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Inferring Neutron-star Properties from Gravitational-wave Signals of Binary Mergers by Bauswein, A.; Stergioulas, N.; Janka, H. -T. is a scholarly article available to read on EtoBox.

What is Inferring Neutron-star Properties from Gravitational-wave Signals of Binary Mergers about?

The oscillations of a merger remnant forming after the coalescence of two neutron stars are very characteristic for the high-density equation of state. The dominant oscillation frequency occurs as a pronounced peak in the kHz range of the gravitational-wave spectrum. We describe how the dominant oscillation frequency of the remnant can be employed to infer the radii of non-rotating neutron stars.

Author

Bauswein, A.; Stergioulas, N.; Janka, H. -T.

Published

2015

Language

EN