Prospects for LISA to detect a gravitational-wave background from first order phase transitions

Abstract

First order phase transitions in the early universe could produce a gravitational-wave background that might be detectable by the Laser Interferometer Space Antenna (LISA). Such an observation would provide evidence for physics beyond the Standard Model. We study the ability of LISA to observe a gravitational-wave background from phase transitions in the presence of an extragalactic foreground from binary black hole mergers throughout the universe, a galactic foreground from white dwarf binaries, and LISA noise. Modelling the phase transition gravitational wave background as a double broken power law, we use the deviance information criterion as a detection statistic, and Fisher matrix and Markov Chain Monte Carlo methods to assess the measurement accuracy of the parameters of the power spectrum. While estimating all the parameters associated with the gravitational-wave backgrounds, foregrounds, and LISA noise, we find that LISA could detect a gravitational-wave background from phase transitions with a peak frequency of 1 mHz and normalized energy density amplitude of ${\Omega }_{\text{p}}\simeq 3\times 10^{-11}$. With ${\Omega }_{\text{p}}\simeq 10^{-10}$, the signal is detectable if the peak frequency is in the range $4\times 10^{-4}$ to $9\times 10^{-3}$ Hz, and the peak amplitude and frequency can be estimated to an accuracy of 10\% to 1\%.

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Cited by in corpus (20)

• Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
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• Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA
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• Reconstructing physical parameters from template gravitational wave spectra at LISA: first order phase transitions
• Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
• A weakly-parametric approach to stochastic background inference in LISA
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• Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds
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• Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA
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• Reconstructing early universe evolution with gravitational waves from supercooled phase transitions
• Superfluids in expanding backgrounds and attractor times
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• Gravitational waves from the sound shell model: direct and inverse phase transitions in the early Universe
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