Episode Transcript
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Speaker 1 (00:09):
Or Hey, what's your favorite number? Well, I like all numbers.
I try not to discriminate between numbers, but you know,
I think since I was little, I've always liked the
number four. Number four. Why is that that's a lot
less than the number of bananas in a bunch for example? Well,
I think I liked it because when I was literally
kind of blew my mind that, you know, four was
two plus two and it was two times two, and
(00:30):
it was two to the two, and so I just
thought that was like amazing, Right, it's pretty two two.
What about you, what is your favorite number? Oh, that's easy.
It's got to be forty two, because forty two. It's
the answer to everything. So maybe that should be our
podcast title. Forty two explains the universe forget about those
two guys. I guess we could stretch that to forty
five minutes, right, The answered everything is just forty two.
(00:52):
Every episode would be forty two minutes long, and we'd
have forty two good jokes. They would cancel it after
forty two episodes, and I hope we have forty two
million listeners. Hi am more hand made cartoonists and the
(01:22):
creator of PhD comments, Hi, I'm Daniel Whitzen. I'm a
particle physicist, and I'm a co author of our book
We Have No Idea, a Guide to the Unknown Universe,
and which we talk about all the amazing open mysteries
of the universe, all the things science has figured out,
and all the things science has not figured out. It's right,
there are a lot of books out there about all
(01:42):
the things we know about the universe, but ours is
about all the things we don't know. And believe it
or not, we filled the whole book with things we
don't know. And it's not just what Jorge and I
don't know about the universe, which is a lot, but
it's about what science in general. We try to speak
for humanity and bring you to the forefront of human knowledge,
to delve into the deepest questions about the biggest things
(02:03):
in the universe, i e. The entire universe, Because it
turns out there's a lot that scientists don't know about
this great, big and complex and beautiful universe, including sometimes
things about numbers. Yeah, because one way to tear the
universe apart is to sort of take it apart literally physically,
and say I am made of bits. What are those
bits made out of what are those bits made out of?
(02:25):
And then you can drill down to the sort of
the the core bit, the fundamental element of the universe.
But there's another way to look at the universe, another
way to think about it, and that's more mathematical, to
think about what are the basic numbers? Like if you
had a theory of the universe, what numbers would appear
in it? Yeah, Like if you had an equation that
(02:45):
just describes everything in the universe, would it have any
numbers in it or not? Or just symbols or concepts?
And what would those numbers be, right? And why would
they be those numbers and not other numbers? I like
to think about some he's sitting at a control panel
for the universe. Maybe the universe is a simulation and
somebody up there has knobs and they're twiddling it. And
(03:06):
you know, as you change those knobs, the universe looks different.
And so our job is to measure the value of
those knobs and then to ask, like why this value
not something else could have been anything? Are these two
knobs actually connected? Is there just one big knob? Yeah?
Like why are our podcast always about forty five minutes?
Is there a universe in which our podcasts are shorter
(03:26):
or longer. That's as long as we can be funny.
For after that it just trails off. Yeah. In fact,
even the number of knobs that the universe might have
would be significant, Like if the universe had seven knobs
versus three knobs, that would be pretty significant and would
tell you a lot about whoever or whatever made this universe. Yeah,
and this is a deep question, not just of science,
(03:49):
but also of philosophy. If you think the goal of
science is to reveal the truth about the universe, then
you have to be prepared to answer the question what
does that truth mean or does it inform us? Right?
If you're going to ask a question, you better know
how to interpret the answer, which is of course the
underlying joke behind forty two. Those folks that build a
huge planet sized computer to figure out the answer to life,
(04:09):
the universe and everything and then have no idea what
it means. You think they know there's a universe out
there in which there Douglas Adam wrote the same book
but used the number forty one, or and there are
jokes are all about that number. I don't know. I'd
love to read an interview with him about how he
chose that number, because it's achieved such cultural prominence. You know,
(04:31):
they did a survey of like all the numbers that
appear in Python code on GitHub, and they plotted the distribution,
and there's a big spike at forty two. People just
like use it as an arbitrary number all the time.
Maybe it's not a coincidence, or you know, maybe it
is a basic number that just pops up. It's the
number of neurons that work in an average person's head. Maybe. Yeah,
(04:54):
So this is an interesting concept to think about the
constants of the universe. And so today on the episode,
we'll be asking the question what are the basic constants
of the universe? And are they even constants? And why
do physicists keep calling things constant when they don't know
if they are. Why can't they be consistent about it
(05:15):
or at least conscientious, Right, It seems like a constant
annoyance to have to recalibrate my meaning of words when
I talk to physicists. Yeah, and I don't think it's
even a conscious thing. You know, we talk about constants,
we really mean numbers. But then there's a question, you know,
are these numbers actually constant. Are they changing? How could
we tell if they were changing? What if two of
them are changing at the same time, would we even notice?
