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Last update: January 12, 2026

The Incredible Precision of the Universe's Laws: Chance or Necessity?

Fine-tuning of universal constants on a cosmic control panel

The Fine-Tuning Problem in Cosmology

The fine-tuning of the universe refers to the fact that several physical constants, as well as the structure of space and the evolution of time, seem to take on very specific values and properties, without which neither stable atoms, nor stars, nor complex chemistry could exist.

Among these parameters are the gravitational constant \(G\), the fine-structure constant \(\alpha\), and the cosmological constant \(\Lambda\). Slight relative variations, sometimes on the order of < 1%, would be enough to make the universe sterile.

Table of Cosmological Constants: The Numbers That Govern Everything

"Fine-tuning" does not concern just one or two constants, but a critical set of independent parameters.

Parameters of the Universe's Fine-Tuning
ParameterValue of the constantRole in the emergence of complexitySensitivity
Gravitational constant \(G\)6.674 × 10-11 m³ kg-1 s-2Formation of stars and galaxiesVariations > 1% → sterile universe
Speed of light \(c\)≈ 299,792,458 m/sStructure of spacetime and causalityVariations → inconsistency in physics
Planck constant \(\hbar\)1.054 × 10-34 J·sDetermines the quantum scaleVariations → atomic and chemical physics impossible
Electric constant \(ε_0\)≈ 8.854 × 10-12 F/mElectrostatic force, atomic stabilityVariations ±1% → chemistry impossible
Elementary charge \(e\)1.602 × 10-19 CAtomic and chemical structureVariations ±1% → chemistry impossible
Fine-structure constant \(\alpha\)≈ 1/137Stability of atoms and moleculesVariations > 1% → chemistry impossible
Proton mass \(m_p\)≈ 1.673 × 10-27 kgNucleosynthesis and chemistryVariations ±10% → chemistry impossible
Electron mass \(m_e\)≈ 9.109 × 10-31 kgStructure of atomsVariations ±10% → chemistry impossible
Ratio \(m_p / m_e\)≈ 1836Conditions chemistry and nuclear balanceVariations ±10% → complex chemistry impossible
Mass and potential of the Higgs fieldMH ≈ 125 GeVDetermines the masses of elementary particlesVariations ±10% → universe without chemistry
Strong and weak coupling constantsαs ≈ 0.118; GF ≈ 1.166 × 10-5 GeV-2Nuclear stability and fusion reactionsVariations ±1% → unstable stars or nuclei
Neutrino masses and mixing anglesmν ≈ 0.01-0.1 eV; θ12, θ23, θ13Neutrino oscillations and cosmic nucleosynthesisVariations → affect formation of light elements
Cosmological constant \(\Lambda\)≈ 1.1 × 10-52 m-2Expansion of the universe and structure formationVariations ×10 → universe without galaxies
Primordial fluctuationsAmplitude ≈ 10-5Emergence of galaxies and structuresAmplitude ±10% → universe too homogeneous or fragmented
Baryonic density, dark matter, dark energyΩb ≈ 0.05; ΩDM ≈ 0.27; ΩΛ ≈ 0.68Formation of galaxies and cosmic dynamicsVariations ±50% → universe without complex structures
Initial conditions of nucleosynthesisAbundances: H ≈ 75%, He ≈ 25%Sets the abundance of light elementsVariations → absence of oxygen or carbon
Number of spatial dimensions3Ensures stability of orbits and gravitational laws≠3 → universe incompatible with stable structures
Metric signature of spacetime+ − − −Guarantees causality and arrow of timeInadequate → impossibility of coherent chronology
Stability of the quantum vacuumΔVvac ≈ 0Ensures long-term coherence of the universeUnstable → catastrophic collapse or expansion

Sources: arXiv.org, CERN Document Server.

The Three Great Interpretations: Chance, Necessity, or Multiverse?

The incredible precision of the fundamental constants cannot be left without explanation. If this precision were that of a watch, we would seek the watchmaker. For the universe, physicists and philosophers have formulated three major possible answers, radically different. Each of them, if true, would revolutionize our conception of reality, causality, and our place in the cosmos.

The Design Hypothesis (or Teleological Argument)

This is the oldest interpretation. Fine-tuning would be proof of intention, of a "Designer" who specifically chose the laws allowing the emergence of life and consciousness. This view, defended by some theologians and philosophers, falls outside the scientific method but answers the question of "why" in a metaphysical way. For its detractors, it simply shifts the mystery one step further (who tuned the tuner?).

N.B.:
A teleological argument is reasoning that seeks to explain a phenomenon by its purpose, goal, or "objective," rather than by its material or mechanical causes. The word comes from the Greek telos, meaning "end" or "purpose."

The Necessity Hypothesis (or Theory of Everything)

Supported by physicists and mathematicians such as Albert Einstein (1879-1955), who believed that "God does not play dice," this perspective argues that the fundamental constants are not free. According to this idea, a future Theory of Everything, possibly derived from string theory or an unknown mathematical formulation, could uniquely predict the observed values.

Other scientists have explored similar paths. Paul Dirac (1902-1984) studied surprising numerical relationships between constants, suggesting they could arise from fundamental constraints. Hermann Weyl (1885-1955) believed that deep mathematical symmetries would determine the constants. Paul Ehrenfest (1880-1933) showed that the stability of atoms and planetary orbits depended on the number of spatial dimensions, suggesting a geometric necessity. More recently, Steven Weinberg (1933-2021) and Max Tegmark (1967-) have studied how certain constants could be fixed by universal physical or mathematical constraints, even if a particular environment allows some variation.

In this framework, there would be no "fine-tuning," simply one possible physics, where the values we observe emerge from fundamental constraints rather than chance. This elegant solution remains to be discovered.

The Multiverse Hypothesis (or Selected Chance)

This is currently the most discussed explanation in the scientific community. It proposes that our universe is just one bubble among an infinity of others in a "multiverse," each with its own set of physical laws and constants. In this immensity, by pure law of large numbers, some universes are, by chance, fine-tuned for life. We inevitably find ourselves in one of them, because it is the only condition where observers can exist to ask the question. This idea is supported by certain interpretations of quantum mechanics and eternal cosmic inflation.

N.B.:
The multiverse hypothesis proposes that our universe is just one among a multitude. In this framework, the fundamental constants could vary from one universe to another. The fine-tuning observed in our universe would then be interpreted as a selection effect: only universes whose constants allow the existence of complex structures and observers would be effectively "observable." This idea is explored in the context of inflationary theories, string cosmology, and certain quantum models.

The Anthropic Principle: An Answer or a Tautology?

The anthropic principle is often seen as a tautology that explains nothing: we observe a universe compatible with our existence because we exist to observe it. However, within the framework of the multiverse hypothesis, it becomes a mechanism of observer selection: among all possible universes, only those whose constants allow the appearance of life can be observed. It does not change the constants, but explains why we observe a universe conducive to our existence.

Is the Next Copernican Revolution Cosmological?

The question "Chance or Necessity?" goes far beyond the framework of astrophysics. It touches on the philosophy of science, metaphysics, and our place in the cosmos. If the multiverse hypothesis were to be corroborated by indirect evidence (such as a particular signature in the cosmic microwave background), it would represent a Copernican revolution as great as the decentering of the Earth or our galaxy: we would not only be in a banal universe, but in one among countless others.

Conversely, the discovery of a fundamental theory that would necessarily deduce our constants would fulfill Einstein's dream of a comprehensible and deterministic universe in its ultimate laws. In the meantime, fine-tuning remains one of the deepest mysteries of contemporary science, a permanent invitation to push the boundaries of knowledge.

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