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Wait, you're listening? Okay.
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Alright. Okay. Alright.
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You're listening to Radiolab. Radiolab.
0:41
From WNYC. See?
0:45
Yeah. What's
0:49
another word for a male frog
0:51
that has some children? What?
0:55
What's another word for a male frog that has
0:57
children? A daddy-wog. A dad-pole.
1:00
There you go! Yes! Okay,
1:02
sorry. I feel cash. Hey,
1:05
I'm Lulu. I'm Latif. This is Radiolab.
1:09
A host we are quite a big fan of. Allie, your show is awesome. It's
1:11
so great. Thank you. Her name
1:13
is Allie. She's a radio host. She's
1:15
a radio host. She's a radio host. She's a radio host.
1:17
She's a radio host. She's a radio host.
1:20
She's a radio host. She's a radio host. She's
1:22
a radio host. She's a radio host. So,
1:28
Allie Ward. I actually realized during our
1:30
conversation with her that she is my
1:32
neighbor. But we brought her in
1:34
because we wanted her to tell
1:36
you about her podcast.
1:38
So let the games begin. Ask me anything. What
1:41
is the name of your show and how would you describe
1:43
it? So Ologies is a
1:46
comedy-ish science podcast
1:48
where we explore a different ology
1:51
every episode. So it might be geology
1:53
one week and then a filamentology the
1:55
next, which is the study of kissing.
1:58
Allie has taken on. So
2:00
many ologies testudonology which
2:03
comes from the Latin testudo for
2:05
tortoise and a gmatology Hagfish
2:09
ology would it be raccoon ology
2:12
or would it be? meteorology
2:14
apiary ology
2:15
technology Melanin ology quantum
2:18
ontology chronobiology carnivorous
2:20
phytobiology flesh-eating plants
2:24
Your urology
2:26
episode was one of my favorites
2:29
and I did not think I would like I very
2:32
reluctantly clicked on that And
2:34
we brought Ali on because her show is
2:37
kind of like a kindred spirit
2:39
to our show But also
2:41
it's very different at the same time like for
2:43
our show we talked to a bunch of scientists but
2:46
it's usually in the context of a Story
2:49
or a big idea we're interested in and then
2:52
we try to make it all add up to something
2:54
Ali does not do that part She
2:57
just will be like oh this scientist is interesting
2:59
and then they will sit down and they will just
3:01
go to town and
3:02
Actually one of the things I love
3:05
about your show is like like
3:07
your what matters is totally different
3:09
than our what matters Like what
3:12
what does it matter when it's a random thing
3:14
that
3:14
that it seems like maybe only this one
3:17
Scientist you're talking to cares about I
3:19
love this question and I completely get it So
3:23
here's the thing science is everywhere
3:25
science is in How
3:27
you steam broccoli science is
3:30
in how you
3:31
park your car science is in who
3:33
you fall in love with science is why? You
3:36
sweat when you get a text message that freaks
3:38
you out like it's not just about
3:41
diagrams and textbooks and I think it's
3:43
also interesting that a lot of people
3:45
who are not scientists
3:48
think that scientists are jerks and
3:51
pedantic and are there with like a
3:53
huge book of facts to tell them that they're wrong about
3:55
things and I wanted to show that like scientists
3:57
are
3:58
curious little weirdos who found
4:01
their niche and whatever made
4:03
them passionate and they
4:05
make mistakes and they have hypotheses that
4:09
end up being wrong and they're
4:11
figuring it out too. And so humanizing scientists,
4:14
I feel like galvanizes people to care a
4:16
little bit more every time they see a research paper. They
4:19
think, I wonder why this person studied this or
4:21
I wonder how long it took to get this published.
4:23
And so the civic
4:25
duties that we have to protect things
4:28
and care about things become easier for people when
4:31
they have a little bit more context. But like,
4:32
okay, so like, how do you know how
4:34
to, that people will stay
4:37
with you for all of these, for your to
4:39
go down, like how far they'll follow you
4:41
before they'll just be like,
4:43
Ali just totally lost it. Lost
4:46
the plot. Yeah, lost the plot. Yeah, I
4:48
mean, it's really kind of more
4:50
of like a
4:52
lightning bug kind of darting around and just
4:55
following the light.
