Testing the accuracy of our method by numerically stimulating hydrodynamic spherical bondi accretion.

Our numerical scheme utilizes the GRMHD code KHARMA[1], a performance-portable C++ implementation based on iharm3D; iharm3D is itself an extension of HARM.

To investigate the mechanism driving the turbulence, we explore the physics of the outward flow of energy.

The authors HC, RN, PN, KS, AR, and KC acknowledge support from the Gordon and Betty Moore Foundation and the John Templeton Foundation

If you want to continue learning about black holes, here's a list of all the references.

Find out the definitions of Hydrodynamic Simulation Setup and Magnetohydrodynamic Simulation Setup and how they pertain to black holes

Find out what GRMHD is and other various definitions to get a deeper grasp of our black hole study.

Wrapping up our black hole study: a final rundown.

Explore how the PBH model's prediction of increasing binary merger rates with redshift, particularly at z ≥ 30, could provide evidence that PBHs exist.

The roadmap for PBH research is set to expand with a range of innovative experiments, from terrestrial and space-based interferometers to lunar arrays. read on!

This paper takes a look at the constraints, possible detection methods, and future tests for PBHs as dark matter candidates.

This paper discusses the current constraints and the potential role of PBHs in observed gravitational wave signals.

This paper discusses the potential effects of PBH clustering on key astronomical observations and the formation of massive structures in the universe.

This paper discusses the challenges in calculating PBH abundance, focusing on the role of nonlinear perturbations.

Learn the unresolved questions surrounding primordial black holes (PBHs), including their abundance, clustering properties, and more.

Explore the intriguing role of primordial black holes (PBHs) in dark matter and gravitational wave astronomy.

Did you know? The existence of primordial black holes (PBHs) is backed by theories in dark matter physics, astrophysics, and quantum cosmology.

Gamma-ray telescopes of the future are set to advance the search for PBHs by detecting signals from Hawking evaporation and other related phenomena.

Learn how distinguishing PBHs from other compact objects through tidal disruption and deformability measurements might reveal new insights into dark matter.

Learn how primordial black holes (PBHs) may address the challenge of the pair instability gap in black hole mass spectra.