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

July 22, 2026
Is the Cosmological Principle Broken? A Field-Theoretic Test of Cosmic Anisotropy

July 21, 2026
The Negative Neutrino Mass Problem: Reconciling DESI DR2 and CMB Lensing via Sign-Switching ΛsCDM

July 20, 2026
Is the Universe Lopsided? Tilted Bianchi Cosmology and the Khronon Field

July 19, 2026
Pinning N_eff to 2.99: How ACT, SPT & Planck Ruled Out Dark Radiation

July 18, 2026
Cosmic Strings and the CMB: A Field-Theoretic Analysis of Topological-Defect Anisotropies and the Nanohertz Gravitational-Wave Tension

July 17, 2026
CMB Spectral Distortions: The μ-Distortion Window Into Inflation

July 16, 2026
CMB Lensing vs. the S8 Tension: Did ACT DR6 and KiDS-Legacy Just End Cosmology's Structure-Growth Crisis?

July 15, 2026
Axion Early Dark Energy: The Pre-Recombination Scalar Field Resolving the Hubble Tension

July 14, 2026
The Hemispherical Power Asymmetry: A Field-Theoretic Analysis of the CMB's Lopsided Sky
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.