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What is Pulse Profiles of Accreting NS From GRMHD Simulations 2025 about?

This study investigates the pulse profiles of accreting millisecond pulsars using global three-dimensional general relativistic magnetohydrodynamic (GRMHD) simulations. It reveals that the morphology of accretion hotspots and the resulting X-ray emissions are influenced by the magnetic inclination of the neutron star, leading to significant variability in pulse amplitudes and characteristics. The findings enhance our understanding of the neutron star

Author

abderrahimelkhou00

Language

EN