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ocw.mit.edu so again welcome to

00:24 - 00:32

1801 we're getting started today with

00:28 - 00:35

what we're calling unit one highly

00:32 - 00:38

imaginative topic uh highly imaginative

00:35 - 00:38

title and it's

00:42 - 00:47

differentiation so let me first tell you

00:45 - 00:48

briefly what's in store in the next

00:47 - 00:56

couple of

00:48 - 00:56

weeks the main topic today is what is a

00:58 - 01:01

derivative

01:03 - 01:06

and we're going

01:07 - 01:13

to look at this from several different

01:10 - 01:16

points of view and the first one is a

01:13 - 01:16

the geometric

01:18 - 01:23

interpretation and that's what we'll

01:19 - 01:26

spend most of today on

01:23 - 01:28

and then we'll also talk about a

01:26 - 01:31

physical

01:28 - 01:31

interpretation

01:32 - 01:35

of what a derivative

01:36 - 01:41

is

01:38 - 01:41

and

01:41 - 01:47

then there's going to be something else

01:44 - 01:49

which I guess is maybe the reason why

01:47 - 01:52

calculus is so fundamental and why we

01:49 - 01:55

always start with it uh at in most

01:52 - 01:58

science and engineering schools which is

01:55 - 02:00

the

01:58 - 02:03

importance of derivatives

02:00 - 02:06

of of this to

02:03 - 02:06

all

02:08 - 02:14

measurements so that means pretty much

02:11 - 02:17

every place that means in science and

02:14 - 02:21

engineering in

02:17 - 02:21

economics in uh political

02:22 - 02:29

science Etc uh polling uh lots of

02:26 - 02:32

commercial applications just just about

02:29 - 02:34

everything now so that's what we'll be

02:32 - 02:37

getting started with and then there's

02:34 - 02:38

another thing that we're going to do in

02:37 - 02:43

this

02:38 - 02:46

unit which is we're going to explain how

02:43 - 02:46

to differentiate

02:49 - 02:54

anything so how to differentiate any

02:52 - 02:54

function you

02:58 - 03:01

know

03:02 - 03:06

and that's kind of a tall order but let

03:04 - 03:09

me just give you an example if you want

03:06 - 03:10

to take the derivative this we'll see

03:09 - 03:13

today as the notation for the derivative

03:10 - 03:16

of something of some messy function like

03:13 - 03:19

e to the X AR

03:16 - 03:25

tan of

03:19 - 03:27

X we'll work this out by the end of this

03:25 - 03:31

unit all right so anything you can think

03:27 - 03:33

of anything you can write down we can

03:31 - 03:38

differentiated all right so that's what

03:33 - 03:40

we're going to do and today as I said

03:38 - 03:43

we're going to spend most of our time on

03:40 - 03:43

this geometric

03:44 - 03:48

interpretation so let's let's begin with

03:49 - 03:55

that so here we go with the

03:52 - 03:55

geometric

03:57 - 04:04

interpretation of uh

04:01 - 04:04

derivatives

04:05 - 04:12

and what we're going to

04:08 - 04:16

do is just ask the geometric problem of

04:12 - 04:16

finding the tangent

04:21 - 04:28

line to

04:24 - 04:31

some graph of some function at some

04:28 - 04:35

point

04:31 - 04:39

which is say x0 y0 so that's the problem

04:35 - 04:41

that we're addressing here um guess I

04:39 - 04:46

should probably turn this

04:41 - 04:48

off all right so here's our problem and

04:46 - 04:51

now let me show you the

04:48 - 04:55

solution

04:51 - 04:55

so well let's graph the

04:57 - 05:04

function so let's say here's its graph

05:00 - 05:06

and here's some point all right maybe I

05:04 - 05:08

should draw it just a bit lower so that

05:06 - 05:11

I

05:08 - 05:12

don't all right so here's a point P

05:11 - 05:15

maybe

05:12 - 05:18

it's above the point

05:15 - 05:22

x0 x0 by the way this was supposed to be

05:18 - 05:24

an x0 that was the some fixed place on

05:22 - 05:24

the x

05:26 - 05:34

axis and now in order to perform this

05:30 - 05:37

this Mighty feat I will

05:34 - 05:42

um use another color of chalk how about

05:37 - 05:45

red okay so so here it is there's the

05:42 - 05:49

tangent line well not quite straight

05:45 - 05:50

close enough right I did it all right

05:49 - 05:54

that's the end that's the geometric

05:50 - 05:57

problem I achieved what I wanted to do

05:54 - 06:00

and uh it's kind of an interesting

05:57 - 06:02

question which unfortunately I can't

06:00 - 06:04

solve for you in this class which is how

06:02 - 06:07

did I do that that is how physically did

06:04 - 06:09

I manage to know what to do to draw this

06:07 - 06:12

tangent line but that's what geometric

06:09 - 06:14

problems are like um we visualize it we

06:12 - 06:17

can figure it out somewhere in our

06:14 - 06:20

brains it happens and the task that we

06:17 - 06:26

have now is to figure out how to do it

06:20 - 06:29

analytically to do it in a way that uh a

06:26 - 06:31

machine could do just as well as I did

06:29 - 06:34

in drawing this tangent

06:31 - 06:34

line

06:34 - 06:41

so so what do we learn in high school

06:38 - 06:44

about what a tangent line is well a

06:41 - 06:46

tangent line has an equation and any

06:44 - 06:51

line through Point has the equation y -

06:46 - 06:55

y0 is equal to M the slope time x - x0

06:51 - 06:58

so so here's the

06:55 - 07:01

the equation for that

06:58 - 07:04

line and now there are two pieces of

07:01 - 07:05

information that we're going to need to

07:04 - 07:08

work

07:05 - 07:10

out uh what the line is the first one is

07:08 - 07:13

the

07:10 - 07:18

point that's that point P there and to

07:13 - 07:20

specify P given given X we need to know

07:18 - 07:23

the uh the the level of Y which is of

07:20 - 07:25

course just f ofx z now that's that's

07:23 - 07:28

not a calculus problem but anyway that's

07:25 - 07:31

a very important part of the process so

