R-mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar

The nature of GW190814's secondary component m 2 of mass 2.50–2.67 M ⊙ in the mass gap between the currently known maximum mass of neutron stars and the minimum mass of black holes is currently under hot debate. Among the many possibilities proposed in the literature, m 2 was suggested to be a...

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Veröffentlicht in:	The Astrophysical journal 2021-03, Vol.910 (1), p.62
Hauptverfasser:	Zhou, Xia, Li, Ang, Li, Bao-An
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTRONOMY AND ASTROPHYSICS Astrophysics Black holes Damping Equations of state Mathematical models Neutron stars Nuclear interactions Nuclear physics Pulsars Radiation X ray binaries X ray stars
Online-Zugang:	Volltext
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