Impact of three-nucleon forces on gravitational wave emission from neutron stars

Gravitational wave emission from rotating superfluid neutron stars

In this paper we investigate the effect of a pinned superfluid component on the gravitational wave emission of a steadily rotating deformed neutron star. We show that the superfluid pinning allows the possibility for there to be gravitational wave emission at both the stellar spin frequency Ω and its first harmonic, 2Ω. This contrasts with the conventional case where there is no pinned superflu...

Detecting gravitational wave emission from the known accreting neutron stars

Detection of gravitational waves from accreting neutron stars (NSs) in our galaxy, due to ellipticity or internal oscillation, would be a breakthrough in our understanding of compact objects and explain the absence of NSs rotating near the break-up limit. Direct detection, however, poses a formidable challenge. Using the current data available on the properties of the accreting NSs in Low Mass ...

Cosmological Gravitational Wave Background from Phase Transitions in Neutron Stars

It has recently been suggested that collapse of neutron stars induced by a phase transition to quark matter can be a considerable source of gravitational waves with kHz frequencies. We demonstrate that if about one percent of all neutron stars undergo this process, the resulting cosmological gravitational wave background would reach about 10 times the critical density. The background would peak...

Gravitational Wave Emission From Core-Collapse of Massive Stars

We derive estimates for the characteristics of gravitational radiation from stellar collapse, using recent models of the core-collapse of Chandrasekhar mass white dwarfs (accretion induced collapse), core-collapse supernovae and collapsars, and the collapse of very massive stars (∼> 300M⊙). We study gravitational-wave emission mechanisms using several estimation techniques, including two-dimens...

Gravitational waves from neutron stars