Cosmology
Investigating the origin, evolution, fundamental structure, and ultimate fate of the entire universe.
Explore by Cosmology

May 29, 2026
Is the Universe a 3-Torus? Cosmic Topology and the Laplace–Beltrami Resolution of the CMB Low-Quadrupole Anomaly

May 28, 2026
Hubble Tension Solutions Showdown 2026: Ranking Cosmological Models

May 27, 2026
ACT DR6 vs. Starobinsky R² Inflation: Diagnosing the Horizon-Scale Tension

May 25, 2026
Missing Baryons Found: How the kSZ Effect Turned the CMB Into a Cosmic Backlight

May 24, 2026
Negative Neutrino Mass at 3σ: Resolving the DESI & ACT Lensing Anomaly

May 23, 2026
Cosmic Birefringence: The Chern-Simons Lagrangian Behind CMB Parity Violation

May 21, 2026
Primordial Non-Gaussianity and the Maldacena Consistency Relation: An EFT-of-Inflation Test

May 21, 2026
The Axis of Evil: Inside the CMB Quadrupole-Octopole Alignment

May 20, 2026
SPT-3G D1 Confirms 6.2σ Hubble Tension: A High-Resolution CMB Power Spectrum Analysis
FAQs about Cosmology
Cosmology is the scientific study of the entire universe. It asks questions about how the universe began, how it has evolved, and what its ultimate fate will be.
The Big Bang Theory is our best explanation for how the universe started. It states that the universe began as an extremely hot, dense point about 13.8 billion years ago and has been expanding and cooling ever since.
These are the two biggest mysteries in cosmology. Dark matter is an invisible substance that provides extra gravity to hold galaxies together. Dark energy is a mysterious force that is causing the expansion of the universe to accelerate.
Because light takes time to travel, looking at distant galaxies is like looking back in time. Telescopes like Hubble and James Webb allow us to see galaxies as they were billions of years ago, giving us clues about the early universe.