Discussion Overview
The discussion centers on the size of black holes and whether it can be calculated. Participants explore the relationship between mass and size, the existence of various sizes of black holes, and the implications of general relativity on their characteristics.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- Some participants propose that the size of a black hole is defined by its mass, with the Schwarzschild radius being a key factor.
- Others argue that black holes can vary significantly in size, with examples given such as a black hole with the mass of the Sun having a diameter of about 6 kilometers.
- A participant mentions that a black hole with the mass of Jupiter would have a diameter of approximately 5 to 6 meters, highlighting the extreme density required for black hole formation.
- It is noted that in general relativity, Kerr black holes are a feasible type, characterized by a ring-shaped singularity and two event horizons.
- Some participants discuss the theoretical possibility of creating small black holes in laboratories, referred to as optical black holes.
- A participant provides a formula for calculating the radius of a black hole's event horizon based on its mass, emphasizing that the calculation is straightforward under certain assumptions.
- Another participant mentions that there is no theoretical limit to the size of a black hole, as any amount of mass can form one if compressed to a high enough density.
- It is stated that the Schwarzschild radius is directly proportional to mass, with specific examples given for black holes of varying masses, including a million-solar-mass black hole having a radius of 3 million kilometers.
Areas of Agreement / Disagreement
Participants express a range of views on the size and calculation of black holes, with no consensus reached on the implications of their findings or the limits of black hole sizes.
Contextual Notes
Some calculations and assumptions regarding the mass and density of black holes are discussed, but the discussion does not resolve the complexities involved in these calculations or the definitions used.