Supercomputer Simulations Explain Massively Powerful Black Hole Jet – Confirms Einstein’s

Gigantic Jet Spied From Black Hole in Early Universe

Cupermassive black hole with an X-ray jet. Credit: NASA/CXC/M.Weiss

Further confirmation of Einstein’s theory of general relativity.

The galaxy Messier 87 (M87) is located 55 million light years away from Earth in the Virgo constellation. It is a giant galaxy with 12,000 globular clusters, making the M87 Relativistic Jet Theoretical Model and Astronomical Observations

The theoretical model (theory) and the astronomical observations (observation) of the launching site of the relativistic jet of M87 are a very good match. Credit: Alejandro Cruz-Osorio

The black hole M87* attracts matter that rotates in a disc in ever smaller orbits until it is swallowed by the black hole. The jet is launched from the center of the accretion disc surrounding M87, and theoretical physicists at Goethe University, together with scientists from Europe, USA, and China, have now modeled this region in great detail.

They used highly sophisticated three-dimensional supercomputer simulations that use the staggering amount of a million CPU hours per simulation and had to simultaneously solve the equations of general relativity by Albert Einstein, the equations of electromagnetism by James Maxwell, and the equations of fluid dynamics by Leonhard Euler.

M87 Black Hole Magnetic Field Lines Relativistic Jet

Along the magnetic field lines, the particles are accelerated so efficiently that they form a jet out to scales of 6000 light years in the case of M87. Credit: Alejandro Cruz-Osorio

The result was a model in which the values calculated for the temperatures, the matter densities and the magnetic fields correspond remarkably well with what deduced from the astronomical observations. On this basis, scientists were able to track the complex motion of photons in the curved spacetime of the innermost region of the jet and translate this into radio images. They were then able to compare these computer-modeled images with the observations made using numerous radio telescopes and satellites over the past three decades.

Dr. Alejandro Cruz-Osorio, lead author of the study, comments: “Our theoretical model of the electromagnetic emission and of the jet morphology of M87 matches surprisingly well with the observations in the radio, optical and infrared spectra. This tells us that the supermassive black hole M87* is probably highly rotating and that the plasma is strongly magnetized in the jet, accelerating particles out to scales of thousands of light years.”

Professor Luciano Rezzolla, Institute for Theoretical Physics at Goethe University Frankfurt, remarks: “The fact that the images we calculated are so close to the astronomical observations is another important confirmation that Einstein’s theory of general relativity is the most precise and natural explanation for the existence of supermassive black holes in the center of galaxies. While there is still room for alternative explanations, the findings of our study have made this room much smaller.”

Reference: “State-of-the-art energetic and morphological modelling of the launching site of the M87 jet” by Alejandro Cruz-Osorio, Christian M. Fromm, Yosuke Mizuno, Antonios Nathanail, Ziri Younsi, Oliver Porth, Jordy Davelaar, Heino Falcke, Michael Kramer and Luciano Rezzolla, 4 November 2021, Nature Astronomy.
DOI: 10.1038/s41550-021-01506-w

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