It is a mystery that has stymied astrophysicists for decades: How do black holes produce so many high-power X-rays?
In a new study, astrophysicists from Johns Hopkins, NASA, and the Rochester Institute of Technology bridged the gap between theory and observation by demonstrating that gas spiraling toward a black hole inevitably results in X-ray emissions.
The paper states that as gas spirals toward a black hole through a formation called an accretion disk, it heats up to roughly 10 million degrees Celsius. The temperature in the main body of the disk is roughly 2,000 times hotter than the sun and emits low-energy or "soft" X-rays. However, observations also detect "hard" X-rays, which produce up to 100 times higher energy levels.
Julian Krolik, a professor of physics and astronomy in the Krieger School of Arts and Sciences, and his fellow scientists used a combination of supercomputer simulations and traditional handwritten calculations to uncover their findings. Supported by 40 years of theoretical progress, the team showed for the first time that high-energy light emission is not only possible but is an inevitable outcome of gas being drawn into a black hole.
"Black holes are truly exotic, with extraordinarily high temperatures, incredibly rapid motions, and gravity exhibiting the full weirdness of general relativity," Krolik says. "But our calculations show we can understand a lot about them using only standard physics principles."
The team's work was recently published in the print edition of Astrophysical Journal. Krolik's collaborators were Jeremy Schnittman, a research astrophysicist from the NASA Goddard Space Flight Center, and Scott Noble, an associate research scientist from the Center for Computational Relativity and Gravitation at RIT. Schnittman was lead author.
As the quality and quantity of high-energy light observations improved over the years, evidence mounted that photons must be created in a hot, tenuous region called the corona. This corona, boiling violently above the comparatively cool disk, is similar to the one surrounding the sun, which is responsible for much of the ultraviolet and X-ray luminosity seen in the solar spectrum.
While the team's study of black holes and high-energy light confirms a widely held belief, the role of advancing modern technology should not be overlooked. A grant from the National Science Foundation enabled the team to access Ranger, a supercomputing system at the Texas Advanced Computing Center located at the University of Texas in Austin. Ranger worked over the course of about 27 days, for more than 600 hours, to solve the equations.
Noble developed the computer simulation solving all the equations governing the complex motion of inflowing gas and its associated magnetic fields near an accreting black hole.
The rising temperature, density, and speed of the inflowing gas dramatically amplify magnetic fields threading through the disk, which then exert additional influence on the gas. The result is a turbulent froth orbiting the black hole at speeds approaching the speed of light. The calculations simultaneously tracked the fluid, electrical, and magnetic properties of the gas while also taking into account Einstein's theory of relativity.
"In some ways, we had to wait for technology to catch up with us," Krolik says. "It's the numerical simulations going on at this level of quality and resolution that make the results credible."
The scientists are familiar with one another as their paths all crossed at Johns Hopkins. Schnittman was a postdoctoral fellow mentored by Krolik from 2007 to 2010, and Noble was an assistant research scientist and instructor, also under Krolik, from 2006 to 2009.
The work was supported by three National Science Foundation grants.
