WEBVTT

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[SQUEAKING]

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[RUSTLING]

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RAFAEL JARAMILLO: Good, all
right, so let's get started.

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Today is lecture
2, 3020, and we're

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going to talk about the
scope of thermodynamics.

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And one last note--

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I'm in another
location, so getting

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used to the configuration
here with the camera.

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My face is hidden behind
the camera half the time.

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I'm sorry for that.

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I think that by Monday I'm going
to have this all worked out.

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But at least you can
see me, so there we go.

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All right, so what does
thermodynamics treat

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and what does it not?

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That's the topic of the day,
the scope of thermodynamics.

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So first we're going to
talk about states of matter.

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What is a state of matter?

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There's different ways
to define it, of course,

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but we're going to
define it as something

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that has well-defined
responses to, let's

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say, squeezing, heating,
adding more of the same stuff,

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and adding different stuff.

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And we're using
colloquial language here,

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but there is way that
matter responds to stimuli

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like these is characterized
by response functions.

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And we're going to
write these down.

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So these are the types of
things that we're going

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to do throughout the term.

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Another thing that we often
do to states of matter

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is we apply fields.

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We don't treat that in 020.

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We don't get there, but the
types of fields we might apply

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are strange fields,
gravitational fields,

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magnetic fields,
or electric fields.

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We might just get to a little
bit of electrochemistry

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in the class.

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We'll see if we get there.

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But, otherwise, we're
not really going

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to spend time talking
about applying fields.

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So we have this stuff, and
we're characterizing it.

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And we characterize
it by how it responds.

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So that's one thing that
thermodynamics treats.

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Thermodynamics also treats
transformations between states.

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So this is pretty generic.

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We have some state A, and
it transforms to some state

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B. It treats transformations.

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So we have starting and final
states described certainly.

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So we have certainty over
what those states are,

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how they behave.

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These diagrams are
really useful for that.

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You say here's the
state that you expect.

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Let's change the
temperature pressure.

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Here's the final
state that you expect.

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So we can use phase diagrams
to make these predictions

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with certainty.

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One thing that's-- and knowing
about thermo when you first

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learn it is that the
process is abstract,

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meaning thermo tells you how
things start out and how they

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end up.

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But a process of
transformation--

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it's very much a
black box in thermo,

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and we don't really treat it.

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There's a class for that.

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It's kinetics.

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You take it in the fall,
so we'll be specific.

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Kinetics is not described.

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There's no time in thermo--

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at least in equilibrium
thermo-- when you first see it,

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like in 020.

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So we will never do this to you.

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Never going to do
that-- we're never going

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to take any time derivatives.

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We're never going
to calculate rates.

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We only calculate what you
get at the end of a process

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if you wait sufficiently long.

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What is sufficient?

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I don't know.

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This is one way
to think about it.

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Thermo describes the why
and only hints at the how.

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I find this an interesting way
to remember what thermo does

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and what it doesn't.

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So, for instance, when
we rupture the hot pack

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or we rupture the cold
pack, we could understand

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those spontaneous reactions.

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We understood why.

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One of them was
driven by entropy.

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The other was driven by energy.

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That was the why.

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But the how, we
didn't talk about it.

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In fact, somebody
thankfully asked

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me a question how that worked.

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What was actually going
on inside the bag?

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It had to do with two
different bags and the surface

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preparation and supersaturation.

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Thermo doesn't
really treat the how.

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It just gives you some ideas.

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So it's a starting point
for understanding the how,

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but it does tell you the why.

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All right, what about the
use of thermodynamics?

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You're here-- you're here
because thermo is useful.

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It's really useful, whether you
become scientists or engineers.

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It's really useful, and that's
why we make you take it.

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So how is it useful?

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How do we use it?

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We use it to predict
and control matter.

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And we use it to
transfer knowledge--

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again, an example
being phase diagrams,

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which are great
summaries of knowledge.

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So let me give you an example.

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Let's have it a
temperature axis here.

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This is temperature
in degrees C.

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And we're going to study water
at one atmospheric pressure.

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So it's one-dimensional
system here, temperature.

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And here it is boiling.

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All right, so what is the
freezing point of water?

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Somebody?

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You know this.

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What's the freezing
point in water in C?

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AUDIENCE: 0 degree Celsius.

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RAFAEL JARAMILLO: Zero, right.

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I'm freezing right
now in this basement

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in the woods in Vermont.

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So I'm freezing.

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What about if we're
here in the summer?

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It wouldn't be boiling, but
what is the boiling point

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of water in degrees C?

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100, someone put the chat.

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Well, I don't really
monitor the chat.

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Not because I'm anti chat--
it's just one too many screens

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cluttering up my thing.

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So next time,
please use the mic.

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But yeah, it's 100.

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Thanks.

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So here's a question.

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How did you know that?

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Anyone who just did a
quantum chemical calculation

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from first principles, I
want you to raise your hand.

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Nobody did that.

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In fact, if you
did, you'd probably

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be writing a paper right now
because that's still a very,

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very, very hard calculation.

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In fact, I've never seen
it-- an accurate prediction

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of the freezing
point of a liquid

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from first principles
using theory.

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So how did you know that?

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AUDIENCE: These are material
properties of water.

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RAFAEL JARAMILLO: These are the
material properties of water.

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You know that because
you know that.

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And you know that because
the data that's out there you

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have access to.

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Materials have properties,
and some of these

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are so commonplace that you
know them without having ever

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taken a class.

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So these are observations.

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These are observations.

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These are two of the huge
number of observations

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on materials that mankind
has taken over millennia.

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Thermal gives you a
framework for ingesting

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those observations and using
them to make predictions

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about states that you
have never seen before.

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So this is the way
to think about it.

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Empirical observations--
so it's a bunch

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of observations, observation 1,
observation 2, observation 3.

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All these little
pieces of data, they

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get fed into something called
the laws of thermodynamics.

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This is the
conceptual framework.

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And then, from
these observations

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and the laws of
thermodynamics, you

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can deduce predictions, or what
I like to call it, decisions.

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Because when we're
scientists, we

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talk about hypotheses
and predictions.

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But when we're engineers,
we have to make a decision.

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What temperature will
they run this furnace?

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How high can this autoclave
run without ruining my product?

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What's the maximum
temperature that this product

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can see during shipping?

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And you don't have time to
run a million experiments.

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So you need a deductive
framework to make decisions.

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And that's what
thermo gives you.

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How do we store observations?

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We store them in databases.

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So as you'll see starting
in the first piece,

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thermo concerns itself very
much with the maintenance

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of databases.

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Without materials data,
these laws of thermo

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are just text on a page.

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They're utterly useless.

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You need this-- the data fed
into the deductive framework

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to make decisions.

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So the databases have
huge economic value.

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When you download the student
version of thermo calc,

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they're giving you a very
minimal set of databases.

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First of all, you'd have
to pay a fair amount

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to get a larger set.

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But if you want to get the real
stuff, these are trade secrets.

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So companies like
Alcoa, they guard

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their thermodynamic databases
the way a company like Intel

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guards its lithography maps.

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It's like the key to
the entire operation.

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So the economic value of
data is huge in thermo

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and material science
more generally.

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Now, fortunately, we
don't need to sit down

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with our pen and
paper and figure out

00:11:46.020 --> 00:11:49.230 align:middle line:84%
what the law of thermodynamics
predict every time.

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We have software for that.

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So databases fed into software
allows you to make predictions

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and helps you make decisions
in a reasonable time frame.

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That's how you'll use
thermo in the real world.

00:12:00.735 --> 00:12:02.610 align:middle line:84%
This is how you use
thermo in the real world.

00:12:02.610 --> 00:12:12.590 align:middle line:90%


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OK, our next topic,
systems in thermodynamics.

00:12:18.870 --> 00:12:33.370 align:middle line:90%


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All right, systems
are characterized

00:12:36.880 --> 00:13:04.240 align:middle line:84%
by temperature, pressure,
volume, and composition, also

00:13:04.240 --> 00:13:05.050 align:middle line:90%
boundaries.

00:13:05.050 --> 00:13:10.980 align:middle line:90%


00:13:10.980 --> 00:13:12.060 align:middle line:90%
So here's an example.

00:13:12.060 --> 00:13:13.995 align:middle line:90%
Here is a balloon.

00:13:13.995 --> 00:13:20.543 align:middle line:90%


00:13:20.543 --> 00:13:21.335 align:middle line:90%
There's a boundary.