(05:38):
These are really fun, interesting questions, and they really go
deep into the nature of the universe itself. You know,
we have these basic laws that describe sort of how
things interact. But then they're just seemed to be numbers
that determine, you know, the relative power, like why is
the gravitational force so much weaker than the other forces?
You know, why our stars so far apart. There's has
(05:59):
to be something to say at these scales to determine
why the universe turned out this way and not other ways. Daniel,
I feel like this baby. This question assumes that there
are basic constants in the universe. Do we know for
sure that there are constants in the universe? Is it
may be just something that we haven't discovered or something Well,
we have constants that we've measured and we do not
know how to derive them, and we'll get into the
(06:20):
definition of what it means to be a basic constant.
Um there used to be more right, and sometimes we discover, oh,
this thing that we thought was fundamental turns out to
just be a combination of these other numbers, and so
we don't need it. Sometimes, like a basic number is
just a combination of other numbers, just a combination to
other numbers. So what we're looking for is the minimal set, right,
We want the smallest number of constants, just like we
(06:41):
want the smallest number of physical laws. We don't want
to describe five thousand forces. We wanted to have one
force that describes everything. All the features of electromagnetism. We've
tied them up so nicely into a few equations with
a small number of numbers in them. So we're always
working to reduce the number of ideas and then the
number of parameters of those ideas. And we're not talking
(07:02):
about things like pie or e, right, which are sort
of mathematical or geometric constants in the universe. We're talking
more about physical constants, right, Yeah, things that you have
to measure, right, not just geometrical stuff that you could
calculate without having access to the universe. Things you have
to go out and actually measure. Because things like pie
and e are like sort of like basic constants in mathematics,
(07:24):
you know, which is sort of abstract. We're talking about
the constants in the universe that seemed to be there
that sort of define how things work. Yes, things that
if you change them, the nature of the universe would change.
Things would be different. You wouldn't have chemistry anymore, or
you wouldn't have stars, or you'd have more stars, or
you know, if different forces would be more powerful, or
(07:46):
we'd be made out of different kinds of particles. You know,
this kind of stuff that fundamentally changed our description of
the universe. But you're right, we don't know how many
constants we actually need right now. We need quite a
few to describe in the number. But if we had
the ultimate theory, how many constants would it happen? It
maybe one, maybe five, maybe ten, Maybe you have pie
number of constants. What does that even mean? It means
(08:09):
I just blew your mind, Daniel. Well, you know we
talked about how in Steven Wolfram's world there are two
point seven dimensions, so maybe you can have three point
one four numbers. Me and Stephen Wolfram are at the forefront. Well,
I pulled our listeners who are willing to participate in
virtual person on the street interviews and ask them this
question about the basic constants of the universe. And if
(08:30):
you would like to participate in these virtual person on
the street interviews, just right to us two questions at
Daniel and Jorge dot com. And you can also display
your knowledge or lack thereof on the podcast. So think
about it for a second. If someone asked you, what
are the basic constants of the universe? What would you answer?
Here's what people had to say this one. It's easy.
(08:51):
I don't know the gravitational constant and Avogadro constant. Other
than light speed, I would say that pie and oiler's
number also constants of the universe. At It's just like
things that we've measured. Well, I don't know. Well, they
gave us one hint of the speed of light, but
I think based on other podcasts that I've listened to
(09:12):
and learned from them, I think entropy might be a constant.
Gravity is a constant. And my last guest would be
maybe thermodynamics. I think physics, the you know, the standard
model of physics as we know it is constant. Right,
coals one equals one um? What else equals one pie?
(09:35):
There's Avogadro's number from ancient chemistry, listens plank mass, plank,
lenks um, Boltzman's constant reintropy. I think there was a
Daniel Why I explained the universe episode onto my dynamics.
I mentioned that the gravitational constant, elementary charge, the exponent
(09:59):
of the radius, the radius squared, and uh Gaussian formula,
and probably, I guess also called Maxwell's equations, death and taxes.
And there's also the charge of an electron and um
maybe the mass of the part of fundamental particles that
(10:21):
have mass. I know there are several constants in the universe,
however I can't remember most of them. The ones I
do remember are the speed of light, the gravitational constant,
and planks constant. Alright, some pretty good answer, is man?
Some of these I've never even heard of. Death and taxes?
You never heard it before? You know, what are taxes?
(10:41):
I don't understand. Is that what I keep playing any
letters in the midid Do you live in the sovereign
state of Jorge? Maybe I'll ask my accountant. But you know,
a lot of people are are talking about real physical
things like light speed and soul and entropy and the
speed of light. Yeah, people are saying things that are
sort of parameters of physical theories. But these are not.
