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.
arXiv comment57 pages, 1 figure, 12 tables
References in corpus (37)
- Habitable Zones Around Main-Sequence Stars: New Estimates
- The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets
- Stability Criteria for Complex Ecosystems
- Rapid planetesimal formation in turbulent circumstellar discs
- Streaming Instabilities in Protoplanetary Disks
- Evolution of the Solar Activity over Time and Effects on Planetary Atmospheres: I. High-energy Irradiances (1-1700 A)
- Understanding the Mass-Radius Relation for Sub-Neptunes: Radius as a Proxy for Composition
- Roche lobe effects on the atmospheric loss of "Hot Jupiters"
- The Effect of a Strong Stellar Flare on the Atmospheric Chemistry of an Earth-like Planet Orbiting an M dwarf
- Statistical Physics of Self-Replication
- The Galactic Habitable Zone and the Age Distribution of Complex Life in the Milky Way
- Helium in the eroding atmosphere of an exoplanet
- Vegetation's Red Edge: A Possible Spectroscopic Biosignature of Extraterrestrial Plants
- Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment
- Compositional imprints in density-distance-time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation
- How to form planetesimals from mm-sized chondrules and chondrule aggregates
- The thermodynamics of prediction
- The Galactic Habitable Zone I. Galactic Chemical Evolution
- A New Window into Escaping Exoplanet Atmospheres: 10830 Å Line of Helium
- Modeling Repeated M-dwarf Flaring at an Earth-like Planet in the Habitable Zone: I. Atmospheric Effects for an Unmagnetized Planet
- Exoplanet Biosignatures: A Framework for Their Assessment
- Autocatalytic Sets and the Growth of Complexity in an Evolutionary Model
- Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life
- Detecting Oceans on Extrasolar Planets Using the Glint Effect
- Gamma-Ray Bursts and the Earth: Exploration of Atmospheric, Biological, Climatic and Biogeochemical Effects
- On detecting biospheres from chemical thermodynamic disequilibrium in planetary atmospheres
- Cosmological variation of deuteron binding energy, strong interaction and quark masses from big bang nucleosynthesis
- Kinetic vs. energetic discrimination in biological copying
- Stellar production rates of carbon and its abundance in the universe
- 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
- Dependence of the triple-alpha process on the fundamental constants of nature
- Atmospheric Seasonality as an Exoplanet Biosignature
- How special is the Solar System?
- Direct High-Resolution Imaging of Earth-Like Exoplanets
- Fundamental Physics in 2025: Status, Decisive Targets, and Path Forward