7
Abstract
We present a physics-based framework that runs from fundamental interactions and constants to biospheres, using a sequence of quantitative nonequilibrium thresholds ("gates"). Each gate is an inequality in measurable variables-free-energy flux, reaction-transport rates, replication fidelity, coding capacity, ecological closure, and climate feedback gains. Crucially, the gate vector is anchored in fundamental physics: dimensionless constants, nuclear resonance placements (e.g., the C Hoyle state), statistical mechanics (Landauer's bound ) fix the energetic, kinetic, information-theoretic margins that propagate through the gates. This anchoring lets us propagate sensitivities of the constants into biosphere-level metrics (net primary productivity (NPP), cycle-closure ratios, and climate feedback gain), yielding an end-to-end map from constants to biospheres. The framework is predictive: it yields testable inequalities, margin rankings, and population-level correlations between stellar and planetary boundary conditions and biosphere feasibility. It does not claim point predictions of life prevalence; rather, it specifies which gate margins are observable-bounded versus prior-dominated under explicitly stated chemistry/solvent families and forward models. Darwinian dynamics (heritable variation under selection) appears mid-pipeline; the end of the pipeline is a planet-scale biosphere capable of sustaining positive NPP, closing elemental cycles over geologic time. Questions of prevalence are secondary; our primary objective is to establish a constructive physics->chemistry->biology->genetics->ecosystems pipeline with testable margins and observables. As a result, we recast abiogenesis and biosphere persistence as a gate vector of falsifiable inequalities and map their margins to exoplanet observables, turning the problem into a phase diagram with explicit, testable slack.
57 pages, 1 figure, 12 tables
References in corpus (10)
- Roche lobe effects on the atmospheric loss of "Hot Jupiters"
- Vegetation's Red Edge: A Possible Spectroscopic Biosignature of Extraterrestrial Plants
- How to form planetesimals from mm-sized chondrules and chondrule aggregates
- The thermodynamics of prediction
- Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life
- Constraints on the Early Terrestrial Surface UV Environment Relevant to Prebiotic Chemistry
- On the role of GRBs on life extinction in the Universe
- A model for the emergence of the genetic code as a transition in a noisy information channel
- Direct High-Resolution Imaging of Earth-Like Exoplanets
- Fundamental Physics in 2025: Status, Decisive Targets, and Path Forward