We’ve devised all sorts of ways of looking for it but still have found nothing.

In April of 2019 though, a team analyzing data from a dark matter detector called XENON1T

announced it had witnessed something extraordinarily rare.

XENON1T was an experiment that’s pretty much what it sounds like:

an absolutely enormous tank filled mostly with the element xenon

cooled to -96 degrees Celsius.

While the vat contained 3.2 metric tons of liquid xenon, the experiment had a targeted

exposure rate of 1 metric ton per year, hence the 1T in the name.

What were they trying to expose the xenon to?

Dark matter, obviously, but specifically one favorite candidate for what dark matter could

be called Weakly Interacting Massive Particles, or WIMPs.

WIMPs are thought to be heavy, slow-moving particles.

As the name would suggest, these hypothetical particles don’t interact with normal matter

much,

even though about a billion of them are predicted to pass through each square meter on Earth

every second.

So the hope is that while watching a gigantic tank of xenon very closely,

a WIMP will collide with an atom, transfer some energy to the atom’s nucleus, and in

turn will excite other xenon atoms.

The process will release faint signals of ultraviolet light and trace amounts of electrical

charge

which can be detected by sensors at the top and bottom of the tank.

To make sure the experiment was isolated from sources that could cause false signals like

cosmic rays, the xenon was about 1,400 meters beneath a mountain in Italy.

Then just to be safe, the detector was shielded inside a tank of water nearly three stories

tall.

Once the experiment was set up, it was allowed to run “blind,”

meaning the scientists couldn’t access the data of interest until the analysis was done.

Now the results are in.

If you couldn’t tell by the fact that I’m not wearing my “We Detected Dark Matter”

party hat, we didn’t detect any dark matter.

XENON1T collected data from 2016 to December of 2018 without a whiff of a WIMP.

But this experiment wasn’t a failure.

In fact, it saw something that had never been seen before.

There are nine isotopes of xenon, and one in every thousand is xenon-124.

Xenon-124 was thought to be relatively stable, but would still decay into Tellurium-124 by

a rare process called two-neutrino double electron capture.

This occurs when two protons in the nucleus simultaneously grab two electrons from the

nearest shell, turning into neutrons and releasing two neutrinos.

As electrons in higher shells cascade down to fill the holes that have been created,

they give off X-rays and also free up other surrounding electrons.

However, these telltale signs are very hard to detect as they can be masked by background

radiation.

So before we could measure it, the half-life of xenon-124—that is, the time it takes

for half the xenon-124 in a sample to decay to tellurium—was thought to be about 160

trillion years.

XENON1T was designed to be extremely sensitive and isolated from background sources,

and after pouring over the data, the scientists noticed 126 instances where the detectors

picked up signals that matched those expected by xenon-124’s double electron capture.

These instances allowed them to calculate how long xenon-124’s half life actually

is.

Are you ready?

Because it’s a big number.

Xenon-124’s half life is actually 18 sextillion years.

Thats 18 with 21 zeros after it, over a trillion times longer than the current age of the universe.

That’s the longest half life we’ve ever directly measured, over now second place bismuth

209’s 19 quintillion years.

While XENON1T didn’t spot a WIMP, the team is excited by the discovery of their record-setting

half life.

It’s not only a feather in their cap, but a demonstration of just how sensitive their

instrument is.

They’re not giving up either: an even bigger tank of about 8 metric tons of xenon is being

built.

While another consolation prize, like the even rarer decay of the isotope xenon-136

would be nice, I’m sure the team is really holding out for the sign of a Dark Matter

interaction, and you can bet I’ll have my party hat ready if it happens.

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Experiments with Xenon aren’t the only way we’re looking for the missing mass of the

universe.

Check out this video on How Close We Are to Finding Dark Matter.

Make sure you subscribe to Seeker to know when we peer even further down into the details

of the universe, and as always, thanks for watching.