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Welcome back.
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We're finally using the Laplace
Transform to do
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something useful.
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In the first part of this
problem, we just had this
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fairly straightforward
differential equation.
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And I know it's a little bit
frustrating right now, because
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you're like, this is such an
easy one to solve using the
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characteristic equation.
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Why are we doing Laplace
Transforms?
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Well I just want to show you
that they can solve even these
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problems. But later on there
are going to be classes of
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problems that, frankly, our
traditional methods aren't as
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good as the Laplace Transform.
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But anyway, how did
we solve this?
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We just took the Laplace
Transform of both sides of
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this equation.
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We got all of this hairy mess.
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We used the property of the
derivative of functions, where
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you take the Laplace Transform,
and we ended up,
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after doing a lot of algebra
essentially, we got this.
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We got the Laplace Transform of
y is equal to this thing.
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We just took the Laplace
Transform of both sides and
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manipulated algebraically.
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So now our task in this video
is to figure out what y's
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Laplace Transform
is this thing?
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And essentially what we're
trying to do, is we're trying
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to take the inverse Laplace
Transform of both sides of
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this equation.
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So another way to say it, we
could say that y-- if we take
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the inverse Laplace Transform
of both sides-- we could say
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that y is equal to the
inverse Laplace
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Transform of this thing.
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2s plus 13, over s squared
plus 5s plus 6.
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Now we'll eventually actually
learn the formal definition of
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the inverse Laplace Transform.
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How do you go from the s
domain to the t domain?
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Or how do you go from
the frequency
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domain to the time domain?
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We're not going to worry
about that right now.
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What we're going to do is we're
going to get this into a
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form that we recognize,
and say, oh,
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I know those functions.
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That's the Laplace Transform
of whatever and whatever.
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And then we'll know what y is.
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So let's try to do that.
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So what we're going to use is
something that you probably
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haven't used since Algebra two,
which is I think when
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it's taught in, you know,
eighth, ninth,
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or 10th grade, depending.
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And you finally see it now in
differential equations that it
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actually has some use.
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Let me write it.
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We're going to use partial
fraction expansion.
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And I'll do a little primer
on that, in case you don't
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remember it.
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So anyway, let's just factor
the bottom part right here.
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And you'll see where I'm
going with this.
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So if I factor the bottom, I get
s plus 2 times s plus 3.
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And what we want to do, is we
want to rewrite this fraction
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as the sum of 2-- I
guess you could
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call it partial fractions.
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I think that's why it's called
partial fraction expansion.
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So we want to write this as a
sum of A over s plus 2, plus B
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over s plus 3.
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And if we can do this, then--
and bells might already be
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ringing in your head-- we know
that these things that look
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like this are the Laplace
Transform of functions that
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we've already solved for.
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And I'll do a little review
on that in a second.
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But anyway, how do we
figure out A and B?
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Well if we were to actually add
A and B, if we were to--
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let's do a little aside right
here-- so if we said that A--
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so if we were to give them a
common denominator, which is
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this, s plus 2 times s plus 3.
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Then what would A become?
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We'd have to multiply A
times s plus 3, right?
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So we'd get As plus 3A.
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This, as I've written it right
now, is the same thing as A
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over s plus 2.
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You could cancel out an s plus
3 in the top and the bottom.
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And now we're going to
add the B to it.
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So plus-- I'll do that in a
different color-- plus-- well,
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if we have this as the
denominator, we could multiply
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the numerator and
the denominator
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by s plus 2, right?
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To get B times s, plus
2B, and that's going
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to equal this thing.
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And all I did is I added
these two fractions.
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Nothing fancier than there.
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That was Algebra two.
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Actually, I think I should
do an actual
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video on that as well.
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But that's going to
equal this thing.
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2s plus 13, all of that over
s plus 2 times s plus 3.
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Notice in all differential
equations, the hairiest part's
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always the algebra.
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So now what we do
is we match up.
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We say, well, let's add
the s terms here.
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And we could say that the
numerators have to equal each
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other, because the denominators
are equal.
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So we have A plus Bs plus 3A
plus 2B is equal to 2s plus B.
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So the coefficient on s, on
the right-hand side, is 2.
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The coefficient on the left-hand
side is A plus B, so
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we know that A plus
B is equal to 2.
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And then on the right-hand side,
we see 3A plus 2B must
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be equal to-- oh,
this is a 13.
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Did I say B?
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This is a 13.
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That's a 13.
