Erratum: “Future Prospects for Ground-based Gravitational-wave Detectors: The Galactic Double Neutron Star Merger Rate Revisited” (2019, ApJ, 870, 71)

2019 ◽  
Vol 874 (2) ◽  
pp. 186 ◽  
Author(s):  
Nihan Pol ◽  
Maura McLaughlin ◽  
Duncan R. Lorimer
Keyword(s):  
Neutron Star ◽  
Gravitational Wave ◽  
Future Prospects ◽  
Gravitational Wave Detectors ◽  
Merger Rate

PULSAR KICKS AND DARK MATTER FROM A STERILE NEUTRINO

2005 ◽  
Vol 20 (06) ◽  
pp. 1148-1154 ◽  
Author(s):  
ALEXANDER KUSENKO
Keyword(s):  
Dark Matter ◽  
Neutron Star ◽  
Gravitational Wave ◽  
Sterile Neutrino ◽  
Supernova Explosion ◽  
Radio Pulsars ◽  
X Ray ◽  
Gravitational Wave Detectors ◽  
Rule Out

The observed velocities of radio pulsars, which range in the hundreds kilometers per second, and many of which exceed 1000 km/s, are not explained by the standard physics of the supernova explosion. However, if a sterile neutrino with mass in the 1–20 keV range exists, it would be emitted asymmetrically from a cooling neutron star, which could give it a sufficient recoil to explain the pulsar motions. The same particle can be the cosmological dark mater. Future observations of X-ray telescopes and gravitational wave detectors can confirm or rule out this explanation.

scholarly journals Implementing a search for aligned-spin neutron star-black hole systems with advanced ground based gravitational wave detectors

2014 ◽  
Vol 90 (8) ◽  
Author(s):  
Tito Dal Canton ◽  
Alexander H. Nitz ◽  
Andrew P. Lundgren ◽  
Alex B. Nielsen ◽  
Duncan A. Brown ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Gravitational Wave ◽  
Gravitational Wave Detectors

scholarly journals Exploring the sensitivity of gravitational wave detectors to neutron star physics

2019 ◽  
Vol 99 (10) ◽  
Author(s):  
Denis Martynov ◽  
Haixing Miao ◽  
Huan Yang ◽  
Francisco Hernandez Vivanco ◽  
Eric Thrane ◽  
...  
Keyword(s):  
Neutron Star ◽  
Gravitational Wave ◽  
Gravitational Wave Detectors
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