# cosmology
Cosmology studies the universe at its largest scale and earliest moments — how it began, how it has expanded, and what invisible mass and structure hold galaxies together. This tag follows that story roughly chronologically: Big Bang Nucleosynthesis — First 20 Minutes and Primordial Nucleosynthesis — Big Bang First 3 Minutes model the first atomic nuclei forming moments after the Big Bang, CMB — Cosmic Microwave Background Power Spectrum examines the afterglow radiation left over from that early universe, and Hubble's Law — Expanding Universe demonstrates the relationship between distance and recession velocity that first revealed cosmic expansion. Further out, Galaxy Rotation Curves — Dark Matter Evidence and Dark Matter Halo present the observational case for dark matter, while Cosmic Web visualizes how matter organizes into filaments and voids across the largest scales of all.
Found: 7 simulations · 0 articles
🧪 Simulations (7)
Facts about this collection
- 7 cosmology simulations are tagged here, spanning the Big Bang through galaxy-scale structure.
- Two simulations cover the same early-universe process from different angles: Big Bang Nucleosynthesis — First 20 Minutes and Primordial Nucleosynthesis — Big Bang First 3 Minutes.
- Galaxy Rotation Curves — Dark Matter Evidence and Dark Matter Halo both address the observational evidence for dark matter.
- Cosmic Web is the largest-scale model in the set, showing how matter clusters into filaments and voids across the observable universe.
Simulations in this topic include Hubble's Law — Expanding Universe, Big Bang Nucleosynthesis — First 20 Minutes, CMB — Cosmic Microwave Background Power Spectrum, Primordial Nucleosynthesis — Big Bang First 3 Minutes, Galaxy Rotation Curves — Dark Matter Evidence and Dark Matter Halo.
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