Detecting Planets around Compact Binaries with Gravitational Wave Detectors in Space
arXiv:0802.3411 · doi:10.1086/587785
Abstract
I propose a method to detect planets around compact binaries that are strong sources of gravitational radiation. This approach is to measure gravitational-wave phase modulations induced by the planets, and its prospect is studied with a Fisher matrix analysis. I find that, using the Laser Interferometer Space Antenna (LISA), planets can be searched for around ~3000 Galactic double white dwarfs with detection limit ~4 M_J (M_J~ 2x10^{30}g: the Jupiter mass). With its follow-on missions, planets with mass ~1 M_J might be detected around double neutron stars even at cosmological distances z~1. In this manner, gravitational wave observation has potential to make interesting contributions to extra-solar planetary science.
4 pages, to appear in ApJL
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Cited by in corpus (13)
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- On networks of space-based gravitational-wave detectors
- Searching For Transiting Circumbinary Planets in CoRoT and Ground-Based Data Using CB-BLS
- Prospects for detecting exoplanets around double white dwarfs with LISA and Taiji
- Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
- LISA double white dwarf binaries as Galactic accelerometers
- The role of triple evolution in the formation of LISA double white dwarfs
- Potential Tertiary Effects on the LISA Verification Binary HM Cancri
- Forecasting Tidal Disruption Events by Binary Black Hole Roulettes
- Perturbative Frequency Expansion for Nearly Monochromatic Binary Black Holes Detectable with LISA