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It looks just like a B, right?
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That was 2s plus 13.
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Anyway, so on the right-hand
side I get, it was 3A plus 2B
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is equal to 13.
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Now we have two equations
with two unknowns,
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and what do we get?
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I know this is very tiresome,
but it'll be
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satisfying in the end.
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Because you'll actually
solve something
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with the Laplace Transform.
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So let's multiply the top
equation by 2, or let's just
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say minus 2.
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So we get minus 2A minus
2B equals minus 4.
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And then we get-- add the two
equations-- you get A is equal
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to-- these cancel out--
A is equal to 9.
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Great.
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If A is equal to 9, what
is B equal to?
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B is equal to 9 plus
what is equal to 2?
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Or 2 minus 9 is minus 7.
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And we have done some serious
simplification.
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Because now we can rewrite this
whole expression as the
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Laplace Transform of y is equal
to A over s plus 2, is
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equal to 9 over s plus 2,
minus 7 over s plus 3.
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Or another way of writing it, we
could write it as equal to
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9 times 1 over s plus 2, minus
7 times 1 over s plus 3.
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Why did I take the trouble
to do this?
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Well hopefully, you'll recognize
this was actually
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the second Laplace Transform
we figured out.
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What was that?
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I'll write it down here just
so you remember it.
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It was the Laplace Transform of
e to the at, was equal to 1
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over s minus a.
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That was the second Laplace
Transform we figured out.
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So this is interesting.
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This is the Laplace
Transform of what?
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So if we were to take the
inverse Laplace Transform--
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actually let me just
stay consistent.
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So that means that this is the
Laplace Transform of y, is
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equal to 9 times the Laplace
Transform of what?
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If we just do pattern matching,
if this is s minus
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a, then a is minus 2.
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So 9 times the Laplace
Transform of e
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to the minus 2t.
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Does that make sense?
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Take this, put it in this one,
which we figured out, and you
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get 1 over s plus 2.
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And let me clean this up a
little bit, because I'm going
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to need that real estate.
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I'll write this.
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I'll leave that there, because
we'll still use that.
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And then we have minus 7 times--
this is the Laplace
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Transform of what?
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This is the Laplace Transform
of e to the minus 3t.
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This pattern matching, you're
like, wow, if you saw this,
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you would go to your Laplace
Transform table, if you didn't
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remember it, you'd see this.
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You're like, wow, that looks
a lot like that.
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I just have to figure
out what a is.
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I have s plus 3.
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I have s minus a.
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So in this case, a is
equal to minus 3.
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So if a is equal to minus 3,
this is the Laplace Transform
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of e to the minus 3t.
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So now we can take the inverse
Laplace-- actually,
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before we do that.
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We know that because the Laplace
Transform is a linear
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operator-- and actually now I
can delete this down here-- we
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know that the Laplace Transform
is a linear
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operator, so we can
write this.
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And you normally wouldn't go
through all of these steps.
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I just really want to make you
understand what we're doing.
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So we could say that this is the
same thing as the Laplace
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Transform of 9e to the minus 2t,
minus 7e to the minus 3t.
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Now we have something
interesting.
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The Laplace Transform of y
is equal to the Laplace
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Transform of this.
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Well if that's the case, then
y must be equal to 9e to the
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minus 2t, minus 7e
to the minus 3t.
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And I never proved to you, but
the Laplace Transform is
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actually a 1:1 Transformation.
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That if a function's Laplace
Transform, if I take a
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function against the Laplace
Transform, and then if I were
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take the inverse Laplace
Transform, the only function
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whose Laplace Transform
that that is, is
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that original function.
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It's not like two different
functions can have the same
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Laplace Transform.
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Anyway, a couple of things
to think about here.
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Notice, we had that thing that
kind of looked like a
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characteristic equation
pop up here and there.
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And we still have to solve a
system of two equations with
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two unknowns.
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Those are both things that we
had to do when we solve an
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initial value problem, when we
use just traditional, the
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characteristic equation.
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But here it happened
all at once.
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And frankly it was a little bit
hairier because we had to
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do all this partial fraction
expansion.
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But it's pretty neat.
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The Laplace Transform got
us something useful.
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In the next video I'll actually
do a non-homogeneous
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equation, and show you that the
Laplace Transform applies
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equally well there.
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So it's kind of a more
consistent theory of solving
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differential equations, instead
of kind of guessing
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solutions, and solving for
coefficients and all of that.
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See you in the next video.