EARLY UNIVERSE SIMULATION

Every atom in your body is what survived an annihilation: for roughly a billion matter-antimatter pairs that wiped each other out, about one matter particle was left over, and the entire material universe is built from that sliver. Earlier still, at 10⁻¹² seconds the four fundamental forces finally parted ways; at 10⁻⁶ seconds quarks lost their freedom and locked into protons and neutrons. Nuclear reactions shut down three minutes after the Big Bang, while light stayed trapped for another 380,000 years before escaping as the microwave background.

▸ Loading the Planck clock (10⁻⁴³ s)…
▸ Initializing the expanding spacetime grid
▸ Calibrating the thermometer (~10³² K → 2.725 K)
▸ Loading the quark–gluon soup & 4 fundamental forces
▸ Building H/He nucleosynthesis (~75/25)
▸ Ready — Online. ✅
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Simulation room The early universe

The First Three Minutes
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inflation · 4 forces · quarks · CMB
Cosmic thermometer
🌡️ Cooling over time
Age of the universe—
Temperature—
Now forming—
H : He ratio—
Forces separated—
Viewing—
Notes
The universe was hot & dense at its birth then expanded & cooled. As it cools, the forces split, particles gradually combine: quarks → protons/neutrons → H, He nuclei → neutral atoms → light escapes (CMB).
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Temperature & Helium fraction vs log(time) temperatureHe fraction
About Big Bang

Every atom in your body is what survived an annihilation: for roughly a billion matter-antimatter pairs that wiped each other out, about one matter particle was left over, and the entire material universe is built from that sliver. Earlier still, at 10⁻¹² seconds the four fundamental forces finally parted ways; at 10⁻⁶ seconds quarks lost their freedom and locked into protons and neutrons. Nuclear reactions shut down three minutes after the Big Bang, while light stayed trapped for another 380,000 years before escaping as the microwave background.

Related topics in Cosmic Timeline