(11:04):
Actually the basic constants that physicists talk about the speed
of light, planks constant, the gravitational constant. They seem basic,
but they're actually susceptible to sort of arbitrary definitions because
they're expressed in terms of human units. Oh, I see,
Meaning that, for example, the speed of light could be
a constant, but the constant wouldn't be three hundred thousand
(11:25):
meters per second, yeah, because that's subject to units. Yeah,
so let's get into that, Like what do we mean
by a basic physical constant? And one important thing is
that it should be dimensionless, like it shouldn't have units.
It shouldn't be expressed in terms of like furlongs per fortnite,
you know, or gallons per second or something. It should
just be a pure number, like a pure number without unit,
(11:48):
without units, like is a number without units, pies a
number without units. But it's not a physical constant because
it doesn't need to be measured with experiment, right, you
can do it in a simulation or on the computer
or something. But we're talking about physical instance that have
to be measured, and those are things like we'll get
into the whole list, but you know, things like the
mass of a particle relative to the mass of another particle,
(12:08):
like ratios, like ratios, which wouldn't change if you suddenly
change what it means if you change, like from English
units to international unit exactly. And there's two important reasons
why you have to use numbers without units. The first
is you want to look at the number and know
what it means, and it doesn't mean anything if it's
relative to some stick in Paris, or you know the
(12:29):
length of somebody's foot a hundred years ago. Right. If
you're interested in knowing a number, then you don't want
to express in terms of human units because it's totally arbitrary,
and you could change that number. It could be a
hundred eighties six thousand miles per second or three times
ten meters per second. Like, you can't look at the
number and say it means anything if it's defined relative
to something totally arbitrary. You need a basic constant to
(12:51):
feel classic, like not subject to the whims of man
and what they consider foot. That's right, And it's more
than just you know, having an maturity standard. You also
need the basic constants to be dimensionless so that you
can tell if they're changing, if they're changing, then you
can tell what's changing. I see, you don't want a
meter to be, you know, the length of a length
(13:14):
of putty, because the length of putty might change. That's right,
of the length of putty might change. But also like
you know, say you're interested in the question, you know,
does the speed of light change? Right? This is a
question you see in science all the time. It turns
out it doesn't actually have the meaning that you think
it does when you drill down into it, because it's
so subject to human conventions. Depends on how you're defining units.
(13:36):
And in fact, in Night three we change what we
meant by the speed of light. Really, yeah, the speed
of light change in after three, it doesn't make any
sense to measure the speed of light. And that's because
before nine eight three, we defind the meter to be
the length of some rod in Paris, and the second
to be um you know, ten trillion oscillations of C
(13:59):
C and one thirty three. So we had the meter
and we had the second, and then you could go
out and you could measure the speed of light. You
could say, how far did a beam of light go
in ten seconds? And I'll measure that distance with my
ruler from Paris or my copy of it, and get
a number. Cool. But then a bunch of people got
together and decided that will keep the second as like
(14:20):
you know, the number of oscillations of set three. But
then we're going to fix the speed of light. We're
going to define it to be something. So we just
pick a number. We say it's two point nine nine
whatever times ten per second. Okay, So once you do that,
you don't have to define the meter anymore. It's already
defined by the other constants. Right, You've got time, and
(14:42):
you've got speed because you have the speed of light.
So a meter then is just defined as how far
light goes in a certain tiny fraction of a second.
So the meter is now defined to be a fraction
of a light second. Right. Light seconds are the reference
for distance now the under mental way we measure distance
to the universe instead of that crazy rod in Paris,
(15:05):
and we're used to measuring distances in terms of time,
like a light year is a unit for distance to
the stars. Right, that's familiar. Well, a meter is now
just a tiny bit of a light second. It's not
defined anymore by a rod in Paris. It's measured by
how far light goes in that tiny slice of a second. Yeah,
(15:25):
we flipped it. And so now you ask, well, a
meter is now measured instead of the speed of light
being measured. Isn't even time variable? You know, according to relativity?
You know how close you are to a gravitational object,
you know, like, isn't even the oscillations of of season
one thirty three also may be subject to you know, relativity. Yeah, absolutely,
(15:46):
And that's why you want to focus on dimensionless constants, right.