07:28 - 07:34

that's the first thing we need to

07:31 - 07:38

know and the second thing we need to

07:34 - 07:38

know is the

07:38 - 07:45

slope and that's this number

07:41 - 07:50

M and in calculus we have another name

07:45 - 07:53

for it we call it frime of x0 namely the

07:50 - 07:54

derivative of f so that's the calculus

07:53 - 07:57

part that's the tricky part and that's

07:54 - 08:00

the part that we have to discuss

07:57 - 08:02

now so just to make that

08:00 - 08:06

uh explicit here I'm going to make a

08:02 - 08:10

definition which is that frime of

08:06 - 08:10

x0 which is known as the

08:12 - 08:17

derivative of

08:14 - 08:23

F at

08:17 - 08:25

x0 all right is the

08:23 - 08:28

slope

08:25 - 08:31

of the tangent

08:28 - 08:31

line

08:33 - 08:40

to Y =

08:35 - 08:44

FX at the point

08:40 - 08:44

uh uh let's just call it

08:47 - 08:52

P all

08:49 - 08:55

right

08:52 - 08:58

so so that's what it is but still I

08:55 - 09:01

haven't made any progress in figuring

08:58 - 09:04

out any better how I drew that line so I

09:01 - 09:06

have to say something that's more

09:04 - 09:08

concrete because I want to be able to

09:06 - 09:12

cook up what these numbers are I have to

09:08 - 09:14

figure out what this number m is uh and

09:12 - 09:18

one way of thinking about that let me

09:14 - 09:19

just uh try it is so I certainly am

09:18 - 09:21

taking for granted the sort of

09:19 - 09:23

non-calculus part that I know what a

09:21 - 09:26

line through a point is so I know this

09:23 - 09:28

equation but another possibility might

09:26 - 09:30

be you know this line here how do I know

09:28 - 09:33

well fortunately I didn't draw it quite

09:30 - 09:37

straight but there it is how do I know

09:33 - 09:43

that this orange line is not a tangent

09:37 - 09:43

line but this other line is a tangent

09:44 - 09:47

line

09:48 - 09:54

well it's it's actually not so obvious

09:52 - 09:57

and but I'm going

09:54 - 09:59

to describe it a little bit it's it's

09:57 - 10:02

not really the fact this thing crosses

09:59 - 10:05

at some other place which is this point

10:02 - 10:07

q but it's not really the fact that the

10:05 - 10:09

thing crosses at two place because the

10:07 - 10:11

line could be Wiggly the curve could be

10:09 - 10:13

Wiggly and it could cross back and forth

10:11 - 10:16

a number of times that's not what

10:13 - 10:19

distinguishes the tangent

10:16 - 10:22

line so I'm going to have to somehow

10:19 - 10:26

grasp this and I first do it in

10:22 - 10:31

language and it it's the following idea

10:26 - 10:35

it's that if you take this orange line

10:31 - 10:38

which is uh called a secant line and you

10:35 - 10:42

think of the Q the point Q is getting

10:38 - 10:44

closer and closer to P then the slope of

10:42 - 10:47

that line will get closer and closer to

10:44 - 10:53

the slope of the red

10:47 - 10:54

line and if we draw it close enough then

10:53 - 10:56

that's going to be the correct line so

10:54 - 10:59

that's really what I did sort of in my

10:56 - 11:00

brain when I drew that first line and so

10:59 - 11:04

that's the way I'm going to articulate

11:00 - 11:04

it first now so the tangent

11:07 - 11:16

line is equal to the

11:11 - 11:16

limit of what so-called secant

11:18 - 11:25

lines

11:20 - 11:27

PQ as Q TS to p and here we're thinking

11:25 - 11:30

of p is being

11:27 - 11:34

fixed and Q is

11:30 - 11:36

varying all right so so that's

11:34 - 11:40

the the G again this is still a

11:36 - 11:41

geometric discussion but now uh we're

11:40 - 11:44

going to be able to put symbols and

11:41 - 11:48

formulas to this computation and we'll

11:44 - 11:50

be able to um to work out uh formulas in

11:48 - 11:50

any

11:53 - 11:57

example

11:55 - 12:00

so so let's do

11:57 - 12:04

that so so first of

12:00 - 12:07

all I'm going to write out these points

12:04 - 12:10

p and Q again so maybe we'll put P

12:07 - 12:12

here and Q

12:10 - 12:14

here and I'm thinking of this line

12:12 - 12:17

through them I guess it was orange so

12:14 - 12:19

we'll leave it as

12:17 - 12:23

orange all

12:19 - 12:26

right and now I want to compute its

12:23 - 12:28

slope and so this is gradually we'll do

12:26 - 12:30

this in two steps and these steps will

12:28 - 12:32

introduce to the basic notations which

12:30 - 12:35

are used throughout calculus including

12:32 - 12:39

multivariable calculus across the board

12:35 - 12:42

so the first notation that's used is you

12:39 - 12:45

imagine here's the x-axis underneath and

12:42 - 12:49

here's the x0 the location directly

12:45 - 12:52

below the point p and we're traveling

12:49 - 12:55

here a horizontal distance which is

12:52 - 12:58

denoted by Delta X so

12:55 - 13:01

that's Delta X

12:58 - 13:04

socaled and we could also call it the

13:01 - 13:04

change in

13:06 - 13:11

X all right so that's one thing we want

13:09 - 13:13

to measure in order to get the slope of

13:11 - 13:16

this line PQ and the other thing is this

13:13 - 13:18

height so that's this distance here

13:16 - 13:21

which we denote Delta F which is the

13:18 - 13:21

change in

13:21 - 13:28

F and then the

13:24 - 13:29

slope is just the ratio Delta F over

13:28 - 13:33

Delta X

13:29 - 13:36

so this is the slope of

13:33 - 13:36

the of the

13:39 - 13:43

secant and the process I just described

13:41 - 13:46

over here with this

13:43 - 13:48

limit applies not just to the whole line

13:46 - 13:50

itself but also in particular to its

13:48 - 13:54

slope and the way we write that is the

13:50 - 13:57

limit as Delta X goes to zero and that's

13:54 - 14:01

going to be our slope so this is the

13:57 - 14:01

