Concept: Pulsars and Gravitational Waves Research
Turbulent black hole coronae can produce observed X-ray spectra
How turbulent coronae around black holes accelerate particles and emit X-rays
Different interferometer combinations vary in axion dark matter sensitivity
Detecting ultralight dark matter with different gravitational wave detector configurations
Lorentz violation changes black hole disk images and polarization
Testing Lorentz violation theory through black hole shadow and polarization patterns
Self-gravitating bosonic configurations have a stability limit
When quantum clouds of bosonic particles collapse under gravity, how stable are they?
Black hole merger spins point near perpendicular directions
Black hole mergers show spins tilted perpendicular to their orbits
Magnetic charge changes orbits and waveforms near regular black holes
How magnetic charge affects orbits and gravitational waves near black holes
Gravitational atom spectroscopy
Detecting scalar field clouds around black holes through gravitational wave frequencies
Quantum-Enhanced In-Context Learning for Geopotential Field Estimation: A Theoretical Framework
How quantum sensors and transformers can estimate Earth's gravitational field
Transition-to-plunge self-force waveforms with a spinning primary
Modeling black hole collisions with spinning primaries for next-generation detectors
Approximate shock models fail at sufficiently high velocities
New model reveals large errors in standard shock emission calculations