00:13:21.335 --> 00:13:25.610 align:middle line:90%


00:13:25.610 --> 00:13:27.170 align:middle line:90%
This is in.

00:13:27.170 --> 00:13:29.670 align:middle line:90%
And this is out.

00:13:29.670 --> 00:13:31.770 align:middle line:84%
All right, so let's say
we want to calculate

00:13:31.770 --> 00:13:35.470 align:middle line:84%
some properties of the gas
inside of this balloon.

00:13:35.470 --> 00:13:38.305 align:middle line:84%
What should we take as the
boundary of our system?

00:13:38.305 --> 00:13:43.817 align:middle line:90%


00:13:43.817 --> 00:13:45.400 align:middle line:84%
It's kind of painfully
obvious, right?

00:13:45.400 --> 00:13:48.767 align:middle line:90%


00:13:48.767 --> 00:13:50.180 align:middle line:90%
You take the plastic.

00:13:50.180 --> 00:13:52.940 align:middle line:84%
You take the actual balloon,
the actual balloon that-- you

00:13:52.940 --> 00:13:54.148 align:middle line:90%
choose that as your boundary.

00:13:54.148 --> 00:13:54.900 align:middle line:90%
That makes sense.

00:13:54.900 --> 00:13:57.530 align:middle line:84%
It's kind of obvious,
but it's good to start

00:13:57.530 --> 00:13:59.480 align:middle line:90%
from an obvious example.

00:13:59.480 --> 00:14:03.410 align:middle line:84%
Why do you choose
the physical balloon

00:14:03.410 --> 00:14:08.160 align:middle line:84%
as a boundary of your system
to analyze the gas inside?

00:14:08.160 --> 00:14:10.310 align:middle line:84%
Why not just choose
an arbitrary volume?

00:14:10.310 --> 00:14:14.450 align:middle line:84%
Why not say no, I'm going
to choose as my system

00:14:14.450 --> 00:14:15.830 align:middle line:90%
the lower half of the balloon?

00:14:15.830 --> 00:14:21.372 align:middle line:84%
And this is an imaginary
line or surface separating

00:14:21.372 --> 00:14:22.580 align:middle line:90%
the two parts of the balloon.

00:14:22.580 --> 00:14:27.742 align:middle line:84%
Why not choose this
lower volume to analyze?

00:14:27.742 --> 00:14:29.700 align:middle line:84%
AUDIENCE: Because there's
nothing separating it

00:14:29.700 --> 00:14:31.010 align:middle line:90%
from the upper volume of gas.

00:14:31.010 --> 00:14:33.010 align:middle line:84%
RAFAEL JARAMILLO: There's
nothing separating it.

00:14:33.010 --> 00:14:35.950 align:middle line:84%
And so as a result,
particles can

00:14:35.950 --> 00:14:38.900 align:middle line:84%
move between the lower
volume and the upper volume.

00:14:38.900 --> 00:14:41.500 align:middle line:84%
So if I choose
the whole balloon,

00:14:41.500 --> 00:14:46.080 align:middle line:84%
I get to use conservation
of particle number.

00:14:46.080 --> 00:14:48.440 align:middle line:90%
That's convenient.

00:14:48.440 --> 00:14:50.570 align:middle line:84%
If I now treat these
as two subsystems--

00:14:50.570 --> 00:14:52.580 align:middle line:90%
system A and system B--

00:14:52.580 --> 00:14:56.770 align:middle line:84%
now I need to keep track of
how they exchange particles.

00:14:56.770 --> 00:14:59.410 align:middle line:90%
It's more work.

00:14:59.410 --> 00:15:02.420 align:middle line:84%
We get the same answer if you
do it, but it's more work.

00:15:02.420 --> 00:15:05.440 align:middle line:84%
So this is, again, a
painfully obvious example.

00:15:05.440 --> 00:15:08.980 align:middle line:84%
But starting as
soon as this p set,

00:15:08.980 --> 00:15:11.140 align:middle line:84%
we hope to make it-- give
you some slightly less

00:15:11.140 --> 00:15:15.100 align:middle line:84%
obvious examples, which is
how you choose boundaries.

00:15:15.100 --> 00:15:19.190 align:middle line:84%
You draw-- you choose
boundaries-- boundaries chosen

00:15:19.190 --> 00:15:21.902 align:middle line:90%
out of convenience.

00:15:21.902 --> 00:15:27.890 align:middle line:90%


00:15:27.890 --> 00:15:31.220 align:middle line:84%
You choose a boundary when
you analyze a system to make

00:15:31.220 --> 00:15:32.940 align:middle line:90%
your life easier.

00:15:32.940 --> 00:15:35.895 align:middle line:84%
It depends on what
questions you're asking

00:15:35.895 --> 00:15:37.520 align:middle line:84%
So I believe in
problem 1 on the p set,

00:15:37.520 --> 00:15:39.937 align:middle line:84%
we asked you to run through
some of these mental exercises

00:15:39.937 --> 00:15:42.380 align:middle line:90%
for different examples--

00:15:42.380 --> 00:15:45.420 align:middle line:84%
right, boundaries chosen
out of convenience.

00:15:45.420 --> 00:15:48.050 align:middle line:90%
So let's do an example.

00:15:48.050 --> 00:15:51.660 align:middle line:90%


00:15:51.660 --> 00:16:06.160 align:middle line:84%
Example, adding sugar to a
glass of water and stirring.

00:16:06.160 --> 00:16:10.800 align:middle line:90%


00:16:10.800 --> 00:16:13.492 align:middle line:90%
So let's see.

00:16:13.492 --> 00:16:14.325 align:middle line:90%
Let's draw a beaker.

00:16:14.325 --> 00:16:22.260 align:middle line:90%


00:16:22.260 --> 00:16:28.910 align:middle line:90%
And there's water, good.

00:16:28.910 --> 00:16:31.360 align:middle line:90%
And here's sugar.

00:16:31.360 --> 00:16:39.520 align:middle line:90%


00:16:39.520 --> 00:16:41.470 align:middle line:84%
There's sugar, and
the sugar gets added.

00:16:41.470 --> 00:16:45.585 align:middle line:90%


00:16:45.585 --> 00:16:46.960 align:middle line:84%
And I'm going to
have a stir bar.

00:16:46.960 --> 00:16:47.860 align:middle line:90%
I have to stir.

00:16:47.860 --> 00:16:50.895 align:middle line:84%
So I have a stir bar-- a little
swizzle stick or something--

00:16:50.895 --> 00:16:55.450 align:middle line:90%


00:16:55.450 --> 00:16:58.390 align:middle line:84%
and stirring that
around so it's moving.

00:16:58.390 --> 00:17:01.790 align:middle line:90%


00:17:01.790 --> 00:17:02.530 align:middle line:90%
This is why.

00:17:02.530 --> 00:17:05.859 align:middle line:90%


00:17:05.859 --> 00:17:06.359 align:middle line:90%
All right.

00:17:06.359 --> 00:17:09.857 align:middle line:90%


00:17:09.857 --> 00:17:11.065 align:middle line:90%
Let's talk about this system.

00:17:11.065 --> 00:17:13.536 align:middle line:90%


00:17:13.536 --> 00:17:15.369 align:middle line:84%
First, I'm going to
write down a list of all

00:17:15.369 --> 00:17:17.300 align:middle line:90%
the things in this picture.

00:17:17.300 --> 00:17:27.619 align:middle line:84%
So the things are water, sugar,
the glass, the atmosphere--

00:17:27.619 --> 00:17:30.930 align:middle line:84%
I didn't really draw
it, but it's there--

00:17:30.930 --> 00:17:32.730 align:middle line:84%
and the stir stick
and the stir bar.

00:17:32.730 --> 00:17:35.280 align:middle line:90%


00:17:35.280 --> 00:17:40.410 align:middle line:84%
I want to get an answer like
how sweet will the water become?

00:17:40.410 --> 00:17:42.180 align:middle line:90%
That's the answer I need.

00:17:42.180 --> 00:17:44.968 align:middle line:84%
What system-- so to analyze,
what should be in the system,

00:17:44.968 --> 00:17:46.510 align:middle line:84%
and what should not
be in the system?

00:17:46.510 --> 00:17:50.330 align:middle line:84%
So would somebody say should
the water be in the system?

00:17:50.330 --> 00:17:52.880 align:middle line:84%
AUDIENCE: Yes, because it's
one of the main components

00:17:52.880 --> 00:17:53.687 align:middle line:90%
of all the mixture.