slope of the tangent line

14:11 - 14:14

okay

14:15 - 14:22

now this is still a little a little

14:19 - 14:26

general and I'm going to I want to work

14:22 - 14:29

out a more usable form here I want to

14:26 - 14:32

work out a better formula for this and

14:29 - 14:36

in order to do that I'm going to write

14:32 - 14:40

Delta F the numerator more explicitly

14:36 - 14:45

here the change in F so remember that

14:40 - 14:45

the point p is the point x0 F of

14:46 - 14:50

x0 all right that's what we got from our

14:48 - 14:55

formula for the

14:50 - 14:56

point and in order to compute these

14:55 - 14:58

distances and in particular the vertical

14:56 - 15:02

distance here I'm going to have to get a

14:58 - 15:06

formula for Q as well so if this

15:02 - 15:10

horizontal distance is Delta X then this

15:06 - 15:14

location is x0 plus Delta

15:10 - 15:15

X and so the point above that point has

15:14 - 15:17

a

15:15 - 15:20

formula which

15:17 - 15:27

is x0 plus uh sorry plus Delta

15:20 - 15:30

x f of and this is a mouthful x0 + Delta

15:27 - 15:30

X

15:32 - 15:35

all right so there's the formula for the

15:33 - 15:38

point Q here's the formula for the point

15:35 - 15:41

p and now I can write a

15:38 - 15:41

different

15:43 - 15:46

formula for the

15:46 - 15:55

derivative which is the following so

15:49 - 15:59

this frime of x0 which is the same as

15:55 - 16:03

m is going to be the limit as Delta X

15:59 - 16:07

goes to zero of the change in F Well the

16:03 - 16:12

change in F is the value of F at the

16:07 - 16:15

upper Point here which is x0 + Delta

16:12 - 16:18

X and minus its value at the lower Point

16:15 - 16:18

P which is f of

16:19 - 16:25

x0 divided by Delta

16:22 - 16:27

X all right so this is the formula I'm

16:25 - 16:30

going to put this in a little box

16:27 - 16:32

because this is by far

16:30 - 16:34

the most important formula today which

16:32 - 16:37

we use to derive pretty much everything

16:34 - 16:41

else and this is the way that we're

16:37 - 16:41

going to be able to compute these

16:45 - 16:50

numbers so let's let's do an

16:57 - 17:00

example

17:06 - 17:11

this example so we'll call this example

17:12 - 17:19

one uh we'll take the function f ofx

17:16 - 17:22

which is

17:19 - 17:25

1/x that's sufficiently complicated to

17:22 - 17:27

have an interesting answer and uh

17:25 - 17:30

sufficiently straightforward that we can

17:27 - 17:33

compute the derivative fairly

17:30 - 17:35

quickly so so what is it that we're

17:33 - 17:39

going to do

17:35 - 17:40

here all we're going to do is we're

17:39 - 17:44

going

17:40 - 17:45

to plug in this this formula here for

17:44 - 17:48

for that function that's that's all

17:45 - 17:51

we're going to do and Visually what

17:48 - 17:54

we're accomplishing is somehow to take

17:51 - 17:57

the hyperbola and take a point on the

17:54 - 18:00

hyperbola and figure

17:57 - 18:01

out some

18:00 - 18:03

tangent line all right that's what we're

18:01 - 18:05

accomplishing when we do that so we're

18:03 - 18:09

accomplishing this geometrically but

18:05 - 18:13

we'll be doing it algebraically so first

18:09 - 18:17

we consider this difference Delta F over

18:13 - 18:19

Delta X and write out its formula so I

18:17 - 18:22

have to have a place so I'm going to

18:19 - 18:23

make it again above this point x0 which

18:22 - 18:25

is a general point we'll make the

18:23 - 18:29

general

18:25 - 18:31

calculation so the value of F at the top

18:29 - 18:35

when we move to the right by F ofx so I

18:31 - 18:39

just read off from this read off from

18:35 - 18:45

here the uh the formula the first thing

18:39 - 18:48

I get here is 1 over x0 + Delta X that's

18:45 - 18:50

the leftand term minus

18:48 - 18:53

1x0 that's the right hand term and then

18:50 - 18:56

I have to divide that by Delta

18:53 - 18:59

X okay so here's

18:56 - 19:03

our expression and by by the way this

18:59 - 19:06

has a name this thing is called a

19:03 - 19:06

difference

19:09 - 19:13

quotient it's pretty complicated because

19:12 - 19:15

there's always a difference in the

19:13 - 19:16

numerator and in Disguise the

19:15 - 19:19

denominator is a difference because it's

19:16 - 19:21

the difference between the value on the

19:19 - 19:24

right side and the value on the left

19:21 - 19:24

side

19:25 - 19:34

here okay so now

19:30 - 19:36

we're going to simplify it by some

19:34 - 19:39

algebra so let's just take a look so

19:36 - 19:43

this is equal to let's continue on the

19:39 - 19:47

next level here this is equal to 1 /

19:43 - 19:48

Delta x * now all I'm going to do is put

19:47 - 19:52

it over a common

19:48 - 19:57

denominator so the common denominator is

19:52 - 19:59

x0 + Delta x * x0 and so in the

19:57 - 20:02

numerator for the first expression I

19:59 - 20:04

have x0 and for the second expression I

20:02 - 20:07

have x0 + Delta

20:04 - 20:09

X so this is a the same thing as I had

20:07 - 20:12

in the numerator before factoring out

20:09 - 20:17

this denominator and here I put that

20:12 - 20:20

numerator into this more amable form and

20:17 - 20:23

now there are two basic cancellations

20:20 - 20:27

the first one is that x0 and x0

20:23 - 20:27

cancel so we have

20:27 - 20:30

this

20:33 - 20:39

and then the second step is that these

20:37 - 20:42

two expressions cancel right the

20:39 - 20:44

numerator and denominator now we have um

20:42 - 20:48

a cancellation that we can make use of

20:44 - 20:53

so we'll write that under

20:48 - 20:55

here and this is uh equals Min -1 over

20:53 - 21:00

x0 + Delta

20:55 - 21:02

x * x0 and then the very last step is to

21:00 - 21:07

take the

21:02 - 21:10

limit as Delta X tends to zero

