Prospects for studying Galactic neutron stars in binaries with LISA

Valeriya Korol

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Abstract

So far detached compact binaries containing neutron stars have been observed either at intermediate stages of the evolution by radio telescopes or at merger by ground-based gravitational wave detectors. Sensitive to gravitational waves from binaries millions to thousands years prior to the merger, the future Laser Interferometer Space Antenna (LISA) will be crucial for bridging the gap between the currently accessible regimes. Depending on the binary type, LISA could potentially discover from a few to several hundreds in the entirely new regime throughout the Milky Way. Here we provide a concise summary of the current expectation for the detection of Galactic binaries containing neutron stars with LISA, focusing on double neutron stars and neutron star - white dwarf binaries. We outline a few examples of science investigations that LISA data will enable for these binaries.
Original languageEnglish
Pages (from-to)203-206
JournalProceedings of the International Astronomical Union
Volume16
Issue numberS363
DOIs
Publication statusPublished - 1 Jun 2020

Keywords

  • Gravitational waves
  • binaries: close
  • stars: neutron
  • white dwarfs

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