Pulsars and Gravitational Waves Research

Simulations show turbulent black hole coronae generate two-temperature plasmas with extended nonthermal ion distributions while producing observed X-ray spectra.

Explore how space-based gravitational wave detectors can detect axion-like dark matter using different time-delay interferometry combinations, achieving sensitivity across a broad mass range.

Numerical study of self-gravitating bosonic systems reveals critical thresholds for equilibrium and stability in the nonrelativistic regime, with applications to ultralight dark matter candidates.

Analysis of gravitational-wave data reveals that merging black holes predominantly exhibit near-perpendicular spin orientations, suggesting most form in triple-star systems.

Study explores how magnetic charge in regular black holes alters gravitational waveforms from periodic orbits, offering new constraints on black hole properties through gravitational wave.

Gravitational atom spectroscopy reveals how self-gravitating scalar field clouds around black holes produce detectable quasinormal mode frequency shifts in gravitational wave signatures.

Theoretical framework proves transformers efficiently learn Earth's gravitational field with quantum gravimetry advantages, but inverse problems remain intractable.

Numerical model reveals that simplified approximations for synchrotron emission from relativistic shocks can be inaccurate by over an order of magnitude, biasing inferred properties of transients.

Existence proof of Q-Monopole-Ball solitons with unit magnetic charge using shooting methods, extending classical monopole theory and providing non-gravitational binding mechanisms.

Compare orbital perturbation modeling methods using ephemeris data. Analyze indirect and frame center acceleration approaches for Earth-Moon system trajectories, examining consistency versus.

Fast, physically consistent framework for modeling interaction-powered transients through self-consistent ejecta-CSM shock and radiative diffusion coupling.

Analytical study of gravitational wave propagation in Myers-Perry higher-dimensional rotating black holes using separation of variables techniques to derive explicit solutions.