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

June 18, 2026
Cosmic Birefringence and CMB Parity Violation: The Chern–Simons Rotation After ACT DR6

June 17, 2026
The Hubble Tension After SPT-3G: A 6.2σ Clash in Cosmology

June 16, 2026
Is the Universe Lopsided? The Cosmic Dipole Anomaly and the 5σ Failure

June 15, 2026
Is Dark Energy Constant or Evolving? ΛCDM vs. w₀wₐCDM After DESI DR2

June 14, 2026
Cosmic Topology and the 3-Torus: Signatures of a Finite Universe

June 12, 2026
Starobinsky Inflation and the ACT DR6 Spectral-Index Shift: Are Plateau Models Ruled Out?

June 11, 2026
CMB Spectral Distortions: The μ-Distortion, Silk-Damping Injection, and the ΛCDM Prediction

June 9, 2026
Axion Early Dark Energy and the Hubble Tension: Pre-Recombination Solutions

June 7, 2026
Primordial Magnetic Fields and the Hubble Tension: A 5–10 Picogauss Relic in the CMB
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.