Friedmann Equations – Definition & Detailed Explanation – Astronomical Units & Measurements Glossary

I. What are the Friedmann Equations? The Friedmann Equations are a set of equations in cosmology that describe the expansion of the universe. They were first derived by the Russian physicist Alexander Friedmann in the 1920s, and later refined by Belgian physicist Georges Lemaître. These equations are a key component of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric, … Read more

TeVeS (Tensor-Vector-Scalar Gravity) – Definition & Detailed Explanation – Cosmology Glossary

I. What is TeVeS (Tensor-Vector-Scalar Gravity)? TeVeS, short for Tensor-Vector-Scalar Gravity, is a modified theory of gravity proposed by Jacob Bekenstein in 2004. It is an alternative to General Relativity, the prevailing theory of gravity put forth by Albert Einstein in 1915. TeVeS aims to address some of the shortcomings of General Relativity, particularly in … Read more

Galaxy Filaments – Definition & Detailed Explanation – Cosmology Glossary

I. What are Galaxy Filaments? Galaxy filaments are vast, thread-like structures in the universe that consist of galaxies, gas, and dark matter. These filaments are the largest known structures in the universe, spanning hundreds of millions of light-years in length. They are often referred to as the “cosmic web” due to their interconnected and web-like … Read more

Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) – Definition & Detailed Explanation – Telescopes & Observatories Glossary

I. What is the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC)? The Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) is a research institute located at Stanford University in California. It is a joint institute between Stanford University and the SLAC National Accelerator Laboratory, focusing on the study of the universe at the intersection … Read more