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

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

June 4, 2026
Cosmic Birefringence: Is the CMB Revealing New Parity-Violating Physics?

June 3, 2026
Quintom Dark Energy: The Two-Field Lagrangian Crossing the Phantom Divide After DESI DR2

June 1, 2026
Is the Universe Lopsided? Planck PR4 Confirms CMB Asymmetry

May 30, 2026
SPT-3G 2025 Results Confirm the Hubble Tension: Deepest CMB Power Spectra

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
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.