00:17:53.687 --> 00:17:56.270 align:middle line:84%
RAFAEL JARAMILLO: Yeah, OK, so
we're going to choose the water

00:17:56.270 --> 00:17:57.712 align:middle line:90%
and the sugar I will say also.

00:17:57.712 --> 00:17:59.670 align:middle line:84%
It's one of the main
components of the mixture.

00:17:59.670 --> 00:18:00.560 align:middle line:90%
So let's go.

00:18:00.560 --> 00:18:01.775 align:middle line:90%
What about the glass?

00:18:01.775 --> 00:18:03.830 align:middle line:84%
Should that be
part of the system?

00:18:03.830 --> 00:18:05.900 align:middle line:90%
AUDIENCE: No.

00:18:05.900 --> 00:18:07.640 align:middle line:84%
RAFAEL JARAMILLO:
Probably not, unless we

00:18:07.640 --> 00:18:10.280 align:middle line:84%
expect some kind of maybe
reaction with the glass.

00:18:10.280 --> 00:18:14.690 align:middle line:84%
But the sugar water, it's
not going to etch the glass.

00:18:14.690 --> 00:18:16.440 align:middle line:84%
If this were a hydrogen
fluoride solution,

00:18:16.440 --> 00:18:17.130 align:middle line:90%
it would etch the glass.

00:18:17.130 --> 00:18:18.090 align:middle line:90%
We'd have to include the glass.

00:18:18.090 --> 00:18:19.798 align:middle line:84%
But we're not going
to include the glass.

00:18:19.798 --> 00:18:23.710 align:middle line:84%
The atmosphere-- do we
have to include that?

00:18:23.710 --> 00:18:25.750 align:middle line:84%
AUDIENCE: No, because
it's not changing.

00:18:25.750 --> 00:18:27.880 align:middle line:84%
RAFAEL JARAMILLO:
Yeah, if this is just

00:18:27.880 --> 00:18:30.280 align:middle line:84%
something you're doing in
your kitchen, probably not.

00:18:30.280 --> 00:18:34.630 align:middle line:84%
If you're running a
factory making sugar water,

00:18:34.630 --> 00:18:36.005 align:middle line:84%
like a simple
syrup or something,

00:18:36.005 --> 00:18:38.505 align:middle line:84%
you probably want to include
the atmosphere because you want

00:18:38.505 --> 00:18:39.880 align:middle line:90%
really good process control.

00:18:39.880 --> 00:18:41.530 align:middle line:84%
And the humidity
in the atmosphere

00:18:41.530 --> 00:18:42.710 align:middle line:90%
might make a difference.

00:18:42.710 --> 00:18:43.630 align:middle line:90%
That's an example.

00:18:43.630 --> 00:18:50.590 align:middle line:84%
Or if you're a monk
brewing a farmhouse ale--

00:18:50.590 --> 00:18:53.260 align:middle line:84%
and we know that the stuff in
the air from the surrounding

00:18:53.260 --> 00:18:55.833 align:middle line:84%
farms makes it into the
beer and helps change.

00:18:55.833 --> 00:18:57.250 align:middle line:84%
So there are
examples where you do

00:18:57.250 --> 00:18:59.708 align:middle line:84%
want to include the atmosphere
in the system, but here not.

00:18:59.708 --> 00:19:00.732 align:middle line:90%
And the stir bar, not--

00:19:00.732 --> 00:19:02.440 align:middle line:84%
the stir bar has a
function, but it's not

00:19:02.440 --> 00:19:05.640 align:middle line:84%
going to be a part of
the thermodynamic system.

00:19:05.640 --> 00:19:06.990 align:middle line:90%
What about the boundaries?

00:19:06.990 --> 00:19:09.690 align:middle line:90%


00:19:09.690 --> 00:19:12.960 align:middle line:84%
All right, these are
the types of boundaries.

00:19:12.960 --> 00:19:33.620 align:middle line:90%


00:19:33.620 --> 00:19:35.420 align:middle line:84%
And before we go
through these, this

00:19:35.420 --> 00:19:39.050 align:middle line:84%
is as good a time as any to
remind you that the associated

00:19:39.050 --> 00:19:41.592 align:middle line:84%
reading is every
bit as much a part

00:19:41.592 --> 00:19:42.800 align:middle line:90%
of the course as the lecture.

00:19:42.800 --> 00:19:44.690 align:middle line:84%
So if you keep up
with the reading

00:19:44.690 --> 00:19:47.570 align:middle line:84%
and do the associated
reading before lecture,

00:19:47.570 --> 00:19:50.375 align:middle line:84%
you'll get a lot more out
of the entire experience.

00:19:50.375 --> 00:19:52.250 align:middle line:84%
So thank you for keeping
up with the reading.

00:19:52.250 --> 00:19:55.280 align:middle line:84%
All right, boundaries--
open or closed?

00:19:55.280 --> 00:19:56.930 align:middle line:90%
Somebody please tell me.

00:19:56.930 --> 00:19:58.190 align:middle line:90%
Is this open or closed system?

00:19:58.190 --> 00:20:01.850 align:middle line:90%
Which would you choose and why?

00:20:01.850 --> 00:20:04.610 align:middle line:84%
And what does that
mean, open or closed?

00:20:04.610 --> 00:20:07.070 align:middle line:90%
Somebody.

00:20:07.070 --> 00:20:09.860 align:middle line:84%
AUDIENCE: I would say it
was closed because nothing

00:20:09.860 --> 00:20:11.240 align:middle line:90%
is leaving the system.

00:20:11.240 --> 00:20:14.180 align:middle line:84%
There's no evaporation
happening or particles leaving.

00:20:14.180 --> 00:20:16.790 align:middle line:84%
RAFAEL JARAMILLO: Good, OK,
that's what I would choose too.

00:20:16.790 --> 00:20:19.310 align:middle line:84%
Closed means no
loss of particles

00:20:19.310 --> 00:20:20.990 align:middle line:90%
or no gain of particles.

00:20:20.990 --> 00:20:22.770 align:middle line:84%
Particle number
remains the same.

00:20:22.770 --> 00:20:25.640 align:middle line:84%
So the example given
there was that if you

00:20:25.640 --> 00:20:27.320 align:middle line:90%
included evaporation--

00:20:27.320 --> 00:20:31.483 align:middle line:84%
loss of water-- it
would be an open system.

00:20:31.483 --> 00:20:33.650 align:middle line:84%
You'd have to include the
atmosphere in your system.

00:20:33.650 --> 00:20:36.362 align:middle line:90%


00:20:36.362 --> 00:20:38.570 align:middle line:84%
And if you're growing-- if
you're in a crystal growth

00:20:38.570 --> 00:20:43.460 align:middle line:84%
experiment where you slowly
let the water evaporate--

00:20:43.460 --> 00:20:48.178 align:middle line:84%
the supernatant-- then
it's an open system.

00:20:48.178 --> 00:20:50.220 align:middle line:84%
But we're doing this
quickly, and we're not going

00:20:50.220 --> 00:20:51.428 align:middle line:90%
to wait for water evaporates.

00:20:51.428 --> 00:20:52.470 align:middle line:90%
So closed, thank you.

00:20:52.470 --> 00:20:56.590 align:middle line:90%
All right, rigid or not rigid?

00:20:56.590 --> 00:21:00.190 align:middle line:84%
AUDIENCE: Maybe not
rigid since the top is,

00:21:00.190 --> 00:21:04.520 align:middle line:84%
like not like a
hard solid surface.

00:21:04.520 --> 00:21:05.720 align:middle line:90%
RAFAEL JARAMILLO: OK, good.

00:21:05.720 --> 00:21:08.000 align:middle line:90%
So the top, it's not rigid.

00:21:08.000 --> 00:21:11.400 align:middle line:84%
That's what I would choose too
Let's talk a little bit more

00:21:11.400 --> 00:21:13.720 align:middle line:90%
about what that means.

00:21:13.720 --> 00:21:16.380 align:middle line:84%
It means that the
volume can change.

00:21:16.380 --> 00:21:17.955 align:middle line:90%
The volume is free to change.

00:21:17.955 --> 00:21:19.080 align:middle line:90%
That's what was said there.

00:21:19.080 --> 00:21:21.130 align:middle line:90%
The top is not a hard surface.

00:21:21.130 --> 00:21:24.220 align:middle line:84%
So we assume that the walls
of the glass are rigid.

