Prospects for gravitational wave and ultra-light dark matter detection with binary resonances beyond the secular approximation
gr-qc, astro-ph.CO, astro-ph.IM, hep-ph
Submitted: 2025-04-23
Updated: 2026-09-23
Comments: 37 pages, 19 figures. Updated to journal published version
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
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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