The discussion revolves around the outcomes of a collision between binary neutron stars, specifically focusing on whether such a merger results in a nova or supernova, and how the final mass of the resulting object influences this outcome. The scope includes theoretical implications, observational requirements, and the potential for gravitational wave and gamma-ray emissions.
Participants express differing views on whether a neutron star merger produces a supernova, with some suggesting it does not, while others highlight the possibility of observable emissions. The discussion remains unresolved regarding the definitive outcomes of such mergers.
Limitations include the current uncertainty surrounding the maximum mass of neutron stars and the implications of mass loss during the merger process, which may affect the final state of the system.
The merger or two neutron stars would not produce a supernova, although the electromagnetic emissions from such a merger may have a similar, but much dimmer, appearance. If the combined mass of both neutron stars exceeds the Tolman-Oppenheimer-Volkoff limit of approximately 3.0 solar masses then a black hole would be formed as a result of the merger. It is also suspected that such a merger would produce gravity waves and may be one source for short duration (less than 2 second) gamma-ray bursts.Irfan Nafi said:I was wondering if a binary system of neutron stars were to collide what kind of nova or supernova would it be. Is it different if the final mass of the neutron star is sufficient enough for a black hole or if it still a neutron star?