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

June 30, 2026
Cosmic Birefringence: How a 0.2° Twist in the CMB's Oldest Light May Reveal Parity-Violating Dark Matter

June 29, 2026
The Negative Neutrino Mass Anomaly: CMB Lensing and the Σmν < 0 Tension After DESI DR2

June 28, 2026
The Negative Neutrino Mass Anomaly: Breaking the Σm_ν Floor with DESI and the CMB

June 27, 2026
The CMB Spectral Index Anomaly: Is Starobinsky Inflation Ruled Out After ACT DR6?

June 25, 2026
The Cosmic Glitch in Gravity: Is Newton's Constant 1% Weaker on Super-Horizon Scales?

June 24, 2026
Cosmic Birefringence: The Twist in the Universe's Oldest Light

June 23, 2026
The S8 Tension Verdict: ACT DR6 CMB Lensing and the 43σ Mass Map

June 22, 2026
Cosmic Inflation vs. the Big Bounce: Did the Universe Bang or Bounce? (2026 Evidence Review)

June 21, 2026
Primordial Magnetic Fields and the bΛCDM Resolution of the Hubble 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.