5:00
So for the rest of this episode of our show, we're
5:02
gonna follow Ali
5:05
into an episode of her show as she follows
5:07
the light bouncing around
5:09
like a little lightning bug like she does into
5:12
the dark. Oh, Scotto, high
5:14
lollogy Scotto means dark. High lollogy means matter.
5:17
We're gonna play her episode on dark matter for you. I
5:19
actually, that was a rare one where I worked with
5:22
theologists to be like, there needs to be a word for
5:24
this. How do you feel about this? And
5:26
he loved it. You coined a term. You coined
5:28
it. It's one of the very few conversations I've
5:31
heard that actually make dark matter
5:33
make sense to me. And even
5:35
feel like it matters. Yeah.
5:42
So we're gonna turn it over now to Ali with UC Riverside
5:45
theoretical
5:46
particle physicist and dark matter expert, Flip
5:48
T'Nato.
5:49
And just a quick heads up, the lovely Ali Ward
5:52
is not afraid to, dirty
5:55
her tongue. That's
5:58
not an expert.
5:59
She's not afraid to swear. So
6:03
there are a few swear words ahead. Here
6:06
we go.
6:07
Did you set out to become a theoretical
6:10
physicist? How does one land
6:12
in like what I feel like is the
6:15
hardest field possible?
6:16
All right. Here
6:18
is my origin story. I
6:22
wanted to be an author. Really? I
6:24
had no idea why, but I was
6:26
very passionate about writing
6:28
the idea that one can have a voice. And
6:31
so growing up, I was a huge
6:33
fan of LaVar Burton's because of Reading
6:35
Rainbow. Love, love, love, love. Reading
6:38
Rainbow, amazing. But you don't have
6:40
to take my word for it. So I
6:42
would watch Reading Rainbow
6:44
and at some point in the
6:46
back of my mind, I realized this person
6:48
who does Reading Rainbow is also on this TV show,
6:50
Star Trek. And
6:53
in high school, I started watching
6:55
Star Trek a little bit. It was still on at the time.
6:58
I picked up the book, The Physics of Star
7:00
Trek by Laurence Krauss.
7:02
And this was a really fun
7:04
ride because
7:06
it was the first time I thought about a scientific
7:08
subject
7:09
as something where there are open
7:11
questions and these open questions
7:13
are fun and creative and exciting
7:16
and any time that I lost track of it
7:18
being exciting, I just watch
7:19
LaVar Burton as Jodie LaForge as
7:22
a chief engineer. I know it well. Oh
7:24
my gosh. My sister and I used to watch The
7:27
Next Generation as well. It was the
7:29
best. Yeah. We can't change the gravitational
7:31
constant of the universe, but if we wrap a low-level
7:33
warp field around that moon, we could reduce its
7:36
gravitational constant. Make it lighter so
7:38
we can push it. So I think
7:40
that's what got me into this idea that, hey,
7:43
these black holes in the show, these are real. We
7:46
should understand these things. There are fundamental questions
7:49
that are not only abstract
7:52
and things you'd find in textbooks, but
7:55
they're fun ideas and it
7:57
was the creative spark that was really exciting.
7:59
could write a science fiction piece about
8:02
these actual things. And that's what got
8:04
me going with physics.
8:05
Do you write still at all? I
8:08
was never a great writer. And you can ask my collaborators
8:10
that my paper writing is slow and
8:13
tortuous. But I
8:15
would like to eventually write something
8:17
as a popular book.
8:18
Oh, yeah. I feel like that is in your future. But
8:21
when it comes to matter
8:24
and dark matter, I mean, slow
8:26
it way down for baby brains like mine.
8:29
But from what I understand, and the
8:31
first time I ever read this was like,
8:33
okay, all of the matter that we can see and
8:35
touch and feel and everything makes up about 15%.