21:07 - 21:13

and now we can do it before we couldn't

21:10 - 21:16

do it why because the numerator and the

21:13 - 21:18

denominator gave us 0 over Z but now

21:16 - 21:20

that I've made this cancellation I can

21:18 - 21:22

pass to the Limit and all that happens

21:20 - 21:26

is I set this Delta x equal to Z and I

21:22 - 21:27

get minus1 /x 0^ 2ar all right so that's

21:26 - 21:30

the

21:27 - 21:30

answer

21:32 - 21:38

right so in other words what I've shown

21:34 - 21:42

let me put it up here is that fime of x0

21:38 - 21:42

is -1 / x0

21:52 - 21:57

2 now uh let's let's look at the graph

21:55 - 22:00

just a little bit to check this for

21:57 - 22:03

plausibility all

22:00 - 22:06

right uh what's Happening Here is first

22:03 - 22:09

of all it's negative right it's less

22:06 - 22:12

than zero which is a good thing you see

22:09 - 22:12

that slope there is

22:16 - 22:23

negative that's the simplest check that

22:19 - 22:26

you could make and the second thing that

22:23 - 22:29

I would just like to point out is that

22:26 - 22:31

as X goes to Infinity that that is if as

22:29 - 22:35

we go farther to the right it gets less

22:31 - 22:38

and less steep so uh

22:35 - 22:41

less and whoops as X go x0 goes to

22:38 - 22:45

Infinity not not zero as x0 goes to

22:41 - 22:48

Infinity less and less

22:45 - 22:50

steep so that's also consistent here is

22:48 - 22:53

when x0 is very large this is a smaller

22:50 - 22:54

and smaller number in in magnitude

22:53 - 22:57

although it's always negative it's

22:54 - 22:57

always sloping

22:57 - 23:00

down

23:01 - 23:05

all right uh so I've managed to fill the

23:03 - 23:08

boards so maybe I should stop for a

23:05 - 23:08

question or two

23:14 - 23:23

yes so the question is to explain again

23:19 - 23:27

this uh limiting process so the formula

23:23 - 23:28

here is We have basically two numbers so

23:27 - 23:32

in other words why is it that this

23:28 - 23:36

expression when Delta x ts to 0 is equal

23:32 - 23:38

to - 1x0 2 let me let me illustrate it

23:36 - 23:41

by sticking in a number for x0 to make

23:38 - 23:45

it more explicit all right so for

23:41 - 23:51

instance let me stick in here for x0 the

23:45 - 23:54

number 3 then it's -1 over 3 + Delta x *

23:51 - 23:56

3 that's the situation that we've got

23:54 - 23:58

and now the question is what happens as

23:56 - 23:59

this number gets smaller and smaller and

23:58 - 24:02

smaller

23:59 - 24:04

and gets to be practically zero well

24:02 - 24:06

literally what we can do is just plug in

24:04 - 24:09

zero there then you get 3 + 0 * 3 in the

24:06 - 24:11

denominator minus one in the numerator

24:09 - 24:15

so this tends

24:11 - 24:17

to tends to -1 over 9 over 3^

24:15 - 24:20

SAR and that's what I'm saying in

24:17 - 24:24

general with this with this

24:20 - 24:24

extra number here other other

24:25 - 24:32

questions yes how did you simplify

24:29 - 24:35

Del Delta X how you simplify from the

24:32 - 24:35

origal equation

24:36 - 24:44

to so the question is how what happened

24:40 - 24:46

between this step and this step right

24:44 - 24:49

explain this this step here all right so

24:46 - 24:52

there were two parts to that the first

24:49 - 24:55

is this Delta X which was sitting in the

24:52 - 24:58

denominator I factored all the way out

24:55 - 25:00

front and so what's in the parentheses

24:58 - 25:03

is supposed to be the same as what's in

25:00 - 25:06

the numerator of this other expression

25:03 - 25:08

and then at the same time as doing that

25:06 - 25:10

I put that expression which is a

25:08 - 25:12

difference of two fractions I expressed

25:10 - 25:14

it with a common denominator so in the

25:12 - 25:17

denominator here you see the product of

25:14 - 25:18

the denominators of the two fractions

25:17 - 25:21

and then I just figured out what the

25:18 - 25:25

numerator had to be without

25:21 - 25:25

really yeah other

25:27 - 25:37

questions okay okay so

25:31 - 25:41

now uh so I I claim that on the

25:37 - 25:45

whole calculus is uh gets a bad wrap

25:41 - 25:48

that it's um actually easier than than

25:45 - 25:51

most things um but it has there's a

25:48 - 25:55

perception that it's that it's that it's

25:51 - 25:58

harder and so I really have a duty to to

25:55 - 26:01

give you the calculus made harder a

25:58 - 26:03

story here so we we we we have to make

26:01 - 26:05

things harder because that's that's our

26:03 - 26:07

job and this is actually what most

26:05 - 26:09

people do in calculus and it's the

26:07 - 26:14

reason why calculus has a bad reputation

26:09 - 26:17

so the the the secret is that when

26:14 - 26:20

people ask problems in calculus they

26:17 - 26:23

generally ask them in context and there

26:20 - 26:25

are many many other things going on and

26:23 - 26:27

so the little piece of the problem which

26:25 - 26:29

is calculus is actually fairly routine

26:27 - 26:31

and has to be isolated and gotten

26:29 - 26:32

through but all the rest of it relies on

26:31 - 26:35

everything else you learned in

26:32 - 26:38

mathematics up to this stage from grade

26:35 - 26:40

school to through high school so so

26:38 - 26:42

that's the complication so now we're

26:40 - 26:44

going to do a little bit of calculus

26:42 - 26:44

made

26:48 - 26:55

hard by uh uh talking about a word

26:52 - 26:59

problem now we we only have one sort of

26:55 - 27:02

word problem that we can pose because

26:59 - 27:04

all we've talked about is this geometry

27:02 - 27:05

uh uh point of view so so far those are

27:04 - 27:07

the only kinds of word problems we can

27:05 - 27:12

pose so what we're going to do is just

27:07 - 27:16

