Our crooked world lies one of science’s greatest unsolved mysteries. Where is all the dark matter? what or what Is all matter dark?
I mean, we know it’s there.
Galaxies, including the Milky Way, rotate so fast that our physics predicts that everything inside should be tossed out like horses in a choppy merry-go-round. But it is clear that this is not happening. You, me, the sun and the earth are held securely together. Therefore, scientists hypothesize that something – perhaps in the form of a halo – must surround the galaxies to keep them from collapsing.
Everything that includes these boundaries is called dark matter. We can’t see it, we don’t feel it, and we don’t even know if it is one thing. It is an elusive example. We only know that dark matter exists.
Despite our inability to view or touch the matter itself, experts have intriguing ways to determine the effects it has on our universe. After all, we infer the existence of dark matter primarily by observing how it holds together between galaxies.
Scientists have taken advantage of this principle, and announced fascinating new findings about dark matter on Monday. Using an instrument cluster made up of warped space, cosmic remnants from the Big Bang and powerful astronomy tools, they discover a deep space region of previously unstudied dark matter halos – each located around an ancient galaxy, faithfully protecting it from living in a terrifying nightmare fun. .
These vortices, according to a study on the discovery published in Physical Review Letters, go way back 12 billion years, just under two billion years after the Big Bang. This could make it the smallest dark matter episode that humanity has ever studied, the authors suggest, and possibly a precursor to the next chapter in cosmology.
“I was glad that we opened a new window into that era,” Hironao Miyake of Nagoya University and an author of the study said in a statement. “12 billion years ago, things were very different. You see more galaxies that are forming than they are now; the first galaxy clusters are starting to form as well.”
Wait, distorted space? cosmic relic?
Yes, you read correctly. Let’s explain.
More than a century ago, when Albert Einstein formulated his famous theory of general relativity, one of the predictions he made was that ultra-strong gravitational fields generated by massive amounts of matter would twist the fabric of space and time, or spacetime. It turns out he was right. Today, physicists are taking advantage of this concept by invoking a technique called gravitational lensing to study very distant galaxies and other phenomena in the universe. It does something like this.
Imagine two galaxies. Galaxy A in the background and B in the foreground.
Basically, when light from galaxy A passes through galaxy B to reach your eyes, that luminescence is distorted by B material, whether it’s dark or not. This is good news for scientists, because often such distortion grow up Distant galaxies are kind of like a lens.
Moreover, there is a kind of inverse calculation that you can do with this light twist to figure out how much dark matter surrounds galaxy B. Many From dark matter, you will see a Many More distortion than expected from the visible matter – the things we can see – within. But if it didn’t contain that much dark matter, the distortion would be much closer to your prediction. This system worked well, but there is a caveat.
A standard gravitational lens only allows researchers to identify dark matter around galaxies that are approximately 8 billion to 10 billion light-years away, maximum.
This is because as you look deeper and deeper into the universe, visible light becomes harder and harder to interpret, and eventually turns into infrared light that is completely invisible to the human eye. (For thisThis is a big deal. It’s our best shot at capturing the faintest, invisible light from the distant universe.) But what this means is that visible-light distortion signals for dark matter studies become too faint after a certain point to help us analyze hidden objects.
Miyatake came up with an alternative solution.
We probably can’t observe the standard light distortions of dark matter detection, but what if there was another type of distortion we could see? As it turns out, there is: microwave radiation from the Big Bang. It’s largely a Big Bang heat remnant, formally known as the cosmic microwave background radiation, or CMB radiation.
“Look at the dark matter around distant galaxies?” Masami Oshi, a cosmologist at the University of Tokyo and co-author of the study, said in a statement. “It was a crazy idea. Nobody realized we could do this. But after I gave a talk about a large, distant galaxy sample, Hironao came to me and said it might be possible to look at the dark matter around these galaxies using the CMB.”
In essence, Miyatake wanted to note how dark matter is the gravitational lensing of the first light of our universe.
Capture parts of the Big Bang
“Most researchers use source galaxies to measure the distribution of dark matter from the present to 8 billion years ago,” Yuichi Harikan, associate professor at the University of Tokyo and co-author of the study, said in a statement. “However, we can look further into the past because we used the farthest CMB to measure dark matter. For the first time, we’ve been measuring dark matter from roughly the very first moments of the universe.”
To arrive at their findings, the new study team first collected data from observations taken by the Subaru Hyper Suprime-Cam Survey.
This led them to identify 1.5 million lensed galaxies – a group of hypothetical B galaxies – that can be traced back 12 billion years ago. Then they requested information from the European Space Agency’s Planck satellite about Big Bang microwave radiation. Put it all together, and the team can see if and how these lenticular galaxies have distorted microwaves.
“This result gives a very consistent picture of galaxies and their evolution, as well as the dark matter in and around galaxies, and how this picture evolves over time,” Nita Bahkal, professor of astrophysics at Princeton University and co-author of the study said in a statement.
Notably, the researchers stressed that their study found that dark matter from the early universe does not appear as lumpy as our current physical models suggest. Ultimately, this part could modify what we currently think about cosmology, especially theories rooted in the so-called Lambda-CDM model.
“What we found is still uncertain,” Miyatake said. “But if true, it would suggest that the entire model is flawed as you go back in time. This is exciting because if the result persists after the uncertainties are reduced, it could indicate an improvement to the model that may provide insight into the nature of dark matter itself.”
Next, the study team wants to explore past regions of space by taking advantage of information held by Vera C. Rubin’s Legacy Survey of Space and Time.
“LSST will allow us to see half the sky,” Harrikan said. “I see no reason why we couldn’t see the distribution of dark matter 13 billion years ago.”