But the point here, the point I was trying to make,
is that, like you can't even tell in this example
if the speed of light is changing, or you know,
the length scale the uni verse itself is changing. It
depends on if you're defining the speed of light to
be fixed and measuring the meter relative to that, or
you're defining the meter to be fixed and measuring the
(16:09):
speed of light relative to that. So the way to
figure out if the universe is changing, if the physics
of the universe are changing in time or static, which
is really what we're trying to get at, where we
measure these numbers and see if they're changing, is to
define only dimensionless numbers, numbers without any units because they're
not subject to any of these totally arbitrary definitions. All right,
(16:30):
So that's kind of what a basic constant is. It's
a number that defines some kind of ratio about physical
things in the universe, which may be there at the
end when we discover the equation of the universe. Yeah,
and I really like thinking about this this way, like
thinking about measuring distances in terms of times. You know,
it makes a lot of sense when you think about,
(16:50):
you know, measuring distances to stars in terms of the
speed of light um and it just shows you that
all these numbers we measure, like the speed of light,
they're really just ways to convert between meters and seconds.
They're just like translations between arbitrary human conventions. So they're
not actually fundamental. The things that are fundamental are things
we'll talk about, you know, a little bit. But yes,
(17:10):
we're looking for sort of a minimal list of dimensionless
quantities which would change the world if if they changed, right,
So let's maybe get into what is that minimal list
of basic constants in the universe and what we know
about them so far. But first let's take a quick break,
(17:40):
all right, Daniel, we're talking about this constant topic that
keeps coming up in physics, which is constants and what
is and what isn't changing about the universe? And are
there constants in the basic equation of the universe? And
there are how many? And what are they? And let's
just get out of the way. It's probably forty two,
but you know, we still have to check. Well, forty
(18:03):
two would be wonderful because it'd be kind of a
good joke, but it would also be kind of disappointing
because forty two is a big number. You're never happy, Daniel.
All answers have both good and bad consequence. I'm constantly disappointed. Now.
What we're looking for. What we'd love is to have
a small number of constants, because that would tell us
that we're close, right like the way we're trying to
(18:24):
boil down the universe to one particle and one rule,
that tells you something deep about the universe. If your
list of particles and your list of rules about how
they interact is fifty pages long, it tells you you're
not really close to the answer. So we want to
get down to a small number of constants because we
think those are probably fundamental. We want to look at
those and say, you know, the theory of the universe
(18:46):
has the number seven in it. What does that mean?
Why is the universe seven? Ish? You know, why seven
and not six? And we're looking for that moment where
we get to ask that philosophical question about the universe.
And you can't really do that if you suspect your
list of numbers is sort of an artifact of not
having gotten there yet. Do you think maybe the last
number in the universe. Do you think it's an integer
(19:08):
like a whole number, or do you think it's gonna
be some weird numbers? I don't know. You know a
lot of particle theorists like numbers that are close to one.
They think all the numbers and there should just be one.
They're like, we got one, we don't need anymore. Yeah,
And they wonder when they find a number that's not one.
You know, they see things and like, well, why is
electromagnetism so much stronger than the weak force? And why
(19:31):
is it so much stronger than gravity? And they have
these numbers and that reflect the relative strength of those forces,
and they wonder, why is it not one? They look
for symmetry and simplicity, so anytime they see a number
that's not one, they get suspicious because they think maybe
there's a reason, maybe there's a simpler way to express things,
where all these things are just one. And that's how
they conduct your social life too. They're like, there's more
than one people here, what's going on? This is not
(19:53):
what I ordered? They have one friend at a time,
you know, one friend at a time. It's like of
one else is apparently that's right. So we are not
there yet. We are not down to one constant. In fact,
we sort of have an embarrassing number of constants so far.
We have twenty six basic constants of the unit. Twenty six.
Oh man, that seems like a significant number in itself,
(20:16):
seems like a special number because it's what two times thirteen, Yeah,
and thirteen is the prime number. Yeah, but that means
twenty six isn't right, so it's much less exciting. Alright,
what do you mean? We have twenty six constants? Meaning
in all of physics and all of the equations that
we currently have about the universe, there twenty six numbers
that you can't break down anymore or that are not
(20:37):
related to each other. If you wrote down the whole
standard model of particle physics, and you have to put
all the numbers into all the four strengths and all
the mass particles and all the way things change to
each other. There are a lot of numbers in there,
like thousands of thousands of numbers, but most of those
numbers come from other numbers, Like how long does the
muan live? That's a number, but you can calculate that
(20:58):
based on the muan mass and the elect on mass
and the fourth strength between them. And so if you
boil it down to the minimal set of numbers that
you needed to find all those other numbers, right, the
ones that, according to our understanding currently are the knobs
of the universe, then you get twenty six. Like I
toss a ball up into the air and catch it,
you can maybe derive that time using other numbers. Yeah, exactly.
(21:20):
If I know the mass to the electron relative to
the gravitational constant and stuff like that, I can derive
most of physics from just a few numbers. All right, Well,
then let's let's talk numbers. Danuel, What what are these
twenty six? Break it down for us. What are these
twenty six apparently basic constants of the universe that we
have right now. Yeah, So there are sort of three categories.