pose such a problem so find the

27:12 - 27:16

areas of

27:19 - 27:22

triangles

27:23 - 27:30

enclosed by the

27:27 - 27:33

axes

27:30 - 27:33

and the

27:34 - 27:43

tangent to um y =

27:39 - 27:47

1X okay so that's a geometry

27:43 - 27:49

problem and let me draw a picture of it

27:47 - 27:52

it's practically the the same as the

27:49 - 27:54

picture for example one of course so

27:52 - 27:56

here's we only consider the first

27:54 - 28:00

quadrant here's our

27:56 - 28:03

shape all right it's the hyperbola and

28:00 - 28:07

here's maybe one of our tangent lines

28:03 - 28:11

which is coming in like this and

28:07 - 28:14

then we're trying to find this area

28:11 - 28:16

here all right so there's our problem so

28:14 - 28:17

why does it have to do with Calculus it

28:16 - 28:20

has to do with Calculus because there's

28:17 - 28:23

a tangent line in it and so we're going

28:20 - 28:26

to need to do some calculus to to answer

28:23 - 28:30

this question but as you'll see the

28:26 - 28:30

calculus is the easy part

30:28 - 30:31

is and once I figured out what the

30:30 - 30:34

tangent line is the rest of the problem

30:31 - 30:37

is no longer calculus it's just that

30:34 - 30:40

slope that we need so what's the formula

30:37 - 30:46

for the tangent line put that over

30:40 - 30:47

here it's going to be Yus y0 is equal to

30:46 - 30:51

and here's the magic number we already

30:47 - 30:55

calculated it it's in the box over there

30:51 - 30:58

it's -1 /x 0^

30:55 - 31:01

2ar x - x0

30:58 - 31:03

so this is the only bit of calculus in

31:01 - 31:03

this

31:12 - 31:18

problem but now we're not done we have

31:16 - 31:19

to finish it we have to figure out all

31:18 - 31:22

the rest of these quantities so we can

31:19 - 31:22

figure out the

31:26 - 31:30

area all right

31:31 - 31:34

so how do we do

31:40 - 31:46

that well to find this point this has a

31:44 - 31:50

name we're going to

31:46 - 31:50

find the um so-called x

31:52 - 31:57

intercept that's the first thing we're

31:54 - 32:00

going to do so to do that what we need

31:57 - 32:03

to do is to find where this horizontal

32:00 - 32:08

line meets that diagonal line and the

32:03 - 32:10

equation for the x intercept is y =

32:08 - 32:12

0 all

32:10 - 32:14

right so we plug in y equals 0 that's

32:12 - 32:17

this horizontal line and we find this

32:14 - 32:22

point so let's do that into

32:17 - 32:24

star so we get 0 minus oh one other

32:22 - 32:29

thing we need to know we know that

32:24 - 32:33

y0 is f of x0 and F ofx is 1 /x so this

32:29 - 32:37

thing is 1 /

32:33 - 32:41

x0 right and that's equal to -1 /x 0^

32:37 - 32:46

2ar and here's X and here's

32:41 - 32:50

x0 all right so in order to find this x

32:46 - 32:52

value I have to uh plug in one equation

32:50 - 32:52

into the

32:53 - 33:01

other so this simplifies a

32:56 - 33:07

bit uh let's put let's see this is uh -

33:01 - 33:10

xx0 2 and this is plus 1 over x0 because

33:07 - 33:14

the x0 and x0 squar cancel somewhat and

33:10 - 33:20

so if I put this on the other side I get

33:14 - 33:23

x / x 0^ 2 is equal to 2

33:20 - 33:25

x0 and if I then multiply through so

33:23 - 33:26

that's what this implies and If I

33:25 - 33:32

multiply

33:26 - 33:32

through by uh x0 2 I get X is equal to 2

33:33 - 33:36

x0

33:39 - 33:44

okay okay so I claim that this point

33:41 - 33:44

we've just calculated it's

33:51 - 33:54

2x0

33:54 - 34:02

now I'm almost done I need to get the

34:00 - 34:05

other one I need to get this one up

34:02 - 34:10

here now I'm going to use a very big

34:05 - 34:10

shortcut to do that so so the

34:11 - 34:17

shortcut to the Y intercept sorry yeah

34:14 - 34:17

the Y

34:18 - 34:23

intercept um is to use

34:26 - 34:31

symmetry right I claim I can stare at

34:29 - 34:34

this and I can look at that and I know

34:31 - 34:36

the formula for the Y intercept it's

34:34 - 34:36

equal

34:36 - 34:42

to 2

34:39 - 34:46

y0 all right that's what that one is so

34:42 - 34:48

this one is 2 y0 and the reason I know

34:46 - 34:51

this is the following so here's the

34:48 - 34:54

symmetry of the situation which is not

34:51 - 34:57

completely direct it's a kind of mirror

34:54 - 34:59

symmetry around the diagonal it involves

34:57 - 35:02

the ex

34:59 - 35:02

change of

35:02 - 35:07

XY with

35:04 - 35:09

YX SO trading the roles of X and Y so

35:07 - 35:12

the Symmetry that I'm using is that any

35:09 - 35:14

formula I get that involves x's and y's

35:12 - 35:15

if I trade all the x's and replace them

35:14 - 35:18

by y's and trade all the Y's and replace

35:15 - 35:19

them by X's then I'll have it a correct

35:18 - 35:21

formula on the other way so everywhere I

35:19 - 35:23

see a y I'm making an X and everywhere I

35:21 - 35:27

see an X I make it a y the switch will

35:23 - 35:29

take place so why is that that's because

35:27 - 35:33

the that's just an accident of this

35:29 - 35:33

equation that's

35:34 - 35:38

because so the Symmetry

35:45 - 35:52

explained is that the equation is y = 1

35:48 - 35:55

/x but that's the same thing as XY = 1

35:52 - 35:59

If I multiply through by X which is the

35:55 - 36:02

same thing as x = 1 y so here's where

35:59 - 36:02

the X and the Y get

36:04 - 36:11

reversed okay now if you don't trust

36:07 - 36:15

this explanation you can also

36:11 - 36:15

get get the Y

36:16 - 36:20

intercept by

36:20 - 36:26

plugging xal 0 into the into the

36:24 - 36:29

equation

36:26 - 36:32

star

36:29 - 36:35

okay we plugged y equals 0 in and we got

36:32 - 36:39

the x value and you could do the same

36:35 - 36:39

thing analogously the other

36:42 - 36:49

way all right so I'm almost done with

36:45 - 36:55

