Low Frequency Gravitational Waves from White Dwarf MACHO Binaries

TL;DR

This paper estimates the gravitational wave background from halo white dwarf binaries, suggesting they could dominate signals detected by LISA and thus help identify dark MACHO populations.

Contribution

It models the contribution of halo white dwarf binaries to low-frequency gravitational waves based on disk binary properties, highlighting their potential dominance.

Findings

Halo white dwarf binaries could produce a gravitational wave background five times stronger than disk binaries.

This background may dominate LISA's response, aiding dark MACHO detection.

Low-frequency gravitational wave observations are crucial for understanding dark matter in the form of MACHOs.

Abstract

The possibility that Galactic halo MACHOs are white dwarfs has recently attracted much attention. Using the known properties of white dwarf binaries in the Galactic disk as a model, we estimate the possible contribution of halo white dwarf binaries to the low-frequency (10^{-5} Hz} < f < 10^{-1}Hz) gravitational wave background. Assuming the fraction of white dwarfs in binaries is the same in the halo as in the disk, we find the confusion background from halo white dwarf binaries could be five times stronger than the expected contribution from Galactic disk binaries, dominating the response of the proposed space based interferometer LISA. Low-frequency gravitational wave observations will be the key to discovering the nature of the dark MACHO binary population.