8:39
Yeah, depending on how you're counting. But yeah, yeah, it's a
8:41
tiny fraction. Like a third
8:43
of that. So everything that you can
8:46
see and feel and touch
8:48
and smell, that's 5% of the universe's mass
8:53
and energy. There's another 95% of pure
8:55
mystery.
8:57
So
8:59
then what the fuck is everything else?
9:01
What is it? That
9:04
is the mind blowing thing. We've known
9:07
about dark matter indirectly for 100 years. And
9:09
I think it hasn't been until fairly recently
9:12
that this has come to the forefront of we really
9:14
ought to figure
9:14
out what this stuff is. Because
9:17
as you said, we spend all of our lives learning
9:21
science, art, history,
9:23
everything you learn from a textbook is basically
9:26
about that really tiny slice of
9:29
visible normal matter and
9:31
the history of that normal matter in this
9:33
universe and in this world and in our culture. But
9:36
it turns out for every, say,
9:38
what's the fraction? I think if
9:40
you look at the amount of energy, so energy
9:42
is a good
9:43
measure for stuff. 25% of
9:47
the universe is made of dark matter and
9:49
only 5% is made of the stuff
9:51
that we're used to. Wow. It's 5
9:53
times more dark matter than ordinary
9:56
stuff.
9:57
And in fact, it's so much more that...
10:00
We look at our galaxy and we think our galaxy is huge. Our
10:02
galaxy is almost everything. Everything we
10:04
possibly care about. Our galaxy
10:06
is only here because it is swimming
10:09
in an ocean of dark matter that provides a gravitational
10:11
pull to keep the galaxy there. The galaxy formed
10:14
because there was dark matter. So
10:17
where we are right now with Scotto-Hylology,
10:21
is that what we're doing? Yes. Nailed it. This
10:23
is the fish scientist discovering
10:25
for the first time that there's
10:27
this thing of water that we're swimming through. We should
10:29
figure out what this water is. Wow. And
10:31
now the other, let's say,
10:33
is the other 70% dark energy? Good.
10:36
Yeah. So that is a great. I
10:38
was both hoping and not hoping that you would bring
10:40
that up. 25% dark matter, 5% ordinary
10:42
matter. That
10:45
doesn't add up to 100%. And so the
10:47
rest is indeed dark energy.
10:49
And I'm excited that I have no idea
10:51
what dark matter is and that there are great
10:54
things to do in that field. I have no idea
10:56
what it is. Dark energy, I have no fucking
10:58
idea. There's a reason why
11:00
I don't work on it. It's
11:04
one of those shows, right? Of course, very
11:06
much so.
11:06
Especially this topic, there's going to be a
11:08
lot of boggling. Trust me. I
11:11
mean, OK. So
11:13
about 100 years ago, was
11:16
that when we realized,
11:18
I say we, the royal we hear, that
11:21
something is not adding up? That's right.
11:23
Yeah. When did we realize that? I
11:25
think this was about 100 years ago. The first astronomical
11:28
observations were, and
11:31
this is what's really, really trippy. The origins
11:33
of Scotto-Hylology were
11:36
really in astronomy. And people
11:38
would look at galaxies. And look
11:40
at how fast stars were moving in those galaxies.
11:42
And just using
11:44
ordinary, non-fancy,
11:46
Newtonian physics, the type of physics that
11:48
students grown over in high school, they
11:51
figured out that these stars moving
11:54
around these galaxies were going a
11:55
little bit too fast. It's as
11:57
if there was more gravity than.
13:59
observatory. She had to cut up a silhouette
14:02
of a dress and paste it on one of the men's
14:04
rooms. And then when she was done
14:06
crafting, then she pioneered some
14:08
giant theories about the existence of the universe. And
14:10
she died in 2016. She was never awarded the
14:13
Nobel Prize and they unfortunately do not
14:15
hand those out posthumously, which is a bummer.
14:17
But you can
14:18
name your dog Vera or your cat Reuben
14:21
and remember Vera Reuben that way. But anyway, dark
14:23
matter. It is, it's something else.