the with the geometry problem and uh

36:49 - 36:55

let's uh let's finish it off

36:56 - 37:00

now

36:58 - 37:02

well let me hold off for one second

37:00 - 37:04

before I finish it off what I'd like to

37:02 - 37:06

say is just make one more tiny remark

37:04 - 37:08

all right and this is the hardest part

37:06 - 37:11

of calculus in my

37:08 - 37:17

opinion so the hardest part of

37:11 - 37:20

calculus is that we call it one variable

37:17 - 37:23

calculus but we're perfectly happy to

37:20 - 37:27

deal with four variables at a time or

37:23 - 37:30

five or any number in this problem I had

37:27 - 37:33

an x a y an x0 and a y z that's already

37:30 - 37:36

four different things they have various

37:33 - 37:37

interrelationships between them so of

37:36 - 37:39

course the manipulations we do with them

37:37 - 37:41

are algebraic and when we're doing the

37:39 - 37:43

the the derivatives we just consider one

37:41 - 37:44

what's known as one variable calculus

37:43 - 37:47

but really there are millions of

37:44 - 37:49

variables floating around potentially so

37:47 - 37:50

that's what makes things complicated and

37:49 - 37:53

that's something that you have to get

37:50 - 37:55

used to now there's something else which

37:53 - 37:58

is more subtle and that I think many

37:55 - 38:00

people who teach the subject or use the

37:58 - 38:01

subject aren't aware because they've

38:00 - 38:03

already entered into the language and

38:01 - 38:06

they're not uh they're so comfortable

38:03 - 38:08

with it that they don't even notice this

38:06 - 38:12

confusion there's something deliberately

38:08 - 38:15

sloppy about the way we deal with these

38:12 - 38:17

variables the reason is very simple

38:15 - 38:19

there are already four variables here I

38:17 - 38:22

don't want to create six names for

38:19 - 38:25

variables or eight names for

38:22 - 38:28

variables and but really in this problem

38:25 - 38:32

there were about eight I just slipped

38:28 - 38:35

them by you so why is that well notice

38:32 - 38:36

that the first time that I got a formula

38:35 - 38:40

for y z

38:36 - 38:44

here it was this point and so the

38:40 - 38:48

formula for y0 which I plugged in right

38:44 - 38:52

here was from the the equation of the

38:48 - 38:56

curve y0 = 1x0 the second time I did it

38:52 - 38:58

I did not use y = 1X I used this

38:56 - 38:59

equation here

38:58 - 39:03

so this is

38:59 - 39:05

not y = 1X that's the wrong thing to do

39:03 - 39:07

that's an easy mistake to make if if the

39:05 - 39:09

formulas are all a blur to you and

39:07 - 39:13

you're not paying attention to where

39:09 - 39:15

they are on the diagram you see that Y

39:13 - 39:18

intercept that x intercept calculation

39:15 - 39:21

there involved where this horizontal

39:18 - 39:25

line met this diagonal line and Y equals

39:21 - 39:25

z represented this line

39:25 - 39:30

here so the liness is that y means two

39:29 - 39:33

different

39:30 - 39:36

things and we do this constantly because

39:33 - 39:38

it's way way more complicated not to do

39:36 - 39:40

it Con to do it it's much more

39:38 - 39:43

convenient for us to allow ourselves a

39:40 - 39:47

flexibility to change the role that this

39:43 - 39:49

letter plays in the middle of the of the

39:47 - 39:50

computation and similarly later on if I

39:49 - 39:54

had done this by this more

39:50 - 39:56

straightforward method for the uh Y

39:54 - 39:57

intercept I would have set x equal to Z

39:56 - 40:01

that would have been this vertical line

39:57 - 40:03

which is x equals 0 but I didn't change

40:01 - 40:07

the letter X when I did that because

40:03 - 40:08

that would be a waste for us so this

40:07 - 40:11

this is this is one of the main

40:08 - 40:13

confusions that happens if you can uh

40:11 - 40:17

keep yourself straight you're you're a

40:13 - 40:21

lot better off and and as I say this is

40:17 - 40:24

this is uh this is one of the

40:21 - 40:25

complexities all right so now let's

40:24 - 40:29

finish off the problem and let me

40:25 - 40:29

finally get this area here

40:31 - 40:37

so actually I'll just finish it off

40:32 - 40:37

right here so the area of the

40:39 - 40:45

triangle is well it's the base times the

40:42 - 40:49

height the base is 2x0 the height is 2

40:45 - 40:55

y0 and a half of that so it's a half 2x0

40:49 - 40:58

* 2 y0 which is 2 x0 y0 which is lo and

40:55 - 41:00

behold two

40:58 - 41:01

so the amusing thing in this case is it

41:00 - 41:05

actually didn't matter what x0 and Y Z

41:01 - 41:08

are we get the same answer every

41:05 - 41:11

time that's just an accident of the

41:08 - 41:14

function 1 /x happens to be the function

41:11 - 41:14

with that

41:19 - 41:25

property all right so we have still have

41:22 - 41:29

more business today serious business so

41:25 - 41:29

let me continue

41:31 - 41:36

so first of all I want to give you a few

41:34 - 41:36

more

41:40 - 41:46

notations

41:42 - 41:47

and these are just other ways that

41:46 - 41:50

people

41:47 - 41:53

uh refer uh notations that people use to

41:50 - 41:55

refer to derivatives and the first one

41:53 - 41:58

is the following we already wrote Y is

41:55 - 42:00

equal to F ofx and so when we write

41:58 - 42:07

deltay that means the same thing as

42:00 - 42:13

Delta F that's a typical notation and

42:07 - 42:16

previously we wrote um f Prime for the

42:13 - 42:19

derivative so this is this is so this is

42:16 - 42:22

Newton's notation for the

42:19 - 42:25

derivative okay but there are other

42:22 - 42:28

notations and one of them is DF

42:25 - 42:31

DX and another one is d ydx meaning

42:28 - 42:34

exactly the same thing and sometimes we