00:21:24.220 --> 00:21:25.630 align:middle line:90%
They're not going to change.

00:21:25.630 --> 00:21:28.680 align:middle line:84%
But the top surface is
what's called a free surface.

00:21:28.680 --> 00:21:32.930 align:middle line:84%
It can exchange volume
with the atmosphere.

00:21:32.930 --> 00:21:36.540 align:middle line:84%
And the ability to
exchange volume--

00:21:36.540 --> 00:21:38.580 align:middle line:84%
that's the mechanism
by which two systems

00:21:38.580 --> 00:21:40.630 align:middle line:90%
arrive at the same pressure.

00:21:40.630 --> 00:21:42.990 align:middle line:84%
So there's notion of
pressure regulation.

00:21:42.990 --> 00:21:47.920 align:middle line:84%
Temperature regulation becomes
very important in thermo.

00:21:47.920 --> 00:21:52.090 align:middle line:84%
Non rigid systems are
pressure regulated

00:21:52.090 --> 00:21:54.430 align:middle line:84%
because they can exchange
volume with the atmosphere.

00:21:54.430 --> 00:21:56.920 align:middle line:84%
If there is a fluctuation
in atmospheric pressure,

00:21:56.920 --> 00:21:59.350 align:middle line:84%
that same temperature-- the
same pressure fluctuation

00:21:59.350 --> 00:22:03.440 align:middle line:84%
will be felt by the
water bath, for instance.

00:22:03.440 --> 00:22:06.020 align:middle line:84%
As opposed to a rigid
system, a rigid system

00:22:06.020 --> 00:22:07.010 align:middle line:90%
can build pressure.

00:22:07.010 --> 00:22:09.410 align:middle line:84%
You can have a bomb or
a high pressure vessel.

00:22:09.410 --> 00:22:11.460 align:middle line:84%
That's a different
pressure from the outside.

00:22:11.460 --> 00:22:11.960 align:middle line:90%
Why?

00:22:11.960 --> 00:22:13.813 align:middle line:84%
Because it's fixed
volume, rigid.

00:22:13.813 --> 00:22:14.480 align:middle line:90%
All right, good.

00:22:14.480 --> 00:22:17.150 align:middle line:84%
And finally, adiabatic
or diathermal?

00:22:17.150 --> 00:22:26.502 align:middle line:90%


00:22:26.502 --> 00:22:28.210 align:middle line:84%
Right, so the non
rigid meant that you're

00:22:28.210 --> 00:22:32.450 align:middle line:84%
going to be at atmospheric
pressure throughout.

00:22:32.450 --> 00:22:37.310 align:middle line:84%
In my view, the Zoom
video camera webcam review

00:22:37.310 --> 00:22:40.850 align:middle line:84%
is blocking this
text right here.

00:22:40.850 --> 00:22:43.940 align:middle line:84%
Is it blocking this text
in anyone else's view?

00:22:43.940 --> 00:22:44.850 align:middle line:90%
AUDIENCE: No.

00:22:44.850 --> 00:22:45.260 align:middle line:90%
RAFAEL JARAMILLO: OK, good.

00:22:45.260 --> 00:22:45.760 align:middle line:90%
Thanks.

00:22:45.760 --> 00:22:47.930 align:middle line:84%
All right, so what about
adiabatic or diathermal?

00:22:47.930 --> 00:22:50.481 align:middle line:84%
Is this adiabatic,
or is it diathermal?

00:22:50.481 --> 00:22:56.170 align:middle line:84%
The boundaries--
adiabatic or diathermal?

00:22:56.170 --> 00:23:00.010 align:middle line:84%
So adiabatic means a
process or a boundary

00:23:00.010 --> 00:23:03.190 align:middle line:90%
that does not allow heating--

00:23:03.190 --> 00:23:05.260 align:middle line:84%
so a thermally
insulating battery.

00:23:05.260 --> 00:23:08.805 align:middle line:90%


00:23:08.805 --> 00:23:09.930 align:middle line:90%
Diathermal is the opposite.

00:23:09.930 --> 00:23:12.660 align:middle line:84%
Diathermal thermal is
a process or a boundary

00:23:12.660 --> 00:23:16.740 align:middle line:84%
that allows heating, allows heat
to flow, allows heat exchange.

00:23:16.740 --> 00:23:18.210 align:middle line:90%
AUDIENCE: So it'd be diathermal.

00:23:18.210 --> 00:23:20.043 align:middle line:84%
RAFAEL JARAMILLO: It'd
be diathermal, right.

00:23:20.043 --> 00:23:27.940 align:middle line:84%
So in the same way that the free
surface allows the atmosphere

00:23:27.940 --> 00:23:30.160 align:middle line:84%
to regulate the
pressure in the water,

00:23:30.160 --> 00:23:32.140 align:middle line:84%
keeping it at
atmospheric pressure

00:23:32.140 --> 00:23:37.220 align:middle line:84%
throughout, the diathermal
boundaries in glass

00:23:37.220 --> 00:23:38.667 align:middle line:90%
might be a little slow--

00:23:38.667 --> 00:23:40.250 align:middle line:84%
slow thermal transport,
but definitely

00:23:40.250 --> 00:23:43.070 align:middle line:84%
have a very fast thermal
transport there at the surface.

00:23:43.070 --> 00:23:47.278 align:middle line:84%
This is going to
keep temperature

00:23:47.278 --> 00:23:49.070 align:middle line:84%
of the room-- this is
the temperature there

00:23:49.070 --> 00:23:50.483 align:middle line:90%
the room throughout.

00:23:50.483 --> 00:23:54.433 align:middle line:90%


00:23:54.433 --> 00:23:55.850 align:middle line:84%
So the diathermal
thermal boundary

00:23:55.850 --> 00:23:57.170 align:middle line:90%
regulates the temperature.

00:23:57.170 --> 00:23:59.855 align:middle line:84%
The non rigid boundary
regulates the pressure.

00:23:59.855 --> 00:24:03.160 align:middle line:90%


00:24:03.160 --> 00:24:05.705 align:middle line:84%
I'm taking my time here,
intentionally introducing

00:24:05.705 --> 00:24:06.580 align:middle line:90%
a bunch of new terms.

00:24:06.580 --> 00:24:11.110 align:middle line:84%
Or if they're not new terms,
the meaning of all these terms

00:24:11.110 --> 00:24:14.320 align:middle line:84%
is very specific in thermo,
so the idea of regulation,

00:24:14.320 --> 00:24:15.760 align:middle line:90%
the idea of choosing boundaries.

00:24:15.760 --> 00:24:19.540 align:middle line:90%


00:24:19.540 --> 00:24:22.690 align:middle line:84%
So you'll do some examples
like this in the p set.

00:24:22.690 --> 00:24:25.825 align:middle line:90%


00:24:25.825 --> 00:24:27.700 align:middle line:84%
All right, let's talk
about types of systems,

00:24:27.700 --> 00:24:28.533 align:middle line:90%
classifying systems.

00:24:28.533 --> 00:24:36.180 align:middle line:90%


00:24:36.180 --> 00:24:37.260 align:middle line:90%
Classifications.

00:24:37.260 --> 00:24:43.940 align:middle line:90%


00:24:43.940 --> 00:24:46.040 align:middle line:84%
All right, so this is just
getting some essentials

00:24:46.040 --> 00:24:47.270 align:middle line:90%
out of the way here--

00:24:47.270 --> 00:24:53.471 align:middle line:90%
unary, one component.

00:24:53.471 --> 00:24:57.620 align:middle line:90%


00:24:57.620 --> 00:25:00.955 align:middle line:84%
All right, so an example of
a component would be water.

00:25:00.955 --> 00:25:27.940 align:middle line:90%


00:25:27.940 --> 00:25:29.050 align:middle line:90%
OK, so here's an example.

00:25:29.050 --> 00:25:30.950 align:middle line:84%
A unary system
has one component,

00:25:30.950 --> 00:25:33.460 align:middle line:90%
one molecular component.

00:25:33.460 --> 00:25:35.290 align:middle line:84%
A multi component system
has more than one.

00:25:35.290 --> 00:25:38.830 align:middle line:84%
So, for example, the binary
system of water and sugar.

00:25:38.830 --> 00:25:43.820 align:middle line:90%


00:25:43.820 --> 00:25:45.820 align:middle line:84%
I've got hydrogen,
oxygen, and carbon here.

00:25:45.820 --> 00:25:47.590 align:middle line:84%
How come it's not
three components?

