Stochastic Gravitational Wave Background from Exoplanets

Abstract

Recent exoplanet surveys have predicted a very large population of planetary systems in our galaxy, more than one planet per star on the average, perhaps totalling about two hundred billion. These surveys, based on electro-magnetic observations, are limited to a very small neighbourhood of the solar system and the estimations rely on the observations of only a few thousand planets. On the other hand, orbital motions of planets around stars are expected to emit gravitational waves (GW), which could provide information about the planets not accessible to electro-magnetic astronomy. The cumulative effect of the planets, with periods ranging from few hours to several years, is expected to create a stochastic GW background (SGWB). We compute the characteristic GW strain of this background based on the observed distribution of planet parameters. We also show that the integrated extragalactic background is comparable or less than the galactic background at different frequencies. Our estimate shows that the net background is significantly below the sensitivities of the proposed GW experiments in different frequency bands. However, we notice that the peak of the spectrum, at around $10^{-5}$Hz, is not too far below the proposed space based GW missions. A future space based mission may be able to observe or tightly constrain this signal, which will possibly be the only way to probe the galactic population of exoplanets as a whole.

7 pages, 2 figures

References in corpus (9)

• A Joint Analysis of BICEP2/Keck Array and Planck Data
• Gravitational-wave sensitivity curves
• One or more bound planets per Milky Way star from microlensing observations
• Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16
• Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
• A new cosmic microwave background constraint to primordial gravitational waves
• Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009-2010 LIGO and Virgo Data
• Estimating the sensitivity of pulsar timing arrays
• Detection regimes of the cosmological gravitational wave background from astrophysical sources