What is the approximate solar mass range for a collapsing core to stabilize specifically as a neutron star?
Answer
Between approximately 1.4 and 3 solar masses.
When the collapsing core mass stabilizes in the range between roughly 1.4 and 3 solar masses, the pressure forces protons and electrons together to form neutrons, creating a neutron star supported by neutron degeneracy pressure.
Related Questions
What triggers the catastrophic implosion in a core-collapse supernova?What speeds can the collapsing iron core approach during implosion?What results from a Type Ia supernova event?What quantum mechanical force is capable of stabilizing a core that is not too heavy after implosion?What is the approximate solar mass range for a collapsing core to stabilize specifically as a neutron star?What happens if the remnant core mass exceeds the Tolman-Oppenheimer-Volkoff (TOV) limit?Where are elements heavier than iron, such as gold and uranium, primarily forged?What is the immediate, visible aftermath of a supernova explosion called?For what initial star mass is a core-collapse supernova the expected fate?What feature defines the boundary of a black hole from which no information can return?