Recent research suggests that the observed expansion of the universe may be in part dominant by the fact that we live in a relatively under dense region of the universe. This video explores the consequences of these findings. See my interview with David Wiltshire for more information. 
What if the key to understanding one of
the biggest mysteries in cosmology lies
in nothing? Literally, the vast expanses
of empty space between galaxies. Recent
research has proposed that a gigantic
void, a region of under dense matter in
our local universe, could be causing the
expansion rate of the cosmos to appear
faster than expected from observations
of the cosmic microwave background
radiation or CMB. Now the CMBB is how
the bread gets buttered around the Keing
household. So this discrepancy known as
the Hubble tension is of particular
importance to me and my cosmologist
friends. It's been a thorn in our sides
for more than a decade now.
What is the Hubble tension? It revolves
around the famous Hubble constant which
is a measurement of how fast the
universe is expanding. We can calculate
this rate using two primary methods.
observations of the cosmic microwave
background which originated from the
formation of hydrogen 380,000 years
after the big bang and the second method
are measurements of type 1A supernova
bright exploding stars in the relatively
modern local universe the problem is
these two different methods give
conflicting results for the value of the
Hubble constant the difference may seem
small about 9% but it's a huge deal in
cosmology because each methodology has
about a 1% % chance of being a fluke,
meaning that these things don't agree at
over the five sigma level. Now, this
reminds me of what many parents get to
experience when their kid is about 2
years old. When you take your child to
the pediatrician at age two, the
pediatrician measures their height and
their weight. And from their height at
age two, they can basically predict,
usually they just double it, but they
predict based on millions or billions of
samples, namely every human being that's
ever been measured in this way, how tall
they'll be at the end of their life or
when they finish growing. And so it be
as if using the baby method, we got a
very different method than if you
measured a kid right before he or she
was done with puberty, local more
recently, and those two values disagreed
wildly. They were off by almost a foot
in some cases. This would be quite
startling.
Now enter the void hypothesis as a
method of explaining and resolving the
Hubble tension. A team of researchers
has found that the massive underdense
region called the Kenan Barger Kawi or
KBC void which stretches across some 700
million lighty years could be
responsible for the Hubble tension. The
model that is being proposed shows that
continuous outflows of matter from this
vast void region towards us could make
the expansion rate appear faster in our
local patch of the universe compared to
the cosmic average from the early
universe. It's like being on a rowboat
on a river. The flow of the river makes
it seem like you're moving faster
relative to the river banks when you add
it to the velocity of your canoe. So,
what evidence and what are the
implications for this hypothesis?
Remarkably, this local void model can
explain both the higher local Hubble
constant values and the observed bulk
motions of galaxies streaming away from
the void without needing to tweak any
parameters precisely. If confirmed, this
could mean we don't necessarily need to
modify our theories of gravity or cosmic
expansion. Those would be more exotic
explanations that would require new
physics. This is good old-fashioned
ordinary galactic physics, the kind that
we've been practicing for literally a
hundred years now and understand quite
well. The effect arises from the
inhomogeneous distribution of matter in
our universe. We're in a sort of special
part of the universe that's not exactly
representative of the entirety of the
universe as a whole. However, the model
depends on a specific void profile
assumed, and it may not account for
interactions with other large scale
structures beyond the local void. There
are also open questions about the scale
of such voids and its impacts on
previously measured data.
Now, are there any other competing
solutions? Why yes, the local void
hypothesis isn't the only game in town
for resolving the Hubble tension. Other
proposed solutions include so-called
early dark energy models that affect the
early expansion rate of the universe in
a way that's very different than the
later expansion rate that we're
experiencing now. There are theories of
modified Newtonian dynamics called man
that change gravity that could cause a
variation of the Hubble constant from
age zero basically to age much later.
The influence of primordial magnetic
fields on the cosmic microwave
background has also been proposed as a
solution to the Hubble tension. Each of
these solutions has its own strengths
and the predictions to be tested against
future observations. So what's the
cosmic perspective in all this?
What this really highlights is that the
vast emptiness of space can have a
profound consequence on our
understanding of the cosmos. The cosmic
model we've constructed may need
revisions to account for the complex
inhomogeneous structure of matter we
observe. Now, as we continue to probe
the depths of space with ever more
powerful telescopes like the James Webb
Space Telescope, the secrets of cosmic
voids and the true nature of the
universe's expansion may be finally
resolved. And this Hubble tension could
go away when astronomers like me will no
longer have anxiety nor need for special
psychotherapists because sometimes
studying the emptiness, the void and
screaming into it is the key to seeing
the bigger picture.
If you enjoyed this video, please click
on this video with my recent interview
with Wendy Freriedman, who also thinks
she may have found a solution involving
somewhat less exotic stars called Tip of
the Red Giant branch stars. And don't
forget to subscribe.