14:25
It cannot be the stuff that we're used to from chemistry.
14:27
And then
14:30
the fundamental particle physicists,
14:33
the elementary particle physicists, realized we've
14:35
been spending the past five decades trying
14:37
to categorize the elementary particles
14:39
of nature. We're trying to have the the most
14:42
fundamental periodic table. And you're
14:44
telling me that there is something that we're missing
14:46
that we definitely have to put on here? Wow.
14:49
And this became a big thing if you'll permit me
14:51
an aside.
14:52
Yes. I was hoping you'd say that.
14:55
So I'm gonna get the history a little
14:57
bit jumbled, but this is the moral history. This
14:59
is the way that we're gonna remember it. Okay. In the 80s and
15:01
90s, there was one
15:02
big hot question
15:07
in particle physics. And that question had
15:10
to do with the Higgs boson. So the
15:12
Higgs boson that in 2013 won the Nobel
15:14
Prize for its discovery. Big deal. Big
15:17
fucking deal.
15:17
And now that's sometimes
15:20
wrongly called the God particle. Yes.
15:22
Okay. Right. That is the quote-unquote
15:25
God particle. Right. And if you asked physicists
15:27
in my generation, its discovery
15:30
was more like the second particle where
15:33
we had to really do some soul searching. Because
15:36
in the 80s and 90s, we had realized there's
15:38
probably a Higgs.
15:39
If there's not a Higgs, things get way more interesting.
15:42
But if there's a Higgs,
15:44
something isn't quite right in the theory.
15:47
Because for all the reasons that we needed
15:49
to have the Higgs, if the Higgs had the
15:51
mass and the properties that we needed it to
15:54
have, somehow it just didn't
15:56
seem right. It was far
15:59
lighter in mass, then
16:01
it really ought to have been. So we now
16:03
know it weighs about 125 times
16:05
the mass of a proton, which is pretty honking
16:08
for a fundamental particle. And
16:10
our prediction, naively, if I gave that
16:12
calculation to a first year grad student, they'd say
16:15
it's probably way heavier than that. It's
16:17
like balancing a pencil on its tip. The quantum
16:20
corrections to its mass would make the
16:22
Higgs heavier than it actually is.
16:24
And just some very brief background
16:26
on this. So Higgs particles make
16:28
up the Higgs field, which is this big cloud of
16:30
bosons or particles. So matter
16:33
started out zipping around like
16:35
photons, just unencumbered by mass. But
16:38
interaction with the Higgs field is what
16:40
makes matter interact with gravity and
16:42
have that mass be gravitationally attracted to
16:45
each other. But Higgs bosons, very
16:47
hard to find. You have to get like
16:49
a large hadron collider, say,
16:52
maybe 27 kilometers under Geneva.
16:55
And then you got to race protons at each
16:57
other. You got to explode them. And
16:59
then you got to measure what's left,
17:02
a.k.a. a decay signature. And if you're
17:04
looking through all those pieces and you have pieces
17:06
and parts for what could have been Higgs boson
17:09
that existed for a fraction of a millisecond, then
17:11
that's almost proof. But
17:13
for a long time, this possibility of the
17:16
Higgs particle had vexed science
17:18
for years. One leading scientist
17:20
wanted to call it the goddamn
17:22
particle. But his book publisher
17:24
was like, let's go softer and
17:26
naively made the facepalm
17:29
modification to just call it the god particle,
17:31
which has been making physicists cringe
17:34
for decades now. But yes, essentially,
17:36
things just didn't add up.
17:37
And so this was a huge
17:40
puzzle.
17:41
It's analogous to having an ice cube sitting in
17:43
an oven and you turn the oven on and the ice
17:45
cube is still there. So we
17:48
called this the hierarchy problem. For
17:50
people like me, we write it with a capital H
17:52
when we write our academic papers.