(21:41):
One is like the strength of forces, another is the
masses of particles and how they mix, and then there's
the cosmological constant and its own category. The first ones
are really really interesting, and these are the fourth ones.
The most important one, the one that you hear about
a lot and I think reveals a lot about what
we mean by a engineless physical constant. Is this one
(22:02):
called the fine structure constant. Fine structure constant, all right,
I'm intrigued. It's a weird name. It's called the fine
structure constant because it comes from when people were trying
to understand the nature of the atom and the structure
of the spectra that it emitted. And so what it
really reveals sort of the strength of the electromagnetic force.
(22:23):
And so this number here tells you about the power
of electromagnetism as probed by the internals of the atom,
but it turns out to be a fundamental number of
the universe. What does it mean? Is it like how
how attracted an electron is to a proton or something
like that. Yeah, it's something like the probability for an
electron to emit a photon, and that number is a
(22:46):
vacuum or um. Will electrons only emit photons inside electromagnetic fields,
of course, And that number everyone knows that. And that
number turns out to be one over one thirty seven.
What exact one over one thirty seven, not exactly. For
a long time people thought it was exactly one over
on seven, and there was a big mystery in physics
(23:07):
like why that number. And Richard Feynman likes to say
that if you were a physicist and you were ever
like stranded in a foreign city, you just hold up
a piece of cardboard that says one over seven on it,
and some other physicists will see that and know that
you're a physicist, come rescuing. It's like a code. I'm
not sure if you're stranded in a city you want,
what you need is a physicist to rescue you. But
(23:29):
you know, let's leave that aside. And um. Alright, So
one of these constants of the universe is kind of
how likely an electron is to admit a photon. Yeah,
it's like the probability for an electron to emit a photon,
and it's it's actually expressed in terms of other numbers
that you will find familiar. Like the way you calculated
(23:49):
is the charge of the electron squared divided by planks
constant h bar times the speed of light, and so
it has all these other of familiar things built into it.
But when you put all those things together, the units cancel,
Like you get up a number that has no units
in it, And that means something really really deep. Um,
(24:10):
what do you mean? What I mean is that it
tells you something about the importance of the speed of light.
It tells you, for example, that the speed of light
is not actually a fundamental constant. That if you change
the speed of light, but then you also change these
other numbers inside the fine structure constant to keep the
fine constructure constant the same, you would not be able
to tell the difference. The universe would work the same way.
(24:32):
As long as you keep these numbers the same, then
you can change the speed of light and the strength
electromagnetic force, and you could not do an experiment that
showed that anything had change, Like it doesn't have any
consequences anywhere else in the universe. That's right. When if
you change the speed of light, Wooden, you we know
it is like, oh, it takes longer for light to
come to us from the sun. If you only change
(24:52):
the speed of light, which means that you're effectively changing
the fine structure constant, then yes. But if you change
the speed of light and you also change like the
charge of the electron or planks constant, or you manipulated
these things in such a way to keep the fine
structure constant the ratio of these things the same, then
you could not tell the difference. It's like, Okay, distance
now means something different. But you know, the electromagnetic force
(25:16):
is now stronger. So what are you using to measure distance.
You're using you know, the photons admitted by electrons or something.
So you cannot devise an experiment that is sensitive to
changes of just planks constant or just the speed of light. Um,
if you keep the fine structure constant fixed, somebody could
change these things and nobody in the universe would even notice.
(25:40):
Nobody in the universe could even notice, you know. Imagine
a simpler example, like, I feel like, I feel like
this is a conspiracy. Suddenly I feel nervous. It's about
our world is relative to our units. Imagine, for example,
somebody came in and change the universe so that now
every distance was doubled. This distance between all particles was doubled. Suddenly,
could you notice? Well? Sure, but not if then they
(26:03):
also increase the power of all the forces so that
things didn't seem as far, and they increase the maximum
speed you could go. Right, then it would take you
just as long to get from here to work, and
your rulers would also change, right, so you would say, oh,
I'm still the same high as that was yesterday. It's
like if somebody just scaled up the universe, but they
made sure that everything worked same, would we even notice? Exactly? Like,
(26:26):
could somebody bottle up the whole universe into a little
bottle and then made sure that all the knobs were
also changed that we wouldn't notice the difference. It could happen.
It could happen. And that's why we focus on these
dimensionless quantities, because you can't change those without changing the physics.
You can change the things that they express, you know,
this fine structure constant. You can change the dimension full
(26:46):
of the unit quantities inside them. But if you change
these fine structure constants, then there's no way to hide
that they do seem like basic constants of the university.
They do. And it's like a basic ratio of the universe,
you know, just like pies, like the ratio of you know,
the radius and the circumference. This is like the basic
ratio of matter and how it moves in the world.
