Discussion Overview
The discussion revolves around the characterization of neutron stars, specifically whether their surfaces can be considered the smoothest in the universe. Participants explore various aspects of neutron star surfaces, including their physical properties, the presence of mountains, and comparisons to other smooth objects, while delving into the implications of atomic structures and the effects of extreme conditions.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
- Mathematical reasoning
Main Points Raised
- One participant suggests that neutron stars have surfaces that could be considered the smoothest due to the small scale of particle spacing and the effects of degeneracy pressure.
- Another participant cites that neutron stars can have surface irregularities, such as mountains measuring up to ~1cm, which raises questions about their overall smoothness.
- There is a discussion about whether neutron stars have perfect crystal lattices, with some participants expressing skepticism about the existence of such structures under extreme conditions.
- Some participants mention that neutron star cores are superfluid and exotic, suggesting that they may not resemble traditional crystals.
- Comparisons are made between neutron stars and other objects, such as the Hubble Space Telescope mirror and fused quartz gyroscopes, with varying claims about their smoothness.
- One participant humorously suggests that human skin could be smoother than a neutron star, prompting further light-hearted commentary.
- Another participant discusses the density differences between neutron stars and white dwarfs, emphasizing the significant distinctions in their physical properties.
- There are references to the methods used to measure smoothness and the implications of the coastline paradox in defining "smoothness."
Areas of Agreement / Disagreement
Participants express a range of views on the smoothness of neutron stars, with no consensus reached. Some argue for their smoothness based on theoretical considerations, while others point out physical irregularities and question the validity of such claims.
Contextual Notes
Participants note the dependence on definitions of smoothness and the scale at which measurements are made, highlighting the complexity of the topic. There are unresolved questions regarding the atomic structure of neutron star surfaces and the implications of extreme conditions on their properties.