Prospects for gravitational wave and ultra-light dark matter detection with binary resonances beyond the secular approximation

arXiv:2504.16988 · gr-qc, astro-ph.CO, astro-ph.IM, hep-ph · Submitted 2025-04-23 · Read on arXiv

gr-qc, astro-ph.CO, astro-ph.IM, hep-ph

Submitted: 2025-04-23

Updated: 2026-09-23

Terminology

• Fisher Information — 7× in this paper · explained in 3 episodes
• Secular Approximation — 5× in this paper · explained in 2 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Degeneracy — 2× in this paper · explained in 3 episodes
• Velocity Dispersion — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Coherence Length — 1× in this paper · explained in 2 episodes
• Scaling Laws — 1× in this paper · explained in 4 episodes
• pulsar timing arrays — 1× in this paper · explained in 2 episodes

Sources

• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Unveiling the Gravitational Universe at \mu-Hz Frequencies
• Bridging the $\mu$Hz gap in the gravitational-wave landscape with binary resonance
• Asteroids for $\mu$Hz gravitational-wave detection
• Constraining the Stochastic Gravitational Wave Background with Photometric Surveys
• Ultra-Light Dark Matter Resonates with Binary Pulsars
• Stochastic gravitational wave background constraints from Gaia DR3 astrometry
• A New Probe of $\mu$Hz Gravitational Waves with FRB Timing
• Binary Systems as Resonance Detectors for Gravitational Waves
• Detecting stochastic gravitational waves with binary resonance
• Gravitational Interaction of Ultralight Dark Matter with Interferometers
• Axion resonances in binary pulsar systems
• Secular effects of Ultralight Dark Matter on Binary Pulsars
• Axion oscillations in binary systems: angle-action surgery
• Discovering mu Hz gravitational waves and ultra-light dark matter with binary resonances
• Cosmological Backgrounds of Gravitational Waves
• Principal Component Analysis: A Natural Approach to Data Exploration
• Ultralight scalars as cosmological dark matter
• Ultra-Light Dark Matter
• Bayesian sensitivity of binary pulsars to ultra-light dark matter

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