42:31 - 42:38

let the function slip down below so that

42:34 - 42:42

becomes d by DX of f or D by

42:38 - 42:45

DX of Y so these are all notations that

42:42 - 42:48

are used for the derivative and these

42:45 - 42:48

were initiated by

42:48 - 42:53

livets

42:50 - 42:56

and these notations are um used

42:53 - 42:58

interchangeably sometimes uh practically

42:56 - 43:02

together they both turn out to be

42:58 - 43:05

extremely useful this one omits notice

43:02 - 43:08

that this thing omits the uh underlying

43:05 - 43:10

base Point x0 that's one of the

43:08 - 43:14

nuisances it doesn't give you all the

43:10 - 43:16

information but there are lots of uh

43:14 - 43:19

situations like that

43:16 - 43:20

where where uh people leave out some of

43:19 - 43:24

the important information you have to

43:20 - 43:28

fill it in from Context so that's

43:24 - 43:31

another couple of notations

43:28 - 43:34

so now I have one more calculation for

43:31 - 43:37

you today uh I carried out this

43:34 - 43:41

calculation of the derivative of the

43:37 - 43:41

um of the

43:42 - 43:48

um the the derivative of the function 1

43:45 - 43:51

/x I want to take care of some other

43:48 - 43:51

powers so let's do

43:56 - 43:59

that

43:59 - 44:02

so example

44:03 - 44:13

two is going to be the function F ofx is

44:07 - 44:16

X to the n and = 1 2 3 one of these

44:13 - 44:19

guys and now what we're trying to figure

44:16 - 44:22

out is the derivative with respect to X

44:19 - 44:25

of x to the n in our new new notation

44:22 - 44:25

what this is equal

44:26 - 44:31

to

44:28 - 44:36

so again we're going to form this

44:31 - 44:38

expression Delta F Delta X and we're

44:36 - 44:40

going to make some algebraic

44:38 - 44:45

simplification so what we plug in for

44:40 - 44:50

Delta f is X+ Delta x to the N minus X

44:45 - 44:52

the N / Delta X now before let me just

44:50 - 44:57

stick this in and I'm going to erase it

44:52 - 45:00

before I wrote x0 here and x0 there but

44:57 - 45:02

now I'm going to get rid of it because

45:00 - 45:03

in this particular calculation it's a

45:02 - 45:05

nuisance I don't have an X floating

45:03 - 45:07

around which means something different

45:05 - 45:09

from the X zero and I just don't want to

45:07 - 45:13

have to keep on writing all those

45:09 - 45:15

symbols it's a waste of Blackboard uh

45:13 - 45:17

energy uh there's a total amount of

45:15 - 45:20

energy that I'm you know I've already

45:17 - 45:22

filled up so many blackboards that it's

45:20 - 45:25

just a limited amount of plus I'm trying

45:22 - 45:29

to conserve chalk okay anyway no

45:25 - 45:31

zeros so think of X is fixed again um in

45:29 - 45:35

this case Delta X

45:31 - 45:39

moves and X is

45:35 - 45:41

fixed in this in this

45:39 - 45:43

calculation all right now in order to

45:41 - 45:45

simplify this in order to understand

45:43 - 45:47

algebraically what's going on I need to

45:45 - 45:50

understand what the nth power of a sum

45:47 - 45:54

is and that's a famous formula we only

45:50 - 45:58

need a little tiny bit of it called the

45:54 - 46:01

binomial theorem so the binomial

45:58 - 46:03

theorem

46:01 - 46:05

binomial

46:03 - 46:08

theorem which is in your

46:05 - 46:12

text and uh explained in an in an

46:08 - 46:15

exercise says uh in an appendex sorry

46:12 - 46:17

says that if you take the sum of two

46:15 - 46:20

guys and you take them to the nth power

46:17 - 46:24

that of course is X Plus Delta

46:20 - 46:28

X multiplied by itself n

46:24 - 46:30

times and so the first term

46:28 - 46:34

is X to the N that's when all of the N

46:30 - 46:36

factors come in and then you could have

46:34 - 46:39

this factor of Delta X and all the rest

46:36 - 46:42

X's so at least one term of the form X

46:39 - 46:45

the n minus1 * Delta X and how many

46:42 - 46:46

times does that happen well it happens

46:45 - 46:48

when there's a factor from here from the

46:46 - 46:50

next factor and so on and so on and so

46:48 - 46:53

on there's a total of n

46:50 - 46:57

possible times that that

46:53 - 47:00

happens and now the great thing is that

46:57 - 47:03

with this alone all the rest of the

47:00 - 47:03

terms are

47:04 - 47:10

junk that we won't have to worry about

47:07 - 47:12

so to be more specific the junk there's

47:10 - 47:17

a very careful notation for the junk the

47:12 - 47:22

junk is what's called Big O of Delta x

47:17 - 47:22

s what that means is that these are

47:22 - 47:29

terms of order uh so with

47:28 - 47:33

Delta

47:29 - 47:36

X2 Delta X cubed or

47:33 - 47:36

higher right that's

47:38 - 47:45

how very

47:40 - 47:47

exciting higher order terms okay so this

47:45 - 47:49

is the only algebra that we need to do

47:47 - 47:52

and now we just need to combine it

47:49 - 47:55

together to get our result so now I'm

47:52 - 47:59

going to just carry out the

47:55 - 47:59

cancellations that we

48:01 - 48:10

need so here we go we

48:05 - 48:14

have Delta F over Delta X which remember

48:10 - 48:14

was 1/ Delta X time

48:17 - 48:30

this which is this times now this is X

48:21 - 48:30

the n + n x nus1 Delta X plus this junk

48:31 - 48:37

term minus x to the

48:34 - 48:41

N all right so that's what we have so

48:37 - 48:44

far based on our previous

48:41 - 48:47

calculations now I'm going to do the

48:44 - 48:50

main C cancellation which is

48:47 - 48:59

this all right so that's one over Delta

48:50 - 48:59

x * n x nus1 Delta X plus this term

49:00 - 49:09

here and now I can divide in by Delta X

49:05 - 49:12

so I get N X nus1 Plus now it's O of

49:09 - 49:14

Delta X there's at least one factor of

49:12 - 49:17

Delta X not two factors of Delta X

