Astronomy - USA (2020-05)

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investigate our universe. But so far, these


problems have proven to be remarkably


stubborn and persistent. With the goal of


identifying the individual particles that


make up dark matter, scientists have


designed and built a series of impressive


experiments — yet no such particles


have appeared. Even powerful particle


accelerators like the Large Hadron


Collider have revealed nothing that


moves us closer to resolving any of these


cosmic mysteries. And despite having


measured the expansion history and


large-scale structure of the universe in


ever increasing detail, we have not


gained any substantively greater under-


standing of the nature of dark energy,


the force that seems to be accelerating
the expansion of the cosmos.
It is from this perspective that some
cosmologists have found themselves ask-
ing whether these cosmic mysteries
might be symptoms of something more
significant than a few loose threads.
Perhaps these puzzles are not as unre-
lated as they might seem, but are instead
collectively pointing us toward a very
different picture of our universe and its
earliest moments.

What we’ve learned by not
discovering dark matter
Dark matter is likely the most celebrated
problem facing modern cosmologists.
Astronomers have determined that most
of the matter in our universe does not
consist of atoms or any other known
substances, but of something else —
something that does not appreciably
radiate, ref lect, or absorb light.
Despite not knowing much about the
nature of dark matter, cosmologists often

TOP: This galaxy cluster, nicknamed El Gordo (Spanish for “The Fat One”), ranks as the largest known cluster
in the distant universe. Composed of two individual clusters colliding at more than 1 million mph (1.6 million
km/h), this structure holds a mass equivalent to 3 quadrillion Suns. ESA/HUBBLE & NASA/RELICS

ABOVE: The blue color added to this image maps the distribution of dark matter in the El Gordo galaxy
cluster. Astronomers traced the presence of this shadowy substance by looking at how it distorts the
appearance of more distant objects. NASA/ESA/J. JEE (UNIVERSITY OF CALIFORNIA, RIVERSIDE)
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