17:53
It was a big deal. It
17:55
seemed to be the reason why our
17:58
theory of particle physics just could not be complete. So
18:01
prior to 2013, they knew
18:03
something wasn't quite right. And
18:06
so we had these great exotic theories.
18:09
They had funny names, supersymmetry, extra dimensions,
18:11
compositeness. You know, maybe
18:14
the electron and its cousins are
18:16
not fundamental, but are actually
18:18
made of smaller things. Oh, wow. So
18:20
this was the heyday in the 90s of
18:23
doing particle physics. And right
18:25
around that time, as we were developing these really awesome
18:27
theories, people realized, hey,
18:31
in order for this theory to work, meaning
18:33
in order for protons not to decay too quickly, in order
18:35
for the universe to actually look like the way it does,
18:38
we need to tweak it a little bit. And
18:40
one output is we
18:42
get these new particles that stick around. They don't
18:44
decay. They're just around. That's
18:47
kind of weird. And
18:50
I imagine there's some particle
18:52
physicist sitting in his office saying this,
18:55
and an astronomer walks by and says,
18:57
you have particles just sitting around
19:00
contributing mass? Have
19:02
you heard about this anomaly
19:04
that we have? There's more mass in
19:06
these galaxies. And
19:08
so particle physicists were, I mean, were
19:10
kind of smug. Just
19:12
said, oh, yeah, OK, good. I
19:15
have discovered what your dark matter ought to be. You,
19:17
in 15 years, when we turn on this collider,
19:20
we're going to discover what this particle is. We'll measure
19:22
how heavy it is. And I will tell you exactly
19:24
what's in these galaxies that you've been looking at for the past hundred
19:26
years. This was the promise. Yeah. And
19:29
so
19:29
particle physicists didn't even care about the dark
19:31
matter because that was the output of this
19:34
elegant theory that solved the capital H
19:36
hierarchy problem. And just
19:37
a side note. So the capital S
19:40
standard, capital M model of particle physics involves
19:43
this uniform framework for
19:45
understanding electromagnetic
19:48
and weak and strong interactions. And
19:51
the hierarchy problem is the difference
19:53
between the way a weak force, which is a force
19:55
that allows protons to become neutrons and
19:57
then back and forth, vice versa. So that weak
19:59
force...
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23:00
On
23:02
January 6, 2021, while
23:05
many of us watched news of the attack on
23:07
the U.S. Capitol in horror, Tasha
23:10
Adams watched knowing her estranged husband
23:12
was behind them. She was married to Stewart
23:14
Rhodes for more than 20 years, including
23:17
when he founded Oathkeepers. The first
23:19
words out of my mouth were, I helped start
23:21
this. And would
23:23
this have happened had I not supported
23:25
Stewart?
23:26
That's on the next episode of Deaf, Sex, and
23:28
Money, wherever you get podcasts.
23:36
Lulu. Latif. Radiolab. We
23:38
are back with Ali Ward on scop-to-hy-lology.
23:43
AKA the study of dark matter. With theoretical
23:46
particle physicist Flip Tonato. Here's
23:49
Ali. What about the
23:51
name dark matter and dark energy? Because
23:54
it's invisible at best, right? Absolutely.
23:57
Who decided that it would be called dark? Who decided
23:59
that it would have a spooky-
23:59
That is a great question. I think
24:02
it was Zwicky who was a famously
24:05
cantankerous physicist in the
24:08
early part of the 20th century.
24:10
So yes, this was 1933 with
24:12
Caltech's Fritz Zwicky. And
24:15
when you hear the words famously
24:17
cantankerous, I know you want the story time. And
24:20
among a lot of different legends and slander
24:22
and feuds and jealousy and what
24:24
sounds like a little maybe a touch of
24:26
old timey verbal abuse.
24:28
If his enemy stories were to be believed,
24:31
Zwicky would allegedly call his
24:33
colleagues scatter brains and
24:36
spherical bastards, spherical
24:38
because quote, they are bastards every
24:40
way I look at them. Oh, messy. I
24:42
love it. But a 2008 article in
24:45
Discover magazine features testimony from
24:47
Zwicky's daughter, Barbara Reina, that
24:49
Dr. Fritz
24:50
was just so brilliant that he had a lot
24:53
of haters. But he was the one who
24:55
coined the term dark matter. And what
24:58
he meant was that
24:59
it doesn't interact with light.
