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A neutron star cannot spin with less than a certain critical period, or else it will start to lose mass from its equator due to the “centrifugal” force. Estimate this period.
The critical period for a neutron star is definitively estimated to be between 8 and 12 years. This period is crucial as it determines the stability of the star's mass against centrifugal forces. Understanding this concept is essential for those studying neutron star physics and high-energy astrophysics.
PREREQUISITESThis discussion is beneficial for astrophysics students, researchers in high-energy astrophysics, and anyone interested in the physical properties and behaviors of neutron stars.
DaveC426913 said:Definitinely between 8 and 12 years, those are the formative years for healthy growth, and good nutrition during this time is critical.
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