00:25:47.590 --> 00:25:48.190 align:middle line:90%
Anybody?

00:25:48.190 --> 00:25:52.252 align:middle line:90%


00:25:52.252 --> 00:25:54.460 align:middle line:84%
AUDIENCE: Because at no
point are we discussing like,

00:25:54.460 --> 00:25:56.858 align:middle line:84%
the separation of
those components.

00:25:56.858 --> 00:25:58.150 align:middle line:90%
RAFAEL JARAMILLO: That's right.

00:25:58.150 --> 00:26:02.260 align:middle line:84%
At no point are we breaking
bonds or in reforming

00:26:02.260 --> 00:26:02.800 align:middle line:90%
molecules.

00:26:02.800 --> 00:26:04.490 align:middle line:84%
This is remaining
water throughout.

00:26:04.490 --> 00:26:07.870 align:middle line:84%
This is remaining
sucrose throughout.

00:26:07.870 --> 00:26:11.480 align:middle line:84%
This is not a digestive system,
and you break down the sugar.

00:26:11.480 --> 00:26:14.170 align:middle line:84%
This is not an electrochemical
water-splitting system

00:26:14.170 --> 00:26:18.280 align:middle line:84%
where you might be using
some source of energy

00:26:18.280 --> 00:26:22.480 align:middle line:84%
to electrochemically generate
hydrogen gas from water.

00:26:22.480 --> 00:26:23.950 align:middle line:90%
So that's good.

00:26:23.950 --> 00:26:27.600 align:middle line:84%
So your choice of
unary, multi component--

00:26:27.600 --> 00:26:30.090 align:middle line:84%
there can be more
than one answer.

00:26:30.090 --> 00:26:32.880 align:middle line:84%
And the same
molecular components

00:26:32.880 --> 00:26:35.890 align:middle line:84%
can be analyzed as unary,
or a multi component system,

00:26:35.890 --> 00:26:37.930 align:middle line:90%
depending on the situation.

00:26:37.930 --> 00:26:40.643 align:middle line:84%
So, again, you make these
decisions out of convenience

00:26:40.643 --> 00:26:42.060 align:middle line:84%
because you
understand the process

00:26:42.060 --> 00:26:44.810 align:middle line:84%
that you're engineering,
that you're designing.

00:26:44.810 --> 00:26:50.940 align:middle line:84%
All right, OK, good, so that's
urinary versus multi component.

00:26:50.940 --> 00:26:52.815 align:middle line:84%
And this kind of
gets-- sometimes

00:26:52.815 --> 00:26:55.770 align:middle line:84%
can get a little bit easy
to get tripped up there.

00:26:55.770 --> 00:27:03.170 align:middle line:84%
All right, two different types
of classification-- homogeneous

00:27:03.170 --> 00:27:05.090 align:middle line:90%
first, heterogeneous.

00:27:05.090 --> 00:27:09.280 align:middle line:90%


00:27:09.280 --> 00:27:11.050 align:middle line:90%
So homogeneous means one phase.

00:27:11.050 --> 00:27:15.200 align:middle line:90%


00:27:15.200 --> 00:27:20.210 align:middle line:84%
So, for example,
sodium acetate--

00:27:20.210 --> 00:27:28.090 align:middle line:90%


00:27:28.090 --> 00:27:29.530 align:middle line:90%
the sodium acetate solution.

00:27:29.530 --> 00:27:34.600 align:middle line:84%
That was-- the supersaturated
sodium acetate solution

00:27:34.600 --> 00:27:39.380 align:middle line:84%
was a starting point
for the incident

00:27:39.380 --> 00:27:42.840 align:middle line:84%
and hot plate, sodium
acetate solution.

00:27:42.840 --> 00:27:45.160 align:middle line:90%
What about heterogeneous?

00:27:45.160 --> 00:27:59.270 align:middle line:84%
More than one phase,
right-- solution plus solid,

00:27:59.270 --> 00:28:00.811 align:middle line:90%
sodium acetate.

00:28:00.811 --> 00:28:04.740 align:middle line:90%


00:28:04.740 --> 00:28:12.160 align:middle line:84%
So that's-- because I think a
little bit less description.

00:28:12.160 --> 00:28:13.570 align:middle line:90%
What about closed versus open?

00:28:13.570 --> 00:28:22.130 align:middle line:90%


00:28:22.130 --> 00:28:23.990 align:middle line:90%
This we've already discussed--

00:28:23.990 --> 00:28:45.490 align:middle line:84%
no mass exchange with
surroundings versus

00:28:45.490 --> 00:28:47.260 align:middle line:84%
can exchange mass
with surroundings.

00:28:47.260 --> 00:28:54.580 align:middle line:90%


00:28:54.580 --> 00:28:57.310 align:middle line:84%
So those are some basic and
important classifications.

00:28:57.310 --> 00:29:01.810 align:middle line:90%


00:29:01.810 --> 00:29:05.260 align:middle line:84%
Next category-- we're going
through the necessary stuff

00:29:05.260 --> 00:29:08.530 align:middle line:84%
here to get started on
real thermal problems.

00:29:08.530 --> 00:29:14.240 align:middle line:84%
State functions or, if
you like, variables.

00:29:14.240 --> 00:29:19.470 align:middle line:84%
We'll use these interchangeably,
state functions and state

00:29:19.470 --> 00:29:20.405 align:middle line:90%
variables.

00:29:20.405 --> 00:29:21.780 align:middle line:84%
So these characterize
the system.

00:29:21.780 --> 00:29:35.240 align:middle line:90%


00:29:35.240 --> 00:29:36.890 align:middle line:90%
They are independent of history.

00:29:36.890 --> 00:29:47.110 align:middle line:90%


00:29:47.110 --> 00:29:51.250 align:middle line:90%
This is a really subtle point.

00:29:51.250 --> 00:29:52.180 align:middle line:90%
This will trip you up.

00:29:52.180 --> 00:29:53.830 align:middle line:90%
It trips me up.

00:29:53.830 --> 00:29:56.610 align:middle line:90%
It seems obvious, right.

00:29:56.610 --> 00:29:59.430 align:middle line:84%
The fact that you could
characterize a system

00:29:59.430 --> 00:30:01.680 align:middle line:84%
with variables which are
independent of the history

00:30:01.680 --> 00:30:04.560 align:middle line:84%
of that system is
very non obvious.

00:30:04.560 --> 00:30:07.860 align:middle line:84%
That was a major
intellectual accomplishment.

00:30:07.860 --> 00:30:10.050 align:middle line:84%
It shouldn't sit
easily with you.

00:30:10.050 --> 00:30:11.520 align:middle line:90%
That takes some getting used to.

00:30:11.520 --> 00:30:13.050 align:middle line:84%
You shouldn't trust
me on this yet.

00:30:13.050 --> 00:30:16.240 align:middle line:90%


00:30:16.240 --> 00:30:31.580 align:middle line:84%
Common state functions
found in 020--

00:30:31.580 --> 00:30:36.350 align:middle line:84%
so would somebody like to
volunteer a state function,

00:30:36.350 --> 00:30:39.630 align:middle line:84%
a common state function
you might find in thermo?

00:30:39.630 --> 00:30:40.560 align:middle line:90%
AUDIENCE: Temperature

00:30:40.560 --> 00:30:41.768 align:middle line:90%
RAFAEL JARAMILLO: Yeah, temp.

00:30:41.768 --> 00:30:44.310 align:middle line:90%
So that's a state function.

00:30:44.310 --> 00:30:46.415 align:middle line:90%
We use t.

00:30:46.415 --> 00:30:56.360 align:middle line:84%
To denote volume, we
use v. Pressure is p.

00:30:56.360 --> 00:30:59.280 align:middle line:90%
Any others?

00:30:59.280 --> 00:31:01.168 align:middle line:90%
AUDIENCE: Enthalpy.

00:31:01.168 --> 00:31:02.460 align:middle line:90%
RAFAEL JARAMILLO: Enthalpy, OK.

00:31:02.460 --> 00:31:03.460 align:middle line:90%
That's a state function.

00:31:03.460 --> 00:31:11.070 align:middle line:90%


00:31:11.070 --> 00:31:15.360 align:middle line:84%
What about one that's not
so specific in thermo?

00:31:15.360 --> 00:31:18.600 align:middle line:84%
Are there others that
are more colloquial?

00:31:18.600 --> 00:31:19.620 align:middle line:90%
AUDIENCE: Concentration.

