Despite its prominence in theoretical models, several questions remain unanswered regarding the extent of energy extracted via the BZ process and the mechanisms that determine whether this energy powers jets or dissipates as heat.
To delve into these mysteries, JILA postdoctoral researcher Prasun Dhang, alongside JILA Fellows and University of Colorado Boulder professors Mitch Begelman and Jason Dexter, employed advanced simulations to analyze highly magnetized accretion disks. Their findings, recently published in *The Astrophysical Journal*, shed light on the intricate physics surrounding black holes and may reshape our understanding of their influence on galactic evolution.
"It's long been known that infalling gas can extract spin energy from a black hole," said Dexter. "Usually, we assume this is important for powering jets. By making more precise measurements, Prasun has shown there's a lot more energy extracted than previously known. This energy could be radiated away as light, or it could cause gas to flow outwards. Either way, extracted spin energy could be an important energy source for lighting up the regions near the black hole event horizon."
However, high-luminosity black holes with thinner and more magnetized disks present a greater challenge. Theoretical models suggest these disks should be unstable due to complex heating and cooling dynamics. Earlier work, including studies by Begelman, indicated that magnetic fields might stabilize such disks, yet the specifics of their role in energy extraction and jet formation remained elusive.
"We wanted to understand how energy extraction works in these highly magnetized environments," Dhang explained.
Using this framework, they simulated black holes spinning at different rates to observe how magnetic flux influenced energy extraction and jet formation.
"The goal was to see how magnetic flux threading the black hole impacts energy extraction and whether it leads to the formation of jets," Dhang said.
The simulations examined how much energy black holes transferred to their surroundings under varying conditions. By analyzing different spin rates and magnetic configurations, the team identified scenarios where energy extraction efficiently fueled jets.
"The higher the spin, the more energy the black hole can release," Dhang noted.
However, not all extracted energy contributed to jets; some was reabsorbed by the disk or dissipated as heat. The exact destination of this residual energy remains uncertain, prompting Dhang to pursue further studies on jet formation, which plays a crucial role in active galactic nuclei, including quasars.
"The unused energy close to the black hole could heat the disk and contribute to a corona," Dhang said.
The corona-a region of hot gas encircling black holes that emits intense X-rays-is critical for shaping the light observed from these systems, yet its formation remains an open question.
Future studies will employ advanced simulations to better understand how black hole coronas emerge and evolve.
This research was supported by the National Science Foundation, the NASA Astrophysics Theory Program, and the Alfred P. Sloan Fellowship.
Research Report:Energy Extraction from a Black Hole by a Strongly Magnetized Thin Accretion Disk
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