Record gamma ray detected in Milky Way’s core

Researchers confirmed the PeVatron source at the galactic center by observing ultra-high-energy gamma rays coming from the Milky Way galaxy. The discovery allows the highest physical processes in the universe to be monitored and sheds light on mysteries at the galactic center.

Researchers peer into a fierce mystery in the Milky Way galaxy at the High Altitude Water Cherenkov (HAWC) observatory, 13,000 feet above sea level in Mexico’s Sierra Negra volcano.

An international team of researchers led by Los Alamos National Laboratory has observed ultra-high-energy gamma rays of more than 100 teraelectron volts, tracing them back to the galactic center for the first time.
“CONFIRMING SOURCE FOR THE FIRST TIME”
“These results are a glimpse into much higher energies than previously seen at the center of the Milky Way,” said Pat Harding, a physicist at Los Alamos and the Department of Energy’s principal investigator on the project. “The research confirms for the first time a PeVatron source of ultra-high-energy gamma rays in a location in the Milky Way known as the Galactic Center Ridge, meaning that the galactic center is home to some of the most extreme physical processes in the universe,” he said.

The HAWC observatory has been collecting data for more than seven years. During this period, the researchers observed about 100 gamma-ray events with energies greater than 100 teraelectron volts. As explained in an analysis led by Sohyoun Yu CArcaron and published in The Astrophysical Journal Letters, these data allow for direct study of cosmic ray interactions with the PeVatron and comparison with other observations, helping to determine the emission processes and the exact location of the center of the Milky Way galaxy.
The sources that can accelerate particles are called PeVatrons, and astronomers are actively pursuing these extreme accelerators in our galaxy.
This region of the Milky Way galaxy is known to contain a supermassive black hole surrounded by neutron stars and white dwarfs that are ripping matter from nearby stars.
The region is blanketed by dense clouds of gas that reach temperatures of millions of degrees and tend to block direct optical observation.
Observing gamma rays is therefore critical to elucidating the cosmic processes at work in this extreme environment.
Cosmic ray protons produced by the PeVatron interact with the dense ambient gas, traveling faster than 99 percent of the speed of light, and causing ultra-high-energy gamma rays.
However, the exact nature of the PeVatrons remains a mystery.
By analyzing the time distribution of the detected particles, the researchers were able to infer their energy density and identify the particles as ultra-high-energy gamma rays.
“Many of these processes are related to each other,” Harding said. “They are so rare that you wouldn’t expect them to happen in our galaxy, or they would happen on scales that don’t correlate to the size of our galaxy. For example, a black hole eating another black hole is an event that is only expected outside our galaxy,” he said.
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