Sunyaev-Zel’dovich Effect – Definition & Detailed Explanation – Cosmology Glossary

I. What is the Sunyaev-Zel’dovich Effect? The Sunyaev-Zel’dovich Effect, named after Russian astrophysicists Rashid Sunyaev and Yakov Zel’dovich, is a phenomenon in astrophysics that occurs when high-energy electrons in the hot gas of galaxy clusters scatter off of the cosmic microwave background radiation (CMB). This effect causes a distortion in the CMB spectrum, which can … Read more

Peebles Model – Definition & Detailed Explanation – Cosmology Glossary

I. What is the Peebles Model? The Peebles Model, named after physicist James Peebles, is a theoretical framework that seeks to explain the formation and evolution of large-scale structures in the universe. It is a key component of modern cosmology and has played a significant role in shaping our understanding of the universe’s origins and … Read more

Silk Damping – Definition & Detailed Explanation – Cosmology Glossary

What is Silk Damping? Silk damping is a phenomenon in cosmology that refers to the smoothing out of small-scale density fluctuations in the early universe due to the diffusion of photons. This process occurs during the era of recombination, when the universe was around 380,000 years old and had cooled down enough for electrons and … Read more

Primordial Isotopes – Definition & Detailed Explanation – Cosmology Glossary

I. What are Primordial Isotopes? Primordial isotopes are isotopes that were formed during the early stages of the universe, specifically during the Big Bang. These isotopes are considered to be some of the oldest elements in the universe and have remained relatively unchanged since their formation. Primordial isotopes are crucial in understanding the history and … Read more

Cosmological Inhomogeneity – Definition & Detailed Explanation – Cosmology Glossary

I. What is Cosmological Inhomogeneity? Cosmological inhomogeneity refers to the uneven distribution of matter and energy in the universe on large scales. In a homogeneous universe, matter and energy would be evenly distributed throughout space, with the same properties and characteristics in every direction. However, observations have shown that the universe is not perfectly homogeneous, … Read more