FINE-TUNING OF COSMIC CONSTANTS

Strengthen the strong nuclear force by a few per cent and hydrogen burns to helium right after the Big Bang, leaving a universe with no water. Several other constants sit in similarly narrow bands, the strangest being the cosmological constant: the observed value is smaller than the quantum estimate by something like a factor of 10¹²⁰. That is where the measurable part stops. Three competing responses — a multiverse of differing constants, anthropic selection, and a deeper theory that fixes the values — are so far indistinguishable by any experiment, and none of them requires the notion of design.

▸ Loading the fundamental constants (Λ, strong force, gravity, α)…
▸ A NARROW band allows stars, atoms, chemistry
▸ A small tweak → a barren universe
▸ Solutions: multiverse · anthropic · deeper theory (open)…
▸ Online. ✅
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Simulation room Fine-tuning of cosmic constants

Fine-Tuning
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🎚️ ? open question
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🎚️ Outcome
Constant—
Universe outcome—
Life-friendly?—
Scenario—
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Drag the constant value: stray from the narrow middle band → a barren universe · pick a constant / solution on the right
Constant value sweeping through the life-friendly bandsweep
About Fine-Tuning

Strengthen the strong nuclear force by a few per cent and hydrogen burns to helium right after the Big Bang, leaving a universe with no water. Several other constants sit in similarly narrow bands, the strangest being the cosmological constant: the observed value is smaller than the quantum estimate by something like a factor of 10¹²⁰. That is where the measurable part stops. Three competing responses — a multiverse of differing constants, anthropic selection, and a deeper theory that fixes the values — are so far indistinguishable by any experiment, and none of them requires the notion of design.

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