Abstract.
Coalescing compact binaries with neutron star (NS) or black hole (BH) components are important sources of gravitational waves for the laser-interferometer detectors currently under construction, and may also be sources of gamma-ray bursts at cosmological distances. This paper focuses on the final hydrodynamic coalescence and merger of NS-NS binaries, and addresses the question of whether black-hole formation is the inevitable final fate of these systems.
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Rasio, F.A. The Final Fate of Coalescing Binary Neutron Stars: Collapse to a Black Hole?. In: Kaper, L., Heuvel, E.P.J.v.d., Woudt, P.A. (eds) Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10720995_74
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DOI: https://doi.org/10.1007/10720995_74
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-41581-7
Online ISBN: 978-3-540-44562-3
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