Small, dark and baffling: the top five dark matter candidates

April 24, 2018 by ​cristy Burne, Particle
Dark matter map of KiDS survey region (region G12). Credit: KiDS survey

What if the universe we know is just one runty part of a larger, mostly invisible universe, and the only way we can interact is via gravity?

This is just one of the ideas that physicists are pursuing in the quest to solve the mystery of dark .

I love the idea of dark matter. For me, it's the ultimate enigma. I mean, our universe contains protons and neutrons and electrons, and that's great. All this 'normal' matter is the basic ingredient for everything from Brad Pitt to intergalactic gas clouds. Normal matter also exerts a , and this is also great. Gravity stops my coffee from floating away and prevents galaxies from spinning apart.

Grave shortfall

But when you add up all the particles in all the galaxies in the universe, there just isn't enough to produce all the gravity in the universe. There's way too much gravitational force and way not enough matter.

For our universe to make sense, it needs a whole load of something extra to make up the gravitational shortfall.

That something extra turns out to be up to 80% of the matter in our universe. We call it 'dark' matter: particles we can't see and don't understand but that bring enough gravitational force to balance the books.

The hunt for missing matter

We've been searching for direct evidence of dark matter for years but found nothing. Not to worry: we knew it would be tricky. Researchers believe dark matter pretty much ignores normal matter and light.

"Dark matter particles could be everywhere around us, but they just don't interact electromagnetically," says Vid Iršič, a University of Washington researcher and dark matter expert. "They could only interact gravitationally."

Watch out! Neutrinos passing through

Though it sounds strange, there's already precedent for particles that don't play well with others. They're called .

"Neutrinos are very, very light particles that interact very weakly," says Vid. "They come from the stars. Neutrinos from our Sun pass through Earth in their billions every second, across every square centimetre."

These particles are passing through you right now, but their interactions are so mild you don't feel a thing. Yet neutrinos are like big brass bands compared to dark matter.

So what are dark matter particles?

There are loads of theories and experiments searching for many different particles in the race to solve the dark matter mystery. Below we outline Vid's personal top five , from most likely to least likely. Thinking caps on.

Candidate #1: Weakly interacting massive particles (or WIMPs)

Weakly interacting massive particle is a catch-all term for a bunch of particles that fit that description. 'Weakly interacting' means they don't interact much with normal matter or light. 'Massive' means they're larger than the mass of a proton.

WIMPs are popular because they've been independently predicted by a few different particle physics theories. And because of the WIMP miracle. The miracle is that these theories also predict the total mass of WIMPs, and it's approximately the same mass as that required to explain all the extra gravitational force. Coincidence? Perhaps not.

Candidate #2: Axions

Axions are a theoretical particle we dreamed up to solve an unsolved problem in quantum dynamics. Specifically, their existence would help explain quirks in our understanding of quarks and how they stick together to form protons and neutrons. But that's a whole different story …

If axions do exist, they'd also tick some dark matter boxes. They're predicted to interact only weakly with and light. And they'd be just the right size for us to have missed them (so far). (That size, in case you're wondering, is somewhere between 2 and 100 micro-electron-volts (and a micro-electron-volt is 1.78×10-42 kilograms).

Axions are also super-amazing. One axion decays into two photons. Plus you can make an axion by combining two photons. We're hoping this will help us detect them some time soon. In April, Vid's university announced it can now search more sensitively than ever before for signs of axion decay.

Candidate #3: Ultralight scalar dark matter

This candidate is a relatively new kid on the block. It's also known as ultralight axions, fuzzy dark matter or wave dark matter.

If it exists, it's super-duper light, something like 10-22 electron-volts. And because it's so light, it behaves in a way that suits string theory and quantum mechanics. The idea is that, when you get a whole galaxy-load of these particles together, they behave more like a wave than a spinning ball.

You end up with miniscule particles that combine into a wave that spans thousands of light years. No wonder they're tricky to find.

Candidate #4: Sterile neutrinos

Dark matter could also be a special form of neutrino, which is tricky, because neutrinos are already special. They come in different flavours (electron, muon and tau), and they can shift between flavours as they travel through space. Plus, they're minimally interactive and super-light.

Dark matter neutrinos, if they exist, are the neutrino's much heavier cousin. Called sterile neutrinos, they're predicted to interact with normal matter only when they flip between flavours.

Candidate #5: Self-interacting dark matter

This is an increasingly popular option. What if there isn't just one type of , but many?

Just as normal matter has a whole bunch of different particles, so too could dark matter. But because normal particles and dark particles don't interact much, we may never know. Perhaps the only way we could observe these particles would be indirectly, through their gravitational effect on the evolution of the cosmos. Thinking caps exploding.

"This is quite fascinating," says Vid, in what could just be the world's biggest understatement.

"More and more people believe that dark matter is not just one particle but a collection of particles, perhaps in a mirror image of the world we know. The standard that we know, but disconnected from us except for gravity and not interacting with us in any other way."

Invisible mystery

Will we ever discover what is really made of? Well, we're going to give it our best shot. Thousands of scientists around the world are searching for signs, trialling new ideas and developing mind-blowing technologies.

We used to think the world was flat. And that our universe was visible. What will the next decades bring?

Explore further: Crystals could help uncover mysteries of dark matter

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1 / 5 (2) Apr 24, 2018
'Scientists Thought All Galaxies Had Dark Matter, but They Just Found One Without It'

Dark matter fills 'empty' space, strongly interacts with visible matter and is displaced by visible matter.

The reason for the mistaken notion the galaxy is missing dark matter is that the galaxy is so diffuse that it doesn't displace the dark matter outward and away from it to the degree that the dark matter is able to push back and cause the stars far away from the galactic center to speed up.

It's not that there is no dark matter connected to and neighboring the visible matter. It's that the galaxy has not coalesced enough to displace the dark matter to such an extent that it forms a 'halo' around the galaxy.

A galaxy's halo is not a clump of dark matter traveling with the galaxy. A galaxy's halo is displaced dark matter.
not rated yet Apr 25, 2018
Cosmologists need to look if DM bends spacetime in the same way as matter for one - i.e. is the lensing effect convex or concave, which will tell us if its part of same universe at least and moving in the same direction.

If the lensing is opposite like I think it is, convex for normal matter and concave for DM it would show how the two dont interact as mass and DM repel each other and thats the main reason we have galaxies - the DM corals mass and compresses it, just because there is more of it.

DM is a mirror image of mass and light, negative entropy, negative time (relative to us, both forward relative to other DM). Made of exactly the same stuff, when all the stars are gone on our side DM will have its chance to expand (in its big bang) and the cycle will continue over and over - as our half of the universe colapses it provides the "dark energy" to pull the light from it. Irony is from the perspective of DM it is normal and we are the DM going backwards.
not rated yet Apr 25, 2018
...A galaxy's halo is displaced dark matter.
I'm not sure how it would be displaced except maybe through BB turbulence. Anyway it is a low density region of the dark energy. Which is what matter is, actually. Matter coming in two forms - quantized (particulate) and continuously distributed gradients in the dark energy density. The gravitational effect is the same under expansion. That is galaxies tend to form in low pressure regions of the dark energy. The acceleration of gravity is actually less inside galaxies because of the lower dark energy density. This is where most galaxies tend to form. If you want to see the curvature of spacetime you look at curves on surfaces of regions of similar dark energy density or similar gravitational acceleration.
not rated yet Apr 25, 2018 the lensing effect convex or concave,
Around regions of matter where the dark energy density is lower the speed of light slows down. That is it takes longer to get from point a to point b because the distance between point a and b is further when the dark energy density is lower. So a wave front approaching an object will be slowed down closer to the object causing it to bend in toward the object. Effectively the index of refraction around the object is higher so it appears as a convex lens. At least it seems that way.

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