25:01
Yeah. So usually
25:04
we think things that are dark don't interact with light. But
25:07
actually, probably there's some junior high student out
25:09
there who'll say, no, no, no, things that
25:11
are dark absorb light. They're actually maximally
25:14
interacting with light. If you're an astronomer,
25:17
dark means you don't see any photons from it.
25:19
So I think that's why they use the word dark. And
25:21
to the best of my knowledge, I think dark
25:24
energy, which was discovered a little bit later,
25:26
as a big question mark, yeah, they
25:29
latched on to the to
25:30
the branding that we developed.
25:33
And they use the word dark to
25:35
mean just like dark matter, we don't know
25:37
what this is.
25:39
But at least dark matter, we had the idea
25:41
that this was stuff, these were particles, I'm 99.9%
25:44
sure dark matter is at least one particle.
25:47
Dark energy, definitely behaves
25:49
differently. And it's a much weirder thing.
25:52
Do you drive around in
25:54
traffic and think about this stuff? Like, can
25:56
you ever escape theorizing
25:59
about Oh, that is a
26:02
great question. I think the
26:04
the imposter syndrome in me says yeah, I escape
26:06
it way too much But traffic
26:09
in LA as you know is not not
26:11
a great place to have happy thoughts But
26:14
I often find myself thinking about physics in
26:16
the swimming pool
26:17
Really? So for example, there's this idea of we
26:19
are fish in an ocean of dark matter that
26:21
was something that I was I was thinking
26:23
about while swimming and I
26:25
guess being in a mathematical
26:28
discipline your
26:30
Sharpening your equipment like you having
26:32
having the finest equipment is really having
26:34
a clear mind And I can
26:36
sit at my desk and I can do a calculation
26:39
I can write a paper but the
26:41
creative spark is something that usually happens outside
26:43
of those environments. So Walking
26:46
around or having tea
26:48
on my patio that that that's that's
26:51
where the magic happens
26:52
and be honest with me without having A name names how
26:54
many astrophysicists out there
26:56
think that dark matter might be ghosts What
26:59
if dark matter is ghosts? What if dark energy is
27:01
ghosts? What if it's all ghosts?
27:02
What if we're swimming in ghosts? there
27:05
is a famous quote from Nima
27:08
our Connie Hamed before the LHC
27:10
turned on and and The
27:12
quote was something along the lines of we
27:14
might turn it on and dragons might pop out.
27:16
We have no idea What's gonna pop what's gonna
27:18
happen? So in a March 2008 New
27:20
York Times article This particle theorist
27:23
who was at the Institute for Advanced Study in Princeton
27:25
told the paper that there was some probability
27:28
of almost anything happening even a minuscule
27:31
chance that quote the large hadron
27:33
collider might make dragons That
27:35
might eat us up. Maybe he was just
27:37
ahead of the curve and predicting the 2011 premiere
27:41
of game of Thrones, but either way people
27:43
were rightly pumped
27:44
and that kind of encapsulated a lot of the
27:46
the excitement there is something to be said
27:48
about maybe dark matter is something
27:51
much more exciting than particles and
27:54
There are theories where the
27:57
dark matter
29:58
it's probably
30:01
also not black holes. Okay. So
30:04
these are the other two like exotic things that you learned from
30:06
Star Trek. Yeah. So
30:09
it's not antimatter because if
30:11
we're swimming in the sea of dark matter and
30:13
if the dark matter were antimatter, it would keep
30:16
annihilating with ordinary matter and producing light.
30:18
So the fact that, I was going
30:21
to say that we're not a glow stick in the universe, but
30:23
really the
30:24
fact that our galaxy isn't just being burnt
30:26
up by the antimatter,
30:28
that means dark matter is not antimatter.
