The proof is out there: extragalactic origins for cosmic rays

After nearly 50 years, researchers show the highest-energy cosmic rays have extragalactic origins.
By | Published: September 25, 2017
High-energy cosmic rays that make it to Earth strike molecules in our atmosphere, causing a cascading reaction that percolates downward until thousands of particles reach the ground.
A. Chantelauze, S. Staffi, L. Bret
Last week, an international team of over 400 researchers from 18 nations finally confirmed that high-energy cosmic rays are not coming from inside the Milky Way Galaxy, but instead from somewhere beyond.

In the study, published September 22 in the journal Science, the researchers gathered over ten years of data taken with the Pierre Auger Observatory to determine whether high-energy cosmic rays were hitting Earth equally from all directions. They are not.

Instead, the researchers found an overabundance of cosmic rays arriving from one specific region in the sky, located about 120 degrees away from our galactic center, in a direction that falls outside the Milky Way’s disk and cannot be associated with any possible sources within the galaxy. The researchers concluded that high-energy cosmic rays must have extragalactic origins.

This sky map shows the flux of high-energy (E ≥ 8 EeV) cosmic rays used for this study. The cross marks the source of the cosmic rays, while the circles denote the 68% and 95% confidence level regions.
The Pierre Auger Collaboration.
High-energy cosmic rays, which scientists have known about for over 50 years, are like tiny space bullets made of charged particles, ranging from single protons to heavy atomic nuclei like iron. They are extremely energetic and can travel vast distances through the cosmos at nearly the speed of light before reaching Earth.

Identifying cosmic ray properties can help astronomers infer important information about the processes that occur within our galaxy and the universe as a whole, including the events that generate them and the structures they travel through to reach us. While lower-energy cosmic rays come from inside the Milky Way — including from our Sun, clusters of stars, and supernova events — the highest-energy cosmic rays have long been believed to originate outside our galaxy.

For the study, researchers concentrated their efforts on cosmic rays with energies over 8 x 1019 electron volts — which is a million times more energy than the Large Hadron Collider (LHC) pumps into a proton, or about as much energy as it takes to lift a laptop one foot above a table.

When a high-energy cosmic ray reaches Earth, it can strike and obliterate any unlucky molecule hanging out in our upper atmosphere. This initial collision starts a devastating chain reaction that cascades down through the atmosphere, ripping apart other molecules, producing what is known as an air shower. These air showers balloon out as they descend downward, and by the time they reach the ground, they can cover an area up to 10,000 acres (40 square kilometers) and contain over 10 billion secondary particles — such as electrons, photons, and muons.

The Pierre Auger Observatory, located in the Argentinian Pampas, does not detect cosmic rays directly. Instead, it observes the secondary particles from air showers using a massive array of over 1,600 individual detectors spanning nearly 1,200 square miles (3,000 square km).

Over 1,600 simple but effective detectors make up the Pierre Auger Observatory. As secondary particles from air showers travel through the water-filled tanks, the Cherenkov effect produces flashes of light.
Céline ANAYA-GAUTIER/CNRS Photothéque
Each detector, spaced about a mile apart, is filled with 12 tons of pure water to help detect cosmic ray events. By analyzing how the arrival times of secondary particles differ between various detectors, researchers can trace the air shower up through the atmosphere and roughly pinpoint where the initial cosmic ray particle originated.

Using a sample of 30,000 high-energy cosmic ray detections, the team found a broad region of the sky where the flux — or inflow of cosmic rays — was 6 percent higher than average. And that region lies outside the Milky Way’s disk.

Though a few percent may not seem like much, there is only a one in five million chance that the increase in flux observed was due to chance.

Unfortunately, the study was unable to pinpoint the precise location of the cosmic ray source. This is partly due to the fact that numerous galaxies crowd the broad region of sky where the increase was found, and partly because cosmic rays can be deflected by the Milky Way’s own magnetic field, which makes them extremely difficult to trace back through space.

Fortunately, the more energy a cosmic ray has, the less it is deflected by a magnetic field, so by studying ultra-high-energy cosmic rays, researchers should be able to constrain the location of the source even further. And by ultimately discovering the source of high-energy cosmic rays, astronomers hope to learn both where exactly they come from, and how they are generated with such great energies.