WMAP (Wilkinson Microwave Anisotropy Probe) – Definition & Detailed Explanation – Cosmology Glossary

I. What is WMAP (Wilkinson Microwave Anisotropy Probe)? The Wilkinson Microwave Anisotropy Probe, or WMAP, was a NASA spacecraft launched in 2001 with the primary goal of studying the cosmic microwave background radiation (CMB). The CMB is the residual radiation left over from the Big Bang, which occurred approximately 13.8 billion years ago. By studying … Read more

BAO (Baryon Acoustic Oscillations) Peaks – Definition & Detailed Explanation – Cosmology Glossary

I. What are Baryon Acoustic Oscillations (BAO) Peaks? Baryon Acoustic Oscillations (BAO) peaks are a unique feature in the large-scale structure of the universe that provide valuable information about its evolution and composition. These peaks are essentially sound waves that traveled through the early universe, leaving a distinct imprint on the distribution of matter we … Read more

Sachs-Wolfe Effect – Definition & Detailed Explanation – Cosmology Glossary

I. What is the Sachs-Wolfe Effect? The Sachs-Wolfe Effect is a phenomenon in cosmology that describes the relationship between the temperature fluctuations in the cosmic microwave background radiation (CMB) and the gravitational potential of large-scale structures in the universe. It was first proposed by Rainer K. Sachs and Arthur M. Wolfe in 1967 as a … Read more

Backreaction (Cosmology) – Definition & Detailed Explanation – Cosmology Glossary

I. What is Backreaction in Cosmology? Backreaction in cosmology refers to the idea that the presence of inhomogeneities and fluctuations in the universe can have a significant impact on its overall evolution. In standard cosmological models, these small-scale structures are often ignored or treated as perturbations around a homogeneous and isotropic background. However, recent research … Read more