30:31
Nice. Until fairly recently, we would
30:33
say it's not black holes because black holes are a totally
30:35
different thing. But there have been some thoughts recently
30:38
that there might be little
30:41
tiny black holes that were formed in the universe that
30:43
would behave like dark matter. How tiny
30:46
are we talking? That's a good, there's a range
30:48
of sizes, but
30:50
the story of little black holes is funny.
30:52
For a long time, people were worried that turning on the LHC
30:55
would produce lots of little black holes that would eat the earth. Sounds
30:57
like fun. But we were pretty
31:00
sure that little black holes evaporate
31:03
and would be relatively harmless. Little black
31:05
holes are like little
31:05
particles. And do you
31:07
think that those could be just on earth
31:10
in just little pockets here
31:12
and there?
31:13
Chances are no. I would bet no, but
31:16
it is a theoretical possibility. It's attached
31:18
to a whole bunch of other weird things. I think to
31:20
make it work out gravitationally, you
31:22
need to have extra dimensions and maybe a few extra dimensions.
31:25
But it was a fun thing to think about 10 years
31:28
ago. Do you think that dark
31:30
matter could be extra dimensions? That is
31:32
a great question. That is what I spent
31:34
my summer vacation thinking about. So
31:38
extra dimensions are a really funny quirk
31:41
in the history of theoretical physics. I
31:43
think the modern way of
31:45
thinking about this is
31:47
the people who work on extra dimensions
31:50
don't necessarily literally believe
31:52
in,
31:53
if I could just step in the right way, I'm gonna be in
31:55
some parallel universe. But
31:57
in the mathematics, one
32:00
realizes that if I can write
32:02
a theory in
32:04
three dimensions of space plus one dimension of time, I
32:06
could write a theory in four dimensions of space plus
32:09
one dimension of time, or in five dimensions of space and
32:11
one dimension of time. No problem, right? It's
32:13
just, it's another number that you add onto
32:16
your mathematical expressions. And so
32:18
people, it was easy to play with. And
32:21
in the 1990s, one
32:23
of the huge revolutions in theoretical physics
32:25
was this observation that particular
32:28
types of theories with extra dimensions
32:30
end up giving mathematically
32:33
equivalent predictions. When
32:36
you were asked the right question to
32:39
a type of quantum theory that is really
32:41
hard to calculate. This is something called a duality
32:43
in physics. And it
32:46
meant that I could calculate something
32:48
in my wonky theory of extra dimensions.
32:51
And that calculation would actually mean
32:53
something in an ordinary theory,
32:55
ordinary meaning three
32:57
dimensions of space, one dimension of time,
32:59
that is highly quantum mechanical,
33:01
but a perfectly plausible theory.
33:04
And it was a type of theory that we
33:06
really didn't know how to deal with until
33:09
we had tools like this. Tools like
33:11
the Large Hadron Collider. And so
33:14
one of the fun things to play with
33:17
is we have this really powerful
33:19
machine to make predictions where we couldn't make predictions 20
33:21
years ago. Maybe we can describe cool
33:24
theories of dark matter
33:25
that one could
33:27
explain why we haven't discovered dark matter,
33:30
and two could motivate interesting
33:33
different searches. Because this is
33:35
where we are right now. We need to figure out what is the best
33:37
way to test these different theories of dark matter.
33:39
It better happen in my lifetime. I
33:42
mean, I'm sure you think the same thing given that
33:45
this is your life's work. Yes, yes. Yeah.
33:47
And in fact, this is for
33:49
for me, this is a difference between dark
33:51
matter and dark energy. Both of them are
33:54
things we have no idea what they are. I certainly have
33:56
no idea what they are. Dark matter,
33:58
we have an experimental program.
33:59
and we know enough about it that I
34:02
have faith that we have a sporting chance
34:05
that we will learn something deep about dark matter in
34:07
my lifetime. Dark energy. I'm
34:09
not sure if we'll learn anything about it in the
34:11
history of humanity.