49:14 - 49:20

because I have to cancel one of

49:17 - 49:21

them and now I can just take the limit

49:20 - 49:25

in the limit this term is going to be

49:21 - 49:28

zero that's why I called it junk

49:25 - 49:31

originally because it disapp appears and

49:28 - 49:35

in math junk is something that goes away

49:31 - 49:39

so this tends to as Delta X goes to zero

49:35 - 49:40

n x n minus1 and so what I've shown you

49:39 - 49:45

is

49:40 - 49:49

that d by DX of x n minus sorry n is

49:45 - 49:49

equal to n x nus

49:50 - 49:55

one so now this is going to be super

49:52 - 49:57

important to you right on your problem

49:55 - 49:59

set in every possible way and I want to

49:57 - 50:01

tell you one thing one way in which it's

49:59 - 50:05

very important and one way that extends

50:01 - 50:05

it immediately so this thing

50:06 - 50:09

extends to

50:10 - 50:17

pols we get quite a lot out of this one

50:13 - 50:21

calculation namely if I take d by DX of

50:17 - 50:24

something like X cubed + 5 x 10th

50:21 - 50:26

power that's going to be equal to

50:24 - 50:32

3x^2 that's applying this rule to X

50:26 - 50:36

cubed and then here I'll get 5 * 10 so

50:32 - 50:38

50 x 9th so this is the type of thing

50:36 - 50:43

that we get out of it and we're going to

50:38 - 50:43

make more hay with that next

50:48 - 50:54

time question yes I turn myself off

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purposes now because we don't happen to

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okay see you next time

Understanding Derivatives: Unlocking the Secrets of Calculus

In this article, we delve into the world of calculus, focusing on the fundamental concept of derivatives. From geometric interpretations to practical applications, we explore how derivatives help us understand changes in measurements across various fields like science, engineering, and economics. By the end, you will not only grasp the essential definition of derivatives but also see their profound implications in real-world scenarios.

What is a Derivative?

A derivative represents the rate of change of a function concerning its variable. In simpler terms, it tells us how a function behaves as its input changes. As we embark on our journey through calculus, we first recognize that understanding derivatives requires looking at geometric interpretations.

Geometric Interpretation of Derivatives

The geometric interpretation of a derivative is often visualized as the slope of the tangent line to a function's graph at a specific point. For instance, given a function ( f(x) ), the tangent line at the point ( (x_0, f(x_0)) ) can be found using the famous slope formula:
[ m = \frac{f(x_0 + \Delta x) - f(x_0)}{\Delta x} ]
Here, ( m ) represents the slope of the tangent line, and as ( \Delta x ) approaches zero, this ratio gives us the derivative of ( f ) at ( x_0 ), denoted as ( f'(x_0) ).

Limits and Secant Lines

Before we can fully appreciate derivatives, we must understand the concept of secant lines and limits. A secant line intersects the function at two points, but as the second point ( Q ) gets closer to point ( P ), the secant line approaches the tangent line. In mathematical terms, we express this using limits:
[ f'(x_0) = \lim_{\Delta x \to 0} \frac{f(x_0 + \Delta x) - f(x_0)}{\Delta x} ]

The Power of Derivatives in Measurement

Derivatives are crucial in numerous fields, from physics to economics. They provide insight into how changes in one quantity affect others. For example, knowing the derivative of a function can help determine the velocity of an object at any point in time.

Real-world Applications

Understanding derivatives allows us to solve various real-life problems. For instance, in business, calculating the marginal cost or profit helps organizations make informed decisions. In science, derivatives help model natural phenomena, such as the rate of reaction in chemistry.

Example: Deriving the Slope

Let’s take a classic example, the function ( f(x) = \frac{1}{x} ). To find its derivative, we apply our limit definition:
[ f'(x_0) = \lim_{\Delta x \to 0} \frac{\frac{1}{x_0 + \Delta x} - \frac{1}{x_0}}{\Delta x} ]

Through simplifications, we discover that:
[ f'(x_0) = -\frac{1}{x_0^2} ]
This result not only gives us the slope of the tangent at any point ( x_0 ) but illustrates the negative relationship between ( x ) and ( f(x) ).

The Importance of Notation

Throughout calculus, different notations are used for derivatives: ( f'(x) ), ( \frac{dy}{dx} ), and ( D_xf ) all signify the same concept. This variety invites clarity and choice according to the context of a problem. Being comfortable with these notations is essential as one progresses through the subject.

Tying it all Together

In calculus, we apply various concepts and techniques to derive derivatives and understand their implications. This interplay forms the backbone of more advanced topics like integration and differential equations.

Engaging with the Concept

While derivatives can initially seem challenging due to their abstract nature, engaging with geometric interpretations can rebuild confidence in calculations. The more familiar one becomes with concepts like limits and slopes, the more intuitive derivatives will appear.

Understanding derivatives opens up a gateway to unraveling the complexities of calculus and its applications, allowing one to transcend beyond calculations into the realms of modeling and real-world problem-solving.

Let Your Curiosity Propel You Forward

As we explore derivatives further, remember that they aren't just academic constructs; they can illuminate the intricacies of the world around you. So, embrace the challenge, for in the realm of calculus lies a profound understanding of change itself—you hold the key to mastering it!