A breakthrough in the study of ghostly particles called high-energy neutrinos that traverse space, zipping unimpeded through people, planets and whole galaxies, is giving scientists an audacious new way to expand our understanding of the cosmos.
An international team of researchers, including five Canadians, said Thursday they have for the first time located a deep-space source for these ubiquitous subatomic particles.
They detected high-energy neutrinos in pristine ice deep below Antarctica’s surface, then traced their source back to a giant elliptical galaxy with a massive, rapidly spinning black hole at its core, called a blazar, located 3.7 billion light years from Earth in the Orion constellation.
Astronomers long have relied on electromagnetic observations - studying light - but this approach has limitations because too many aspects of the universe are indecipherable using light alone.
The ability to use particles such as high-energy neutrinos in astronomy enables a more robust examination, much as the confirmation of ripples in the fabric of space-time called gravitational waves, announced in 2016, opened another new frontier in astronomy. This emerging field is dubbed “multi-messenger astrophysics.”
“It’s like sitting down to a good meal,” said University of Alberta astronomer Greg Sivakoff, who was involved in the discovery. “A good dish will look good, smell good, feel good and the taste will be good. A good meal will engage all of your senses. Multimessenger astronomy is the beginning of us sitting down to the meal and doing more than just looking at it. We’re beginning to have more than one sense.”
The key observations were made at the IceCube Neutrino Observatory at a U.S. scientific research station at the South Pole and then confirmed by land-based and orbiting telescopes.
The findings solve a mystery dating to 1912 over the source of subatomic particles like neutrinos and cosmic rays that dash through the cosmos. It appears they arise from some of the universe’s most violent locales.
“One hundred billion neutrinos go through your thumbnail every second, but in all likelihood not a single one of them will ever hit an atom of your thumb in your lifetime,” said Penn State physicist Doug Cowen, another of the researchers. “It is accurate to say that we are all swimming in neutrinos.”
High-energy neutrinos are produced by the same sources as cosmic rays, the highest-energy particles ever observed, but differ in a key respect, said University of Wisconsin physicist and IceCube Neutrino Observatory lead scientist Francis Halzen.
As charged particles, cosmic rays cannot be traced straight back to their source because strong magnetic fields in space alter their trajectory.
Neutrinos are electrically neutral, undisturbed by even the strongest magnetic field, and rarely interact with matter, earning the nickname “ghost particle.” The direction from which they arrive points directly back to their original source.
The IceCube neutrino detector involves 86 holes drilled 2,500 metres into the Antarctic ice. Some 5,160 light sensors register small flashes of light produced during rare instances when a neutrino collides with an atomic nucleus in the transparent ice. The key detection came on Sept. 22, 2017, with the neutrino ultimately traced back to the blazar.
Scientists then determined that other neutrinos earlier detected by IceCube originated from the same source.
“In many ways neutrinos are nature’s ideal astronomical messenger,” said University of Alberta physicist Darren Grant, spokesman for the IceCube scientific collaboration. “They can essentially escape their site of production and bring that information directly across the cosmos to their point of detection.”
Not all neutrinos are the high-energy variety. Lower-energy neutrinos, for example, are produced prolifically in the fusion processes of stars like our sun.
Blazars are probably not the only sources for high-energy neutrinos or high-energy cosmic rays, Prof. Grant said, mentioning other objects and phenomena like galactic nuclei, quasars, gamma ray bursts and some types of stellar explosions called supernovas.
The U.S. National Science Foundation-supported research was published in the journal Science.