(27:07):
And now I'm gonna disappoint you because it turns out
it's not actually constant. No. No, but it's not that
it's not constant in time. It's really weird and we're
gonna dig into this next week when you talk about renormalization.
But it depends on how fast you're going when you
measure it. Isn't that what I brought up earlier, like
relativity special relativity. Yeah, it's actually it's more about the
(27:28):
momentum you have relative to the thing that you're measuring,
rather than actual velocity. You just can't admit I was right,
You're always right, or hey, that's one constant of the
universe relatively speaking. All right, So that's that's a good flavor.
I think that gives us a good flavor for what
these constants mean. And it blows my mind that there
are twenty six of these that we think we know
(27:49):
about twenty six things that can't change or could change
internally but we wouldn't notice. Yeah, all right, Well, let's
get into the other kinds of constants in the universe
that we have and what they mean and whether or
not there are more of them. But first let's take
another quick break. All right, then, we're talking about the
(28:18):
basic constants of the universe that are not constant, but
we think are sort of constant consistently. Well, that's one
thing we don't know, right. We measure this thing, we've
measured a lot of different times, over many different years,
and we do not see it changing in time, and
so we say, maybe this is constant, and it's just
like the rest of science. We have no reason to
believe that you do an experiment today and you do
(28:40):
experiment in a week, you should get the same answer
in the same conditions. But it seems to be true.
We live in an empirical universe where you can repeat experiments,
and it seems like these numbers are fixed. We may discover,
if we keep doing science over a thousand years or
a million years, that they're very slowly varying, and that
would be fascinating, But so far they do seem constant.
(29:00):
All right, And so you're telling me that physicists have
twenty six of these constants, and some of them are
related to like how particles interact with each other and
how attracted they are to each other, but some of
them are also related to their masses. So tell me
about this, yea. So we have to the determine the forces.
One is the fine structure constant that tells you about electromagnetism.
There's a second one which tells you about the strong
(29:21):
nuclear force. But then most of these constants actually relate
to the particles, and that's because we just don't know
why the particle masses are what they are. Like, we
have twelve matter particles that make up the standard model.
There are six kinds of quirks up down, charm strange
top bottom. Those are six different particles with six different masses.
(29:44):
And then there's six leptons, electrons, muans, towels, and their
three neutrinos. So those are twelve particles and we do
not know why they have the masses they do. We
can't predict it, we can't calculate it. We don't even
see a pattern. And so we just have to put
one parameter when to mention this constant for each one.
You wish they were related, but so far they don't
(30:06):
seem to be. Yeah, we wish that. You know, the
muon was twice the mass of the electron and the
towel was four times the mass or there was some relationship,
so you could only fix one number that would determine
all the rest of them, and also that would give
us some insight to like why are there these other
particles and why are they heavier and stuff like that,
But we see no pattern at all. There's a huge range.
(30:27):
The electron is super duper light, the neutrinos are even lighter.
The top cork is like enormously heavy relative to all
the other ones. So there are some very general rough patterns,
but really nothing we can put our finger on. So
it's the masses of these particles. And I guess the
question is how do you measure these masses? Is it
like how much they weigh when you put them on
a scale in Paris, or you know, it more like
(30:50):
if you push a towel particle, how much does it move?
What he called the mass of these particles. Yeah, so
here we're talking about the rest mass, right, which means
how much energy it has essentially when it's at rest,
when you're in its reference frame, and it's hard to
measure because particles are very very small and their masses
are very very light. And so what we do instead
is we wait for one of these things to decay,
(31:11):
for example, and we measure the energy of the particles
that come out. So if a massive particle turns into
massless particles, then the mass of the original particle gets
turned into energy of those massless particles. We measure those
energies like the photons, etcetera. Then we can measure the
mass of the original particle, and so we can do
(31:32):
things like that, but it gets harder. The particles that
don't do that, like the electron stable, so there you
have to do things like put it in a magnetic
field and see how much it bends, because that's partially
determined by its mass. I guess it would be route
just to ask him what the mass. They don't like
to talk about it constantly, but they have to be
dimensionless numbers. And so what you could do is, because
(31:52):
I'm gonna fix the mass of the electron, and I
would measure everything relative to the mass of the electron.