00:31:19.620 --> 00:31:21.870 align:middle line:84%
RAFAEL JARAMILLO: Concentration,
I'll say composition.

00:31:21.870 --> 00:31:31.420 align:middle line:84%
Yeah, composition-- and we'll
use atomic percent often

00:31:31.420 --> 00:31:33.460 align:middle line:90%
in this class.

00:31:33.460 --> 00:31:42.647 align:middle line:84%
What about mole number,
total system size, like that?

00:31:42.647 --> 00:31:43.730 align:middle line:90%
And then there's enthalpy.

00:31:43.730 --> 00:31:47.920 align:middle line:84%
And then there are
others which are more

00:31:47.920 --> 00:31:49.270 align:middle line:90%
specific to thermodynamics.

00:31:49.270 --> 00:31:51.022 align:middle line:90%
There's entropy.

00:31:51.022 --> 00:31:52.105 align:middle line:90%
There's Gibbs free energy.

00:31:52.105 --> 00:31:59.030 align:middle line:90%


00:31:59.030 --> 00:32:00.500 align:middle line:84%
And there's Helmholtz
free energy.

00:32:00.500 --> 00:32:14.510 align:middle line:90%


00:32:14.510 --> 00:32:15.800 align:middle line:90%
If we were course 2--

00:32:15.800 --> 00:32:18.500 align:middle line:84%
if we were mechanical
engineers--

00:32:18.500 --> 00:32:27.480 align:middle line:84%
we would be spending a lot more
time on Helmholtz free energy

00:32:27.480 --> 00:32:30.140 align:middle line:90%
and enthalpy.

00:32:30.140 --> 00:32:31.880 align:middle line:84%
If we were physicists,
we'd be spending

00:32:31.880 --> 00:32:34.680 align:middle line:84%
a lot more time on
Helmholtz free energy

00:32:34.680 --> 00:32:42.160 align:middle line:84%
and energy, which we're going
to use u for internal energy.

00:32:42.160 --> 00:32:43.840 align:middle line:84%
But as material
scientists, we spend

00:32:43.840 --> 00:32:49.330 align:middle line:84%
most of our time on Gibbs free
energy and enthalpy for reasons

00:32:49.330 --> 00:32:52.900 align:middle line:84%
that we'll discuss at length
in a couple of lectures.

00:32:52.900 --> 00:32:53.770 align:middle line:90%
But there are more.

00:32:53.770 --> 00:32:55.270 align:middle line:90%
There are more.

00:32:55.270 --> 00:32:59.710 align:middle line:84%
Like magnetization, that's
one we don't-- that electric

00:32:59.710 --> 00:33:01.240 align:middle line:90%
polarization.

00:33:01.240 --> 00:33:01.870 align:middle line:90%
There're many.

00:33:01.870 --> 00:33:08.068 align:middle line:90%


00:33:08.068 --> 00:33:09.360 align:middle line:90%
OK, so we have state functions.

00:33:09.360 --> 00:33:10.780 align:middle line:90%
We have state variables.

00:33:10.780 --> 00:33:12.630 align:middle line:90%
We also have equations of state.

00:33:12.630 --> 00:33:20.690 align:middle line:90%


00:33:20.690 --> 00:33:22.760 align:middle line:84%
So an equation of
state, in general,

00:33:22.760 --> 00:33:27.940 align:middle line:84%
is some state function X equals
a function of other state

00:33:27.940 --> 00:33:32.695 align:middle line:90%
functions Y1, Y2, Y3.

00:33:32.695 --> 00:33:35.350 align:middle line:90%


00:33:35.350 --> 00:33:42.100 align:middle line:84%
And in this formulism,
that's a state function.

00:33:42.100 --> 00:33:46.250 align:middle line:90%
And these are state variables.

00:33:46.250 --> 00:33:48.770 align:middle line:84%
But I'm going to use this
interchangeably-- state

00:33:48.770 --> 00:33:50.420 align:middle line:90%
functions, state variables.

00:33:50.420 --> 00:33:54.282 align:middle line:84%
All right, so you all
know one state function.

00:33:54.282 --> 00:33:55.740 align:middle line:84%
What's the state
function everybody

00:33:55.740 --> 00:33:56.907 align:middle line:90%
knows, even on the T-shirts?

00:33:56.907 --> 00:34:00.525 align:middle line:90%


00:34:00.525 --> 00:34:01.900 align:middle line:84%
When I do this
lecture in person,

00:34:01.900 --> 00:34:05.100 align:middle line:84%
I wear my MIT T-shirt with
a state function on it.

00:34:05.100 --> 00:34:08.440 align:middle line:90%


00:34:08.440 --> 00:34:09.699 align:middle line:90%
AUDIENCE: It'd be PV=nRT.

00:34:09.699 --> 00:34:11.290 align:middle line:84%
RAFAEL JARAMILLO:
Yeah, PV=nRT, right.

00:34:11.290 --> 00:34:15.989 align:middle line:90%
PV equals nRT.

00:34:15.989 --> 00:34:18.310 align:middle line:90%
OK, so that's a state function.

00:34:18.310 --> 00:34:20.469 align:middle line:84%
That's a state function
for an ideal gas.

00:34:20.469 --> 00:34:24.760 align:middle line:84%
This is true always for an
ideal gas at equilibrium.

00:34:24.760 --> 00:34:28.675 align:middle line:84%
That's pretty cool, and
you can do a lot with that.

00:34:28.675 --> 00:34:30.050 align:middle line:84%
But before we do
a lot with that,

00:34:30.050 --> 00:34:34.409 align:middle line:84%
I want to warn you this is the
exception rather than the rule.

00:34:34.409 --> 00:34:37.530 align:middle line:84%
For almost every
system, every material

00:34:37.530 --> 00:34:39.120 align:middle line:84%
which you'll use
in your careers,

00:34:39.120 --> 00:34:42.989 align:middle line:84%
we do not have a state
function like this.

00:34:42.989 --> 00:34:46.960 align:middle line:84%
Maybe we have some that
are empirically determined.

00:34:46.960 --> 00:34:49.780 align:middle line:84%
You might find some magnetic
systems for which state

00:34:49.780 --> 00:34:51.550 align:middle line:84%
functions have been
exactly derived

00:34:51.550 --> 00:34:54.642 align:middle line:84%
from fundamental
principles like this one.

00:34:54.642 --> 00:34:56.600 align:middle line:84%
But this is the exception
rather than the rule.

00:34:56.600 --> 00:34:59.440 align:middle line:84%
Usually, you can't write
down a closed form like this.

00:34:59.440 --> 00:35:04.240 align:middle line:84%
Usually, you have to deal with
much more complicated data

00:35:04.240 --> 00:35:05.050 align:middle line:90%
resources.

00:35:05.050 --> 00:35:08.770 align:middle line:90%


00:35:08.770 --> 00:35:10.690 align:middle line:90%
Something on units here--

00:35:10.690 --> 00:35:12.460 align:middle line:90%
try to sneak this in.

00:35:12.460 --> 00:35:17.910 align:middle line:90%
R equals PV over nT.

00:35:17.910 --> 00:35:21.210 align:middle line:90%
What are the units of that?

00:35:21.210 --> 00:35:24.930 align:middle line:90%
Pressure is Pascals.

00:35:24.930 --> 00:35:27.930 align:middle line:90%
Volume is meters cubed--

00:35:27.930 --> 00:35:31.270 align:middle line:84%
make this so that it
looks like Pascals.

00:35:31.270 --> 00:35:33.817 align:middle line:90%
Mole is unitless, just a number.

00:35:33.817 --> 00:35:34.900 align:middle line:90%
And temperature is Kelvin.

00:35:34.900 --> 00:35:37.500 align:middle line:90%


00:35:37.500 --> 00:35:40.050 align:middle line:84%
In fundamental SI
units, a Pascal

00:35:40.050 --> 00:35:42.360 align:middle line:90%
is a Newton per meter squared.

00:35:42.360 --> 00:35:45.180 align:middle line:84%
Force over area,
that's pressure.

00:35:45.180 --> 00:35:49.670 align:middle line:84%
We have a meter cubed,
and we have a Kelvin.

00:35:49.670 --> 00:35:54.500 align:middle line:84%
So then, you get
Newton meter by--

00:35:54.500 --> 00:35:58.310 align:middle line:84%
and what's a force displaced
over a meter, Newton meter?

