Researchers have suggested the existence of a new type of neutron star. In his article published in
Previous studies have shown that neutronstars are formed when an ordinary star collapses under its own gravity, becoming a supernova. The resulting neutron star-like remnant is much smaller and highly dense.
Also, physicists previously suggested that whenIn the collision of two neutron stars, a single object with a mass exceeding the Tolman-Oppenheimer-Volkow limit will appear and, therefore, collapse into a black hole. However, this limitation only applies to neutron stars that stop spinning due to a collision.
Scientists have now suggested that a star that is not rotating can still exist for a period of time under certain circumstances.
Suvorov and Glampedakis believe that ifWhen two stars collide, a strong enough magnetic field will be generated that will prevent the formation of a black hole. At least for a few years. Scientists suggest that the lifetime of such a star would depend on a variety of factors, including the strength of the magnetic fields of both neutron stars before the collision, their masses, and the temperature of their cores.
If such a neutron star appeared, thenIt would have a unique signature consisting of rapid bursts of gamma rays, then X-rays in the initial stage, and then rapid bursts of radio waves as its gravitational field weakened.
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