But then the electron mass then is still a dimension
full number. And so what we do is we set
all these things relative to the gravitational constant big G,
which has the same units of mass, and so all
these things are relative to big G. Big G meaning
like nine eight per second square. No, that's little little
(32:15):
G is But just you said louder, little G is
the force of gravity at the surface of the Earth, right,
And that's a number that's important to us, irrelevant, but
definitely not a constant of the universe. It just depends
on the size of the Earth and how much mass
it is, and this kind of stuff. Big G is
the number that goes inside Newton's equation and then later
(32:36):
also in Einstein's field equations for gravity that determines the
strength of the gravitational force. It's more basic. It's more basic, yeah,
and it should be true all over the universe. And
so we measure the mass of these particles relative to
that because usually what you're interested in is actually the
ratio of inertial mass two forces, right, like how much
gravity are you putting on this thing? How much is
(32:58):
it going to accelerate? That depends on how much mass
it has, and so we measure these things relative to
big g also to keep them dimensionless. And so it
seems that we have twelve particles and their masses. That
seems to be basic about the universe. And are these
constants sort of like define structure constant where I could,
you know, change the mass of an electron and I
wouldn't notice. Now, if you change the fine structure constant,
(33:20):
you would definitely notice. But if you change one of
the numbers inside of it, you you might not notice.
So as long as it's a constant, then we would
have noticed. Yeah. And so if you change the mass
of the electron, for example, and made it heavier than
the muan, then a lot of things would change, because
then the electron wouldn't be stable anymore. It could decay
into muans. And then maybe our atoms would we have
(33:40):
muans in them instead of electrons, right, we'd be muonic
matter instead of electronic matter. But what you're I guess
what you're saying is that the speed of light could change.
But as long as you change everything else, we wouldn't notice.
And as long as you also don't change the masses
of the particles, yeah, but if you change these massive
the particles relative to the gravitational constant, you'll definitely notice,
(34:00):
and especially if you change their relative orders, you know,
because there's a hierarchy there, and if you change those
things then we will definitely notice. It would change the
way physics and chemistry works. All right, Okay, we have
twenty six constants. Two of them are about the forces
of the universe, twelve are about the masses of the particles,
and some of them are also sort of related to
how particles mixed together. Right, and then we have the
(34:24):
cosmological constants, which we talked about in a previous episode. Yeah,
and so all the other ones relate to the particles
and how they mix and and all of that stuff.
There's three more for the force particles Higgs, W, and Z,
and then eight for how the particles turn into each
other and how often it happens. But then you write
the big one, the one at the end, is the
(34:44):
cosmological constant. That's the one that tells us how fast
the expansion of the universe is accelerating, or if it's
accelerating at all, and it determines like the overall shape
of the universe. But you guys, don't go in between here,
it's either but little tiny particles or the entire universe.
It turns out little tiny particles determine the entire universe.
(35:07):
Do you think maybe the cosmological constant is related to
something about particles? It could be right. People have tried
to calculate it. They say, let's try to predict the
cosmological constant. If it's in fact just the energy of
empty space, like the vacuum of empty space it becomes,
for example, from the Higgs Boson field, then we should
be able to calculate it. And they've tried. But the
number they get is different from the number we measure
(35:30):
by ten to the hundred and twenty a little bit.
We're not even close. Yeah, we're not even close to
getting that one right. But we'd love to. You're right,
we'd love to be able to derive this number from
the other numbers, because then we could take it off
our list and we'd be down to a thin and
trim twenty five numbers, and you would make a little
bit of progress in the constant define the universe. All right, Well,
(35:50):
we uh, there are twenty six right now that physicists
can't break down anymore. And is that it do you
think maybe there are more? Do you think there should
be less? Are you guys aiming to collect more? Are
or to you know, do some spring cleaning and get
rid of some of these. I think there should definitely
be a fewer, right, we should have one number, maybe
maybe even zero. I'd love a theory the universe that
has zero numbers. Yeah, well, zero numbers in terms of physics,
(36:14):
but maybe like if you can get it to come
down to a mathematical constant, then that would be cool,
that's what you mean, right, Yeah, maybe you could have
pie and E and I and there. It would be
cool if there are no physical parameters in the fundamental theory.
But we're sort of working in the other direction right now, Like,
if anything, we're moving in the direction of adding more numbers.
Because this theory we've been talking about, the standard model
(36:36):
that describes the universe, we know, doesn't actually describe everything
in the universe, and so as we add to it
to describe those other bits, were just figuring out that
we're gonna need more numbers. Yeah, because it turns out
that apparently the standard model only covers about five percent
of the entire universe, right, Yeah, And you know, it's
a staggering achievement so far. But there's a lot of
(36:57):
stuff out there it does not describe. And so what
about dark matter? For example, if dark matter is fifty
kinds of particles and we don't understand why they are
fifty and why they all have different masses, Boom, that's
fifty more numbers right there, or maybe could have one number,
or I wonder if it could help you cancel some
of your numbers. Dark matter has the same structure as
normal matter, and now we understand the masses because we
(37:20):
see more of the pattern and it reveals itself and
we get some insights and it helps us figure it out.