00:35:58.310 --> 00:36:01.650 align:middle line:90%


00:36:01.650 --> 00:36:03.780 align:middle line:90%
AUDIENCE: The joule.

00:36:03.780 --> 00:36:05.610 align:middle line:84%
RAFAEL JARAMILLO:
Joule, joule Kelvin.

00:36:05.610 --> 00:36:11.833 align:middle line:84%
So R equals 8.314
joules per Kelvin.

00:36:11.833 --> 00:36:13.125 align:middle line:90%
It's a handy thing to remember.

00:36:13.125 --> 00:36:16.253 align:middle line:90%


00:36:16.253 --> 00:36:18.420 align:middle line:84%
We're going to be sticklers
for units in this stuff.

00:36:18.420 --> 00:36:21.140 align:middle line:90%


00:36:21.140 --> 00:36:23.160 align:middle line:90%
I was going to say more things--

00:36:23.160 --> 00:36:24.510 align:middle line:90%
thermodynamic properties.

00:36:24.510 --> 00:36:36.420 align:middle line:90%


00:36:36.420 --> 00:36:37.920 align:middle line:84%
All right, so at
the very beginning,

00:36:37.920 --> 00:36:41.960 align:middle line:84%
I told you that states of
matter had certain responses

00:36:41.960 --> 00:36:45.860 align:middle line:84%
when you squeeze them or you
added stuff or you heated them.

00:36:45.860 --> 00:36:54.100 align:middle line:84%
And these are going
to be described

00:36:54.100 --> 00:36:56.750 align:middle line:84%
by thermodynamic
response functions.

00:36:56.750 --> 00:36:59.650 align:middle line:84%
So that response function
term sounds kind of fancy.

00:36:59.650 --> 00:37:00.820 align:middle line:90%
Don't let it scare you.

00:37:00.820 --> 00:37:03.700 align:middle line:84%
It describes how a system
responds to something.

00:37:03.700 --> 00:37:05.670 align:middle line:84%
So someone screams,
you cover your ear.

00:37:05.670 --> 00:37:07.520 align:middle line:90%
That's your response function.

00:37:07.520 --> 00:37:12.330 align:middle line:84%
So some common response
functions that we use in thermo

00:37:12.330 --> 00:37:25.460 align:middle line:84%
are compressibility, isothermal
compressibility, a fixed

00:37:25.460 --> 00:37:26.546 align:middle line:90%
temperature.

00:37:26.546 --> 00:37:31.110 align:middle line:90%


00:37:31.110 --> 00:37:34.560 align:middle line:84%
And, of course, this is
the same as d log V dP.

00:37:34.560 --> 00:37:35.640 align:middle line:90%
So you see this a lot.

00:37:35.640 --> 00:37:42.400 align:middle line:90%


00:37:42.400 --> 00:37:44.860 align:middle line:84%
The only real
prerequisite for thermo

00:37:44.860 --> 00:37:47.517 align:middle line:90%
is multivariable calculus.

00:37:47.517 --> 00:37:49.850 align:middle line:84%
And I think the first time I
learned thermo and probably

00:37:49.850 --> 00:37:52.580 align:middle line:84%
a second time even,
I didn't appreciate

00:37:52.580 --> 00:37:55.760 align:middle line:84%
just how much I relied on
multivariable calculus.

00:37:55.760 --> 00:37:58.550 align:middle line:84%
So just know that now so that
you're not surprised later.

00:37:58.550 --> 00:38:01.350 align:middle line:90%


00:38:01.350 --> 00:38:03.610 align:middle line:90%
All right, thermal expansion--

00:38:03.610 --> 00:38:04.690 align:middle line:90%
it's another common one.

00:38:04.690 --> 00:38:10.550 align:middle line:90%


00:38:10.550 --> 00:38:13.340 align:middle line:84%
Alpha equals--
again, we're going

00:38:13.340 --> 00:38:18.250 align:middle line:90%
to make this volume independent.

00:38:18.250 --> 00:38:22.490 align:middle line:90%


00:38:22.490 --> 00:38:24.580 align:middle line:84%
And we're going to do
that at fixed pressure.

00:38:24.580 --> 00:38:32.910 align:middle line:90%


00:38:32.910 --> 00:38:37.910 align:middle line:84%
And there are others, but
these are the easiest ones

00:38:37.910 --> 00:38:40.190 align:middle line:90%
to write down.

00:38:40.190 --> 00:38:43.152 align:middle line:84%
I'm giving you an idea of the
sorts of properties that we're

00:38:43.152 --> 00:38:44.360 align:middle line:90%
going to calculate in thermo.

00:38:44.360 --> 00:38:59.126 align:middle line:84%
So let's consider ideal gas
compression at fixed temp--

00:38:59.126 --> 00:39:05.400 align:middle line:90%


00:39:05.400 --> 00:39:09.000 align:middle line:84%
volume initial at
pressure initial

00:39:09.000 --> 00:39:14.080 align:middle line:84%
going to volume final
at pressure final.

00:39:14.080 --> 00:39:20.390 align:middle line:84%
All right, so compressibility
Bose minus 1 over V dV

00:39:20.390 --> 00:39:23.870 align:middle line:90%
dP at fixed temperature.

00:39:23.870 --> 00:39:28.000 align:middle line:84%
And for an ideal gas,
this is very, very simple.

00:39:28.000 --> 00:39:41.860 align:middle line:84%
This is minus 1 over V dVP at
fixed temperature nRT over P.

00:39:41.860 --> 00:39:48.780 align:middle line:90%
This equals nRT over VP.

00:39:48.780 --> 00:39:55.870 align:middle line:84%
1 over P equals
1 over P. This is

00:39:55.870 --> 00:40:00.700 align:middle line:84%
really simple for an ideal
gas and only for an ideal gas.

00:40:00.700 --> 00:40:02.850 align:middle line:84%
So the final volume
after compression

00:40:02.850 --> 00:40:05.055 align:middle line:84%
is going to be the initial
volume plus the change.

00:40:05.055 --> 00:40:12.470 align:middle line:90%


00:40:12.470 --> 00:40:16.770 align:middle line:84%
So it's like second fundamental
theorem of calculus.

00:40:16.770 --> 00:40:18.050 align:middle line:90%
So we're going to plug in--

00:40:18.050 --> 00:40:26.060 align:middle line:90%


00:40:26.060 --> 00:40:27.380 align:middle line:90%
what's the integrand?

00:40:27.380 --> 00:40:28.805 align:middle line:90%
It's minus V beta.

00:40:28.805 --> 00:40:33.060 align:middle line:90%


00:40:33.060 --> 00:40:34.900 align:middle line:90%
You continue to plug in.

00:40:34.900 --> 00:40:36.630 align:middle line:90%
This is volume initial minus--

00:40:36.630 --> 00:40:39.570 align:middle line:90%


00:40:39.570 --> 00:40:55.700 align:middle line:84%
so hang on-- dP nRT over P. 1
over P equals V initial minus

00:40:55.700 --> 00:41:08.540 align:middle line:84%
nRT P initial plus nRT P final,
which, of course, just equals

00:41:08.540 --> 00:41:09.330 align:middle line:90%
V final.

00:41:09.330 --> 00:41:11.900 align:middle line:84%
So this calculation is really
trivial for an ideal, guys.

00:41:11.900 --> 00:41:14.265 align:middle line:84%
You get exactly what
you think you would get.

00:41:14.265 --> 00:41:15.890 align:middle line:84%
The reason why I took
the time to do it

00:41:15.890 --> 00:41:22.350 align:middle line:84%
is to show you the manipulations
that you'll need to do later

00:41:22.350 --> 00:41:25.470 align:middle line:90%
on for non ideal gasses.

00:41:25.470 --> 00:41:26.970 align:middle line:84%
Now, thinking about
this, you've got

00:41:26.970 --> 00:41:28.830 align:middle line:84%
to put your multivariable
calculus hat on.

00:41:28.830 --> 00:41:32.570 align:middle line:90%


00:41:32.570 --> 00:41:35.910 align:middle line:84%
Of course, for an
ideal gas we get this--

00:41:35.910 --> 00:41:41.960 align:middle line:90%
1 over x, these relationships--

00:41:41.960 --> 00:41:49.920 align:middle line:84%
P initial, V initial,
P final, V final.

00:41:49.920 --> 00:41:52.305 align:middle line:90%
And this curve is an isotherm.

