Discovering mu Hz gravitational waves and ultra-light dark matter with binary resonances
astro-ph.CO, gr-qc, hep-ph
Submitted: 2025-04-21
Updated: 2026-09-23
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Physics, Astrophysics and Cosmology with Gravitational Waves
- Unveiling the Gravitational Universe at \mu-Hz Frequencies
- A New Probe of $\mu$Hz Gravitational Waves with FRB Timing
- Dissecting the Stochastic Gravitational Wave Background with Astrometry
- Constraining the Stochastic Gravitational Wave Background with Photometric Surveys
- Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe Mission: Massive black hole binaries, early universe signals and ultra-light dark matter
- Asteroids for $\mu$Hz gravitational-wave detection
- Binary Systems as Resonance Detectors for Gravitational Waves
- Detecting stochastic gravitational waves with binary resonance
- Bridging the $\mu$Hz gap in the gravitational-wave landscape with binary resonance
- The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Ultra-Light Dark Matter
- Ultralight scalars as cosmological dark matter
- Relaxation in a Fuzzy Dark Matter Halo
- Heating of Milky Way disc Stars by Dark Matter Fluctuations in Cold Dark Matter and Fuzzy Dark Matter Paradigms
- Gravitational Interaction of Ultralight Dark Matter with Interferometers
- Ultra-Light Dark Matter Resonates with Binary Pulsars
- Secular effects of Ultralight Dark Matter on Binary Pulsars
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation