Dark matter is a ghostly substance that astronomers have failed to detect for decades, yet which we know has an enormous influence on normal matter in the universe, such as stars and galaxies. Through the massive gravitational pull it exerts on galaxies, it spins them up, gives them an extra push along their orbits, or even rips them apart.
Author
Andreea Font
Reader in Theoretical Astrophysics, Liverpool John Moores University
Like a cosmic carnival mirror, it also bends the light from distant objects to create distorted or multiple images, a process which is called .
And suggests it may create even more drama than this, by producing stars that explode.
For all the havoc it plays with galaxies, not much is known about whether dark matter can interact with itself, other than through gravity. If it experiences other forces, they must be very weak, otherwise they would have been measured.
A possible candidate for a dark matter particle, made up of a hypothetical class of weakly interacting massive particles (or ), has been studied intensely, so far with no observational evidence.
Recently, other types of particles, also weakly interacting but extremely light, have become the focus of attention. These particles, called , were first to , but they may also fit the bill for dark matter.
Unlike WIMPs, which cannot “stick” together to form small objects, axions can do so. Because they are so light, a huge number of axions would have to account for all the dark matter, which means they would have to be crammed together. But because they are a type of subatomic particle known as a , they don’t mind.
In fact, calculations show axions could be packed so closely that they start behaving strangely – collectively acting like a wave – according to the rules of quantum mechanics, the theory which governs the microworld of atoms and particles. This state is called a , and it may, unexpectedly, of their own.
This would happen when the wave moves on its own, forming what physicists call a “soliton”, which is a localised lump of energy that can move without being distorted or dispersed. This is often seen on Earth in vortexes and whirlpools, or the bubble rings that .
The provides calculations which show that such solitons would end up growing in size, becoming a star, similar in size to, or larger than, a normal star. But finally, they become unstable and explode.
The energy released from one such explosion (dubbed a “bosenova”) would rival that of a supernova (an exploding normal star). Given that dark matter far outweighs the visible matter in the universe, this would surely leave a sign in our observations of the sky. We have yet to find such scars, but the new study gives us something to look for.
An observational test
The say that the surrounding gas, made of normal matter, would absorb this extra energy from the explosion and emit some of it back. Since most of this gas is made of hydrogen, we know this light should be in radio frequencies.
Excitingly, future observations with the radio telescope may be able to pick it up.
So, while the fireworks from dark star explosions may be hidden from our view, we might be able to find their aftermath in the visible matter. What’s great about this is that such a discovery would help us work out what dark matter is actually made of – in this case, most likely axions.
What if observations will not detect the predicted signal? That probably won’t rule out this theory completely, as other “axion-like” particles are still possible. A failure of detection may indicate, however, that the masses of these particles are very different, or that they do not couple with radiation as strongly as we thought.
In fact, this has happened before. Originally, it was thought that axions would couple so strongly that they would be able to . But since models of star cooling showed stars were just fine without this mechanism, the axion coupling strength had to be lower than originally assumed.
Of course, there is no guarantee that dark matter is made of axions. WIMPs are still contenders in this race, and .
Incidentally, some studies suggest that WIMP-like dark matter . In this case, the stars would still be normal (made of hydrogen and helium), with dark matter just powering them.
These WIMP-powered dark stars are predicted to be supermassive and to live only for a short time in the early universe. But they could be observed by the James Webb space telescope. A recent study has claimed , although the jury is still out on whether that’s really the case.
Nevertheless, the excitement about axions is growing, and there are many plans to detect them. For example, axions are expected when they pass through a magnetic field, so observations of photons with a certain energy are targeting stars with magnetic fields, such as neutron stars, or even .
On the theoretical front, there are efforts to refine the predictions for what the universe would look like with different types of dark matter. For example, axions may be distinguished from WIMPs through gravitational lensing.
With better observations and theory, we are hoping that the mystery of dark matter will soon be unlocked.
Andreea Font does not work for, consult, own shares in or receive funding from any company or organisation that would benefit from this article, and has disclosed no relevant affiliations beyond their academic appointment.