00:41:52.305 --> 00:41:56.182 align:middle line:90%


00:41:56.182 --> 00:41:57.640 align:middle line:84%
So we'll come back
to these when we

00:41:57.640 --> 00:42:01.210 align:middle line:84%
do heat engines and the
Carnot cycle at lecture 4.

00:42:01.210 --> 00:42:08.460 align:middle line:90%


00:42:08.460 --> 00:42:09.250 align:middle line:90%
We're almost done.

00:42:09.250 --> 00:42:11.040 align:middle line:90%
Let's see, one last--

00:42:11.040 --> 00:42:14.970 align:middle line:84%
two last points here, intensive
versus extensive properties.

00:42:14.970 --> 00:42:29.190 align:middle line:90%


00:42:29.190 --> 00:42:47.090 align:middle line:84%
All right, intensive properties
can be defined and measured

00:42:47.090 --> 00:42:53.815 align:middle line:90%
at any point within a system.

00:42:53.815 --> 00:43:03.798 align:middle line:90%


00:43:03.798 --> 00:43:05.590 align:middle line:84%
Would somebody like to
volunteer an example

00:43:05.590 --> 00:43:06.745 align:middle line:90%
of an intensive property?

00:43:06.745 --> 00:43:12.530 align:middle line:90%


00:43:12.530 --> 00:43:13.512 align:middle line:90%
AUDIENCE: Temperature.

00:43:13.512 --> 00:43:14.720 align:middle line:90%
RAFAEL JARAMILLO: Yeah, temp.

00:43:14.720 --> 00:43:19.588 align:middle line:90%


00:43:19.588 --> 00:43:21.130 align:middle line:84%
When they take your
body temperature,

00:43:21.130 --> 00:43:23.963 align:middle line:84%
they assume that you have
one body temperature.

00:43:23.963 --> 00:43:26.130 align:middle line:84%
And they can take it--
there's different places they

00:43:26.130 --> 00:43:28.995 align:middle line:84%
can stick the thermometer, but
you should get the same number.

00:43:28.995 --> 00:43:31.880 align:middle line:90%


00:43:31.880 --> 00:43:38.090 align:middle line:84%
Density-- now, you can
locally define density,

00:43:38.090 --> 00:43:40.010 align:middle line:90%
and you can measure it locally.

00:43:40.010 --> 00:43:42.710 align:middle line:84%
Composition for a uniform
system, composition.

00:43:42.710 --> 00:43:45.840 align:middle line:90%


00:43:45.840 --> 00:43:52.330 align:middle line:90%
Pressure-- and there are more.

00:43:52.330 --> 00:44:15.300 align:middle line:84%
Extensive properties depend
on the extent of the system.

00:44:15.300 --> 00:44:18.480 align:middle line:90%
And they scale with system size.

00:44:18.480 --> 00:44:26.740 align:middle line:90%


00:44:26.740 --> 00:44:41.660 align:middle line:84%
So some examples here would be
energy, volume, mass, entropy,

00:44:41.660 --> 00:44:43.460 align:middle line:90%
and so forth.

00:44:43.460 --> 00:44:45.680 align:middle line:84%
The doctor can take
your temperature

00:44:45.680 --> 00:44:48.020 align:middle line:84%
at several different
places, but the way you--

00:44:48.020 --> 00:44:49.640 align:middle line:84%
your whole body has
to be on a scale.

00:44:49.640 --> 00:44:52.790 align:middle line:84%
They can't weigh you just
by weighing your arm.

00:44:52.790 --> 00:44:55.250 align:middle line:84%
So extensive, you need
to know the extent.

00:44:55.250 --> 00:44:58.100 align:middle line:84%
Intensive, it can be
defined and measured

00:44:58.100 --> 00:45:02.257 align:middle line:84%
at any point inside
or within a system.

00:45:02.257 --> 00:45:03.340 align:middle line:90%
Easy way to remember that.

00:45:03.340 --> 00:45:06.542 align:middle line:90%


00:45:06.542 --> 00:45:08.000 align:middle line:84%
All right, we're
going to end today

00:45:08.000 --> 00:45:11.675 align:middle line:84%
with definition of the
phases-- a phase of matter.

00:45:11.675 --> 00:45:23.368 align:middle line:90%


00:45:23.368 --> 00:45:25.410 align:middle line:84%
So I'm going to define a
phase the following way.

00:45:25.410 --> 00:45:28.020 align:middle line:90%


00:45:28.020 --> 00:45:49.290 align:middle line:84%
Phase is a region within which
all intensive properties are

00:45:49.290 --> 00:45:49.790 align:middle line:90%
uniform.

00:45:49.790 --> 00:45:54.542 align:middle line:90%


00:45:54.542 --> 00:45:56.840 align:middle line:84%
All intensive
properties are uniform.

00:45:56.840 --> 00:45:59.800 align:middle line:90%
That's a phase of matter.

00:45:59.800 --> 00:46:05.930 align:middle line:84%
So, for example, solid
sucrose, some things

00:46:05.930 --> 00:46:23.400 align:middle line:84%
we've seen here-- water,
simple syrup, grass,

00:46:23.400 --> 00:46:32.420 align:middle line:90%
some examples on length scales.

00:46:32.420 --> 00:46:40.870 align:middle line:90%


00:46:40.870 --> 00:46:42.790 align:middle line:90%
It's an important caveat.

00:46:42.790 --> 00:46:45.850 align:middle line:84%
If I zoomed down to
atomic length scales,

00:46:45.850 --> 00:46:48.633 align:middle line:90%
I might say this isn't uniform.

00:46:48.633 --> 00:46:50.050 align:middle line:84%
I've got different
metal elements,

00:46:50.050 --> 00:46:52.065 align:middle line:90%
depending on where I'm looking.

00:46:52.065 --> 00:46:53.440 align:middle line:84%
So this has to be
on length scale

00:46:53.440 --> 00:46:54.982 align:middle line:84%
of large and molecular
length scales.

00:46:54.982 --> 00:47:00.280 align:middle line:90%


00:47:00.280 --> 00:47:03.950 align:middle line:84%
And phase boundaries,
which, of course,

00:47:03.950 --> 00:47:08.610 align:middle line:84%
are a really important topic
in thermo and material science,

00:47:08.610 --> 00:47:19.380 align:middle line:84%
are classified similarly
to system boundaries.

00:47:19.380 --> 00:47:25.800 align:middle line:90%


00:47:25.800 --> 00:47:28.000 align:middle line:84%
All right, so we have
a two-phase system.

00:47:28.000 --> 00:47:29.905 align:middle line:90%
For example, sugar and water--

00:47:29.905 --> 00:47:34.470 align:middle line:90%


00:47:34.470 --> 00:47:43.737 align:middle line:84%
we have some sugar,
and it's in water.

00:47:43.737 --> 00:47:44.945 align:middle line:90%
We have a sugar water system.

00:47:44.945 --> 00:47:49.290 align:middle line:90%


00:47:49.290 --> 00:47:55.780 align:middle line:84%
And we're going to think about
this boundary in the same way

00:47:55.780 --> 00:47:57.880 align:middle line:84%
that we classified
system boundaries.

00:47:57.880 --> 00:48:02.780 align:middle line:84%
And so that's an open boundary
because sugar molecules

00:48:02.780 --> 00:48:05.690 align:middle line:84%
can go across the
boundary into the water.

00:48:05.690 --> 00:48:09.330 align:middle line:84%
And similarly, sugar molecules
can come out of solution

00:48:09.330 --> 00:48:12.620 align:middle line:90%
and go back into the solid.

00:48:12.620 --> 00:48:14.810 align:middle line:84%
This is a boundary
that exchanges volume.

00:48:14.810 --> 00:48:18.380 align:middle line:84%
It exchanges heat energy,
and it exchanges mass.

00:48:18.380 --> 00:48:22.500 align:middle line:90%


00:48:22.500 --> 00:48:25.320 align:middle line:84%
Good, so that's all I
had prepared for today.

00:48:25.320 --> 00:48:29.448 align:middle line:90%
It is 10:54, almost perfect.

00:48:29.448 --> 00:48:30.240 align:middle line:90%
Thanks for joining.

00:48:30.240 --> 00:48:33.120 align:middle line:84%
As usual, hang out
until at least 11:00

00:48:33.120 --> 00:48:35.930 align:middle line:84%
if folks want to talk
or ask any questions.

00:48:35.930 --> 00:48:38.190 align:middle line:90%
Otherwise, I'll see you Monday.

00:48:38.190 --> 00:48:41.000 align:middle line:90%