New research suggests an unseen ‘mirror world’ of particles that interacts with our world only via gravity that might be the key to solving a major puzzle in cosmology today — the Hubble constant problem.
The Hubble constant is the rate of
expansion of the universe today. Predictions for this rate — from cosmology’s
standard model — are significantly slower than the rate found by our most
precise local measurements. This discrepancy is one that many cosmologists have
been trying to solve by changing our current cosmological model. The challenge
is to do so without ruining the agreement between standard model predictions
and many other cosmological phenomena, such as the cosmic microwave background.
Determining whether such a cosmological scenario exists is the question that
researchers, including Francis-Yan Cyr-Racine, assistant professor in the
Department of Physics and Astronomy at The University of New Mexico, Fei Ge and
Lloyd Knox at the University of California, Davis have been trying to answer.
According to NASA, cosmology is the
scientific study of the large-scale properties of the universe as a whole.
Cosmologists study concepts such as dark matter, and dark energy and whether
there is one universe or many, sometimes called a multiverse. Cosmology entails
the entire universe from birth to death with mysteries and intrigue at every
turn.
Now, Cyr-Racine, Ge, and Knox have
discovered a previously unnoticed mathematical property of cosmological models
which could, in principle, allow for a faster expansion rate while hardly
changing the most precisely tested other predictions of the standard
cosmological model. They found that a uniform scaling of the gravitational
free-fall rates and photon-electron scattering rate leaves most dimensionless
cosmological observables nearly invariant.
“Basically, we point out that a lot of
the observations we do in cosmology have an inherent symmetry under rescaling
the universe as a whole. This might provide a way to understand why there
appears to be a discrepancy between different measurements of the Universe’s
expansion rate.”
The research, titled “Symmetry of
Cosmological Observables, a Mirror World Dark Sector, and the Hubble Constant”
was published recently in Physical Review Letters.
This result opens a new approach to
reconciling cosmic microwave background and large-scale structure observations
with high values of the Hubble constant H0: Find a cosmological model in which
the scaling transformation can be realized without violating any measurements
of quantities not protected by the symmetry. This work has opened a new path
toward resolving what has proved to be a challenging problem. Further model
building might bring consistency with the two constraints not yet satisfied:
the inferred primordial abundances of deuterium and helium.
If the universe is somehow exploiting
this symmetry researchers are led to an extremely interesting conclusion: that
there exists a mirror universe very similar to ours but invisible to us except
through gravitational impact on our world. Such “mirror world” dark sector
would allow for an effective scaling of the gravitational free-fall rates while
respecting the precisely measured mean photon density today.
“In practice, this scaling symmetry
could only be realized by including a mirror world in the model — a parallel
universe with new particles that are all copies of known particles,” said
Cyr-Racine. “The mirror world idea first arose in the 1990s but has not
previously been recognized as a potential solution to the Hubble constant problem.
“This might seem crazy at face value,
but such mirror worlds have a large physics literature in a completely
different context since they can help solve important problem in particle
physics,” explains Cyr-Racine. “Our work allows us to link, for the first time,
this large literature to an important problem in cosmology.”
In addition to searching for missing
ingredients in our current cosmological model, researchers are also wondering
whether this Hubble constant discrepancy could be caused in part by measurement
errors. While it remains a possibility, it is important to note that the
discrepancy has become more and more significant as higher quality data have
been included in the analyses, suggesting that the data might not be at fault.
“It went from two and a half Sigma, to
three, and three and a half to four Sigma. By now, we are pretty much at the
five-Sigma level,” said Cyr-Racine. “That’s the key number which makes this a
real problem because you have two measurements of the same thing, which if you
have a consistent picture of the universe should just be completely consistent
with each other, but they differ by a very statistically significant amount.”
“That’s the premise here and we’ve been thinking about what could be causing that and why are these measurements discrepant? So that’s a big problem for cosmology. We just don’t seem to understand what the universe is doing today.”
Source: https://news.unm.edu/news/ghostly-mirror-world-might-be-cause-of-cosmic-controversy
Journal article: https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.128.201301
Photo by Mike Zeng for Quanta Magazine
Source: Ghostly
‘mirror world’ might be cause of cosmic controversy – Scents of Science
(myfusimotors.com)
No comments:
Post a Comment