Discussion Overview
The discussion revolves around the implications of the rotation rate of the neutron star PSR J1748-2446ad, particularly concerning the conservation of momentum and the possibility of surface speeds exceeding the speed of light. Participants explore theoretical aspects related to angular momentum and relativistic effects.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant questions how conservation of momentum can hold if a neutron star's surface speed could theoretically exceed the speed of light based on its initial rotation rate.
- Another participant explains that angular momentum does not scale linearly with angular velocity and suggests that the conservation of angular momentum can be maintained without exceeding the speed of light.
- A later reply emphasizes that momentum does not increase linearly with speed and provides a relativistic formula for momentum, indicating that large momentum can be achieved at speeds below the speed of light.
- Some participants acknowledge the complexity of neutron stars and the need to consider their full stress-energy tensor in these discussions.
Areas of Agreement / Disagreement
Participants express differing views on the implications of neutron star rotation rates and the conservation of momentum, with no consensus reached on whether speeds greater than light could be permissible or how angular momentum is conserved in such scenarios.
Contextual Notes
Participants note the limitations of the Newtonian approximation when discussing relativistic speeds and the complexities involved in neutron star physics.