What theoretical limit governs the maximum stable mass for a neutron star like a magnetar?

Answer

The Tolman-Oppenheimer-Volkoff (TOV) limit

The absolute maximum mass that a neutron star can support against the overwhelming force of its own gravity before succumbing to complete collapse is defined by a critical threshold known in astrophysics as the Tolman-Oppenheimer-Volkoff (TOV) limit. When a stellar remnant, regardless of whether it is a standard neutron star or a magnetar, exceeds this threshold—a point where even the outward pressure generated by degenerate neutrons fails to resist gravity—an unstoppable implosion begins. This boundary condition is fundamental to determining the ultimate fate of these ultra-dense objects, signaling the irreversible transition toward forming a singularity.

What theoretical limit governs the maximum stable mass for a neutron star like a magnetar?

#Videos

What If a Magnetar Collided With a Black Hole? - YouTube

What if a Magnetar Came Close to Earth? - YouTube

Related Questions

What intensity in Gauss defines the upper range of a magnetar's magnetic field?What process is responsible for generating a magnetar's phenomenal magnetic field strength?What high-energy radiation bursts are caused by stresses on a magnetar's crust?If a magnetar's magnetic field decays before mass limits are reached, what does it become?What theoretical limit governs the maximum stable mass for a neutron star like a magnetar?How does the magnetic pressure in a magnetar potentially affect the application of the TOV limit?What is the stated final destiny for the magnetar's magnetic field after crossing the event horizon?Which observational signal is primarily anticipated from the final gravitational collapse of a massive magnetar?How do the observational signatures of a magnetar's birth via collision differ from its death via collapse?What happens to the initial mass estimate of a magnetar if its magnetic field acts as a temporary support beam?
starastrophysicsneutron starcollapsemagnetar