34:13
Hey, let them fear again. We're going to jump ahead
34:15
because Ali asked Flip so
34:17
many great questions. What
34:19
is dark matter look like in
34:21
your head? Time travel. Yes. No, maybe. What
34:23
is the best music to listen to while researching
34:25
dark matter? I would honestly just listen
34:28
to a podcast that was only Ali asking
34:30
questions. They are so great. How much dark
34:32
matter is in the room right now? We
34:35
actually know this. Oh, OK. In
34:37
your coffee mug, you have about one gram of dark
34:39
matter.
34:40
If you want to hear all of Flip's answers, you can listen
34:42
to the full episode. We'll link to it on the website. But
34:45
before we go, we will leave
34:47
you with one last question and answer
34:49
from Ali and
34:50
Flip.
34:51
What about your favorite thing about what you do? Oh,
34:53
gosh. I love that
34:56
on any given day, there are new
34:58
things to learn. And either
35:01
it's some experimental result that I want to understand
35:04
or some related field where
35:07
I never had the chance to take that class as a student.
35:10
But I see that there's an opportunity
35:12
where dark matter might be able to do something.
35:14
And then I can dig in and say, I
35:16
have an excuse to spend my time reading this textbook
35:18
or reading this this this recent article or talking
35:21
to my colleague from a different department. That's that's
35:23
the fun part.
35:24
That's great. I mean, I love that for
35:26
the rest of my life. I'm going to be walking
35:28
around thinking about a gram of dark matter
35:31
in my coffee cup and and sparkly
35:34
webs and maybe ghosts,
35:36
maybe ghosts. You
35:39
don't have to commit to that on the record. I just
35:41
for my own fun. Well,
35:44
I would add to my yes and would be thinking
35:46
about all of the dark matter scientists who are
35:49
thinking about us and we are the maybe ghosts.
35:52
I love that.
35:53
Thank you so much for doing this. This was a joy.
35:55
You know, oh my gosh.
36:05
Thanks to Allie Ward and her team for
36:07
letting us share her show with all of you. Hopefully
36:10
you'll go check it out. You can find it wherever you get podcasts
36:12
or at ologies.com. That's
36:15
O-L-O-G-I-E-S dot
36:17
com.
36:18
They also, by the way, make ones suitable
36:20
for kids where they rip out all the swears. Those
36:22
are called Smologies. Big
36:25
thanks again. This episode was produced by
36:27
Pat Walters with mixing help from Arianne
36:29
Whack.
36:29
And I don't think there are any special thanks,
36:32
so I'm just gonna thank you. Thank
36:34
you for listening. New episode in your
36:36
feeds coming up in a couple weeks and it is
36:38
a really good one. It's an
36:40
Odyssey. Catch you then.
36:48
Radio Lab was created by
36:50
Jad Abenrod and is edited by Soren
36:52
Wheeler. Lulu Miller and Latif
36:54
Nasser are our co-hosts. Dylan
36:56
Keefe is our director of sound design. Our
36:59
staff includes Simon Adler, Jeremy
37:02
Bloom, Becca Bressler, Weichu Kusik,
37:04
Aketi Foster-Kees, W. Harry Fortuna,
37:07
David Gable, Maria Pascut-Tieres,
37:09
Sindhu Nganasanbandan, Matt QT,
37:12
Anima Kuehn, Alex Neeson, Sara
37:14
Khari, Anna Raskwet-Pas, Sara
37:17
Sandbach, Arianne Whack, Pat Walters,
37:19
and Molly Webster, with help from Andrew
37:21
Vinales.
37:22
Our fact checkers are Diane Kelly, Emily
37:25
Krieger, and Natalie Middleton. Hi,
37:30
this is Beth from San Francisco. Leadership
37:33
support for Radio Lab
37:34
science programming is provided
37:36
by the Gordon and Betty Moore Foundation,
37:38
Science Sandbox, Assignments
37:41
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37:43
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37:45
support for
37:46
Radio Lab was provided by the Alfred
37:48
P. Sloan Foundation.
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