That's why we're always struggling to attack the parts of
the universe we don't understand, because they could be the
puzzle piece that lets us see the whole picture. And so, yeah,
there could be more out there, because there's a lot
of the universe we don't know about. And you're also
telling me that they're not really Maybe even constants, like
(37:43):
maybe the mass of the electron could be changing, is
that possible, or you know, this fine structure constant could
also be different, not just in time, but in different
parts of the universe. Yeah, we don't know if these
things are constant in space and in time. It's sort
of like a hypothesis. It's the simplest description so far,
because we haven't seen them change, and they seem really
basic and fundamental. But because we don't know where they
(38:05):
come from and why they're important, why we have this
set not a smaller set, we can't say anything about
whether they really are constant. It's just an observation. It's
like if you live in l A. And you go
outside and you're like, hey, every day is sunny. Well,
that doesn't mean it's gonna be sunny every day. There
might be a reason why it's sunny or in l
A than it is in New York, but unless you
understand the reason for it, you can't really make an
(38:27):
accurate prediction. But you know, I like looking forward to
the end days when we have that theory and we're
looking at it and we're asking questions about what those
numbers mean. So I went around and I did a
little informal survey in my department. I asked some of
the particle theorists. I said, how many numbers do you
expect to see in a theory of everything expect to
be or want there to be. I think, I think,
(38:51):
isn't it the same seem you know, you're asking whether
they expect to be disappointed? Essentially? Yeah, kind of. So
what did they say? How many numbers did they predict
our final theory of the universe will have? I was surprised.
I was expecting them to say one number, and that
numbers shouldn't be one or close to one one number
(39:11):
one quantity, Yeah, exactly, but they really didn't know. They said,
you know, could be one number, could be seven numbers.
You know, they expected to be smallish, you know, maybe
less than ten numbers, but they wouldn't give a firm prediction.
And then I asked them, well, what do you expect
those numbers to look like? Like? Should they be huge
numbers or small numbers? Should they all be close to
one and one of them? A friend of mine, Tim Tait,
(39:31):
sort of blew my mind, and he said, it doesn't
really matter if it's close to one, because close to
one is just relative to the integers, and who knows
if like equally spaced numbers one unit apart means anything anyway.
So he's like thinking about like whether integers are a
kind of unit. But yeah, exactly, questioning the nature of
numbers themselves. Yes, yes, And you know, it doesn't even
(39:54):
make sense to have mathematics in terms of equally space numbers,
because you know, the numbers were all there. Just declaring
these equally space numbers to be meaningful, you know, it's
sort of a human convention. Let's just throw everything out
the door, Daniel, numbers don't mean anything. Distance, the word constant, Yeah,
that doesn't mean anything. Well, that's why we try to
drill down, because we try to peel away the human
(40:15):
bias and look at the universe the way it actually is,
which is why you know, I like stories about alien
scientists where the aliens don't have differentiated bodies that they're
like part of some larger mass, and so they never
come up with this idea of integers because they never
count like me and you and indistinct objects, and they
aren't linked to this kind of assumption in their mathematics,
(40:38):
and that makes them think differently about the universe. And
that's what we're trying to do here, not specifically meet
those weird aliens, but get out of our human bias
and think about the universe as close to objectively as
we can, right, Yeah, I think the lesson here is
don't go to a physics theorist if you want the
concept simplified. That's what I'm here for. I'm trying to
(40:59):
filter the sixth theory for everybody. All Right, Well, that
was a pretty cool discussion. I feel like it's amazing
to think that there are constants that you know, kind
of define our universe and that maybe in another universe
those numbers are different and they're having different discussions about
the whole thing. Yeah, And it could be that we
get down the theory of everything and it has a
(41:20):
few numbers in it, and we wonder, like why those numbers,
And you know, it could be that those numbers are
just an accident that there are zillions universes and they're
all set randomly, or it could be that, you know,
they were set for some other reason, or it could
be that they could only be those numbers. It will
be a fascinating moment when if we finally get there,
there could be no answer. You're preparing to be disappointed.
(41:43):
I'm always looking forward to the future the universe, expecting
it to be chock full of insights and discoveries. And
mind blowing revelations. That's why I'm helping out. You're a
constant optimist, and yeah, exactly so far, I've revealed exactly
zero truths about the universe in my professional career, but
I am optimistic. Hey, zero is a basic constantly the universe.
(42:05):
You know, Douglas Adam would be proud today. Zero What
I've accomplished today, the number of pairs of pants I
put on today. Well, we hope you guys enjoyed that.
Thank you for joining us, and think about whether the
universe around you is constant and what that means. See
you next time. Thanks for listening, and remember that Daniel
(42:32):
and Jorge Explain the Universe is a production of I
Heart Radio. For more podcasts for my Heart Radio, visit
the I Heart Radio Apple Apple Podcasts, or wherever you
listen to your favorite shows.