Discussion Overview
The discussion revolves around the maximum weight of a neutron star, exploring theoretical limits, implications of mass thresholds, and the conditions under which a neutron star may collapse into a black hole. The scope includes theoretical constructs, equations of state, and the implications of mass measurements.
Discussion Character
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants reference an article stating a maximum weight of 2.16 solar masses for a neutron star, questioning its accuracy and the implications of exceeding this mass.
- Others note that theoretical constructions generally suggest a maximum mass of less than 3 solar masses, indicating a range of accepted values.
- One participant cautions against interpreting the term "infinitesimal addition" too liberally, suggesting that a few percent uncertainty could represent a significant mass change.
- Another participant proposes that the equation of state used is crucial, suggesting that a "stiff" equation could allow for a neutron star mass limit of about 5 solar masses before collapsing into a black hole.
- It is mentioned that rotating neutron stars may be stabilized by angular momentum, potentially allowing them to exceed the mass limits of stationary stars before collapse.
- Concerns are raised about the longevity of neutron stars exceeding 3 solar masses, indicating that such stars may not exist for extended periods.
Areas of Agreement / Disagreement
Participants express differing views on the maximum mass of neutron stars, with no consensus reached on a definitive limit. Multiple competing models and interpretations of the data are presented.
Contextual Notes
The discussion highlights the dependence on specific equations of state and the uncertainties in mass measurements, which may influence the conclusions drawn about neutron star stability and collapse.