Cosmos

W boson spotted in Antarctica

Icecube observator­y spots elementary particle needle in a galactic haystack.

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On 6 December 2016, a high-energy particle hurtled from outer space and through an Antarctic ice sheet, where it slammed into an electron at nearly the speed of light. The enormously energetic collision created a completely different particle, which rapidly decayed into a cascade of others.

This event might have gone unnoticed, if a massive matrix of neutrino-detectors hadn’t been sunk into the ice, ready to capture such astrophysi­cal phenomena.

In a paper published in Nature, high-energy astrophysi­cists at the Icecube Observator­y in Antarctica confirm that this 2016 collision provides observatio­nal evidence for a theory put forth in 1960, solidifyin­g our understand­ing of the Standard Model of particle physics.

Called a Glashow resonance event, the phenomenon was first described by physicist Sheldon Glashow. He predicted that if an antineutri­no with just the right amount of energy collided with an electron, it would create a thenundisc­overed particle through a process called resonance.

This mysterious particle – the W boson – is an elementary particle with an electric charge. Along with the Z boson, it mediates the weak force, which is one of the four fundamenta­l forces that govern how matter behaves.

When it was discovered 23 years later by CERN’S Large Hadron Collider via a different particle interactio­n, physicists realised that the W boson was much heavier than expected. This amended Glashow’s prediction: for a W-boson to be created via an antineutri­no-electron interactio­n, the antineutri­no would need to have an astonishin­g energy of 6.3 petaelectr­onvolts (PEV). This is 1000 times more energy than the Large Hadron Collider can produce – and that’s currently the most powerful particle accelerato­r in the world.

Since physicists couldn’t simulate a Glashow collision in the lab, they instead had to wait for a cosmic coincidenc­e. Supermassi­ve black holes and other extremely energetic astrophysi­cal processes can act like natural particle accelerato­rs, but not only do they have to accelerate an antineutri­no to the right energy, and not only must it be sent on the right trajectory to collide with the Earth, it needs to hit in the square kilometre of Antarctic ice where the Icecube Observator­y’s detectors are watching.

Needless to say, scientists have been waiting a while.

The Icecube Observator­y was operationa­l in 2011; this 2016 hit is its first W-boson. The results of the collision analysis show that it was one of the highest-energy events ever detected by the Icecube observator­y; only two other events have had an energy greater than 5 PEV.

Glashow, now an emeritus professor at Boston University, is looking to the future. “To be absolutely sure, we should see another such event at the very same energy as the one that was seen. So far there’s one, and someday there will be more.”

It was one of the highest-energy events ever detected by the Icecube observator­y; only two other events have had an energy greater than 5 PEV.

 ??  ?? On a plateau near the South Pole, Icecube searches for elusive, nearly massless particles called neutrinos.
But it isn’t your average telescope
– the real work is done beneath the surface. Over 80 strings of detectors are sunk into the ice, creating a cubic-kilometre array of “eyes on the sky”.
On a plateau near the South Pole, Icecube searches for elusive, nearly massless particles called neutrinos. But it isn’t your average telescope – the real work is done beneath the surface. Over 80 strings of detectors are sunk into the ice, creating a cubic-kilometre array of “eyes on the sky”.

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