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Scientists finally trace neutrinos to source

Elusive particles traveled nearly 4 billion light years

- By Amina Khan Los Angeles Times amina.khan@latimes.com

Using a neutrino detector made of Antarctic ice, astronomer­s have for the first time pinpointed the source of a handful of high-energy neutrinos from far beyond our galaxy: a powerful blazar shining like a beacon from nearly 4 billion lightyears away.

The extragalac­tic neutrinos and their origins, described in two papers in the journal Science, shed light on the century-old question of where cosmic rays come fromand offer the first clear proof of the potential for this nascent brand of astronomy.

“We are not going to solve high-energy astrophysi­cs in the oldfashion­ed way anymore,” said FrancisHal­zen, a particle astrophysi­cist at the University of Wisconsin, Madison and principal investigat­or for IceCube, the frozen observator­y that made the discovery.

Neutrinos are exceedingl­y tiny particles, weighing less than one ten-billionth the mass of a proton. Many billions of these subatomic particles pass through your fingertip every second. Even though they’re plentiful, neutrinos don’t interact much with matter, passing through planets, stars, even entire galaxies like speeding subatomic phantoms.

But astronomer­s hunt for neutrinos anyway, partly because they’ve suspected that they could solve the in Antarctica to create a neutrino detector. mystery of the origins of the cosmic rays that bombard Earth fromspace.

Cosmic rays are highly energetic charged particles, mostly protons, that have been revved up to enormous energies and hurled across the universe. It would take a powerful cosmic engine — say, a supermassi­ve black hole at a galaxy’s heart, or an enormous supernova— to accelerate these atomic fragments to such high energies.

But until now, scientists haven’t known for sure where these cosmic rays come from. That’s because as they travel intergalac­tic distances, their paths are warped by the magnetic fields that permeate space — which means that by the time they get to Earth, they’re no longer pointing back at their source.

Neutrinos offer a solution to thisproble­mbecause these neutral particles are unaffected by magnetic fields. By the time they reach Earth, they’re still pointing the way home. On top of that, the kinds of powerful cosmic forges that would generate high-energy cosmic rays also would produce a torrent of highenergy neutrinos.

But the very quality that makes these ghostly particles so useful— the fact that they don’t interact with matter— also makes neutrinos exceedingl­y difficult for scientists to catch in action. For every individual highenergy neutrino hit, Halzen said, roughly 10,000 or 100,000 more pass through unscathed.

The IceCube collaborat­ion set out to detect that rare, singular neutrino strike.

Composed of more than 5,000 sensors embedded in a cubic kilometer of ice sitting deep beneath the Antarctic surface, IceCube picks up the flashes of blue light caused by secondary particles after a neutrino makes contact. The scientists can analyze that resulting light track to tell what direction the particle came from and how energetic it was when it hit.

In 2013, the collaborat­ion announced it had found 28 high-energy neutrinos that had originated from deep space, but the groupwas not able to tell where exactly any of them came from.

Then, on Sept. 22, 2017, the scientists picked up an energetic neutrino that had clearly originated far outside our interstell­ar neighborho­od.

Gamma ray and X-ray telescopes turned toward the source, picking up a light signal across the electromag­netic spectrum. The light was coming from a blazar named TXS 0506+056, a giant elliptical galaxy with a black hole at the center that’s gobbling up material and shooting out twin beams of light on either side of its disk, one of which is pointed directly at Earth like the beam of a flashlight.

Still, there was a small chance— about 1 in 1,000— that the neutrino’s apparent origin and the blazar signal were mere coincidenc­e. So the researcher­s went back in the archives, looking for previous neutrino measuremen­ts that also could have come from the blazar’s direction.

Sure enough, the researcher­s found more than a dozen neutrinos from September 2014 to March 2015 that appeared to be coming from the direction of the blazar. Those results were published in a second paper in Science.

“In my opinion, this is as significan­t as the first steps in X-ray astronomy, which were awarded the Nobel Prize,” said Alexander Kusenko, a particle astrophysi­cist at UCLA who was not involved in the study.

Such neutrino discoverie­s could help astronomer­s to better understand the inner workings of these cosmic events, Kusenko said.

It also may allow scientists to see old events in a new light, Halzen said.

For one thing, it would have taken an extremely powerful source to push these particles to such high energies and then send them across nearly 4 billion light years, he pointed out.

“So there’s something special about this source,” Halzen said — something special thatwas not obvious from the blazar’s light profile and which will require further study to understand.

Already, he added, neutrino astronomy is revealing extraordin­ary events right in front of scientists’ eyes.

“In my opinion, this is as significan­t as the first steps in X-ray astronomy, which were awarded the Nobel Prize.”

— Alexander Kusenko, particle

astrophysi­cist, UCLA

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