Search for Neutron Star Binaries in the Local Group Galaxies Using LISA
arXiv:1909.01471 · doi:10.1093/mnras/stz2439
Abstract
We discuss the prospects of LISA for detecting neutron star binaries (NSBs) in the local group galaxies such as LMC and M31. Using the recently estimated merger rate and inversely applying the conventional arguments based on the -band galaxy luminosities, we estimate the frequency distributions of NSBs in the local galaxies. We find that, after 10 year observation with its current design sensitivity, LISA might detect NSBs both in LMC and M31 with signal-to-noise ratios larger than 10. Some of the NSBs might be three-dimensionally localized well within LMC. These binaries will be useful for studying various topics including the origin of r-process elements.
7 pages, 3 figures
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- Ultra-relativistic astrophysics using multi-messenger observations of double neutron stars with LISA and the SKA
- How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
- Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves
- Astrophysics with the Laser Interferometer Space Antenna
- The effects of Galactic model uncertainties on LISA observations of double neutron stars
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- Probing the millisecond pulsar origin of the -ray excess in the Galactic centre with LISA