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

May 12, 2026
Simons Observatory CMB First Light: B-Mode Polarization Hunt at σ(r)=10⁻³

May 11, 2026
The Cosmic Dipole Anomaly: A Superhorizon Isocurvature Lagrangian Resolving the 5.4σ CMB-Quasar Matter Dipole Tension

May 11, 2026
Cosmic Birefringence: Chern-Simons Axions and the ACT DR6 Anomaly

May 10, 2026
Scalar Chemical Potential Cosmological Collider: A CMB Lagrangian

May 9, 2026
Fab-Four Self-Tuning Inflation: Lagrangian Origin of CMB Anisotropy

May 8, 2026
ACT DR6 Inflation Crisis: n_s = 0.9743 Excludes Starobinsky R²

May 7, 2026
Webb First Direct Exoplanet Surface Spectroscopy: LHS 3844 b Reveals Dark Airless Basaltic Super-Earth

May 5, 2026
ACT DR6 + BICEP/Keck Constraints Rule Out Major Inflation Models: The Hunt for Primordial B-Modes

May 5, 2026
ACT DR6 Cosmic Birefringence: Axion Parity Violation at β=0.215°
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.