Discussion Overview
The discussion centers on the gravitational collapse of a cylinder, exploring theoretical frameworks and models that may describe its behavior under collapse. Participants examine the relationship between mass, radius, and height, and consider implications for event horizons and singularities.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants reference the Schwarzschild solution for spherical masses and inquire about analogous treatments for cylindrical masses.
- There is a proposal that any collapsing cylinder would ultimately form a sphere if it is not rotating, linked to the "no hair theorem." However, exceptions are noted for infinitely long cylinders.
- Participants discuss the maximum height to diameter (H/D) ratio for a cylinder to form an event horizon, particularly considering a square cylinder on the verge of collapse.
- Some express uncertainty about whether the black hole theorem applies if the result of collapse is a different type of singularity rather than a conventional black hole.
- One participant speculates on the behavior of a finite cylinder that is long enough for the collapse of its ends to occur outside the past light cone of the center reaching infinite density.
- The Weyl vacuum is mentioned as a cylindrical equivalent to the spherically symmetric vacuum, though participants note a lack of solutions for a collapsing cylinder.
- It is stated that the requirements for an event horizon depend on mass being contained within a certain radius, regardless of the shape of the mass.
- Some participants challenge earlier claims and refine their arguments, but no consensus is reached on the implications of these discussions.
Areas of Agreement / Disagreement
Participants express multiple competing views on the behavior of collapsing cylinders, the applicability of the no hair theorem, and the nature of singularities. The discussion remains unresolved with no clear consensus.
Contextual Notes
Limitations include the dependence on specific definitions of mass and radius, as well as unresolved mathematical steps regarding the conditions under which event horizons form.