Intermediate Black Holes

Intermediate black holes are a class of black holes with masses between stellar black holes and supermassive black holes. They have masses ranging from 100 to 100,000 times that of the sun. These black holes are of particular interest to astronomers as they may provide insights into the formation and growth of supermassive black holes.

Formation of Intermediate Black Holes

Intermediate black holes are thought to form through a variety of mechanisms. One proposed mechanism is the direct collapse of massive gas clouds in the early universe. Another possibility is the merger of smaller black holes, leading to the creation of intermediate-sized black holes.

Characteristics of Intermediate Black Holes

Intermediate black holes exhibit characteristics that are distinct from both stellar black holes and supermassive black holes. They are larger and more massive than stellar black holes, but smaller and less massive than supermassive black holes. Their presence can be inferred through their gravitational effects on surrounding matter, such as stars and gas clouds.

Study Guide

1. Mass Range: What is the mass range for intermediate black holes?
2. Formation: Describe the proposed mechanisms for the formation of intermediate black holes.
3. Characteristics: How do the characteristics of intermediate black holes differ from those of stellar black holes and supermassive black holes?
4. Observation: How can the presence of intermediate black holes be inferred?

Further Research

For further understanding of intermediate black holes, it is recommended to explore the latest research articles, astronomical observations, and theoretical models related to these intriguing cosmic objects.