Discussion Overview
The discussion revolves around the gravitational properties of neutron stars compared to their original stars, particularly focusing on why neutron stars exhibit stronger gravity despite containing the same mass. Participants explore concepts related to gravitational force, compaction of mass, and the generation of gravitational waves during collisions of compact objects like black holes and neutron stars.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant questions why the gravity of a neutron star is stronger than that of its original star, suggesting that since the mass remains the same, gravity should also be the same unless compaction affects it.
- Another participant asserts that the total gravity of a neutron star does not increase, but the gravitational force experienced can be much stronger due to the proximity to the mass when it is compacted into a smaller volume.
- Some participants discuss the relationship between distance from the center of mass and gravitational force, noting that being closer to the mass of a neutron star results in significantly stronger gravity compared to a larger star.
- Questions are raised about the detection of gravitational waves, specifically why only colliding black holes produce detectable waves, with some suggesting that the high density of black holes contributes to this phenomenon.
- It is mentioned that gravitational waves have also been detected from merging neutron stars, indicating that both types of compact objects can produce gravitational waves during their interactions.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between mass compaction and gravitational strength, with some asserting that gravity remains the same for a given mass regardless of compaction, while others emphasize the importance of proximity to the mass in determining gravitational force. The discussion on gravitational waves also reveals a lack of consensus on the conditions necessary for their detection.
Contextual Notes
Participants reference various distances and gravitational forces without resolving the underlying assumptions about gravity in compact objects. The discussion includes unresolved questions about the mechanisms behind gravitational wave production and the specific conditions that lead to their detection.
Who May Find This Useful
This discussion may be of interest to those exploring astrophysics, particularly the properties of neutron stars and black holes, as well as the phenomena of gravitational waves.