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Math2510Section14 4

This section discusses gradients and directional derivatives in the plane, explaining how to compute the rate of change of a function in arbitrary directions using unit vectors. It introduces the concept of the directional derivative and provides a formula that relates it to the gradient of the function. The gradient vector is shown to represent the maximum rate of change of the function at a given point.

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0% found this document useful (0 votes)
16 views37 pages

Math2510Section14 4

This section discusses gradients and directional derivatives in the plane, explaining how to compute the rate of change of a function in arbitrary directions using unit vectors. It introduces the concept of the directional derivative and provides a formula that relates it to the gradient of the function. The gradient vector is shown to represent the maximum rate of change of the function at a given point.

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Section 14.

4
Gradients and Directional Derivatives in the
Plane
14.4 Gradients and Directional Derivatives in the Plane

The partial derivatives of a function f tell us the rate of change


of f in the directions parallel to the coordinate axes.
14.4 Gradients and Directional Derivatives in the Plane

The partial derivatives of a function f tell us the rate of change


of f in the directions parallel to the coordinate axes.
In this section we see how to compute the rate of change of f in
an arbitrary direction.
Directional Derivative

Suppose we want
to compute the rate of change
of a function f (x, y) at the
point P = (a, b) in the direction
of the unit vector ~u = u1~i + u2~j.
Directional Derivative

Suppose we want
to compute the rate of change
of a function f (x, y) at the
point P = (a, b) in the direction
of the unit vector ~u = u1~i + u2~j.
For h > 0, consider the point
Q = (a + hu1 , b + hu2 ) whose
displacement from P is h~u .
Directional Derivative

Suppose we want
to compute the rate of change
of a function f (x, y) at the
point P = (a, b) in the direction
of the unit vector ~u = u1~i + u2~j.
For h > 0, consider the point
Q = (a + hu1 , b + hu2 ) whose
displacement from P is h~u .
Since ||~u || = 1 , the distance
from P to Q is h.
Directional Derivative

Suppose we want
to compute the rate of change
of a function f (x, y) at the
point P = (a, b) in the direction
of the unit vector ~u = u1~i + u2~j.
For h > 0, consider the point
Q = (a + hu1 , b + hu2 ) whose
displacement from P is h~u .
Since ||~u || = 1 , the distance
from P to Q is h.
Thus, the average rate of change in f from P to Q is given by

Change in f f (a + hu1 , b + hu2 ) − f (a, b)


=
Distance from P to Q h
Directional Derivative

Suppose we want
to compute the rate of change
of a function f (x, y) at the
point P = (a, b) in the direction
of the unit vector ~u = u1~i + u2~j.
For h > 0, consider the point
Q = (a + hu1 , b + hu2 ) whose
displacement from P is h~u .
Since ||~u || = 1 , the distance
from P to Q is h.
Thus, the average rate of change in f from P to Q is given by

Change in f f (a + hu1 , b + hu2 ) − f (a, b)


=
Distance from P to Q h
Taking the limit as h → 0 gives the instantaneous rate of change and
the following definition.
Directional Derivative of f at (a, b) in the Direction of a
Unit Vector ~u
If ~u = u1~i + u2~j is a unit vector, we define the directional
derivative,f~u , by

f (a + hu1 , b + hu2 ) − f (a, b)


f~u = lim
h→0 h
provided the limit exists.
Directional Derivative of f at (a, b) in the Direction of a
Unit Vector ~u
If ~u = u1~i + u2~j is a unit vector, we define the directional
derivative,f~u , by

f (a + hu1 , b + hu2 ) − f (a, b)


f~u = lim
h→0 h
provided the limit exists.
Notice that if ~u = ~i , so u1 = 1, u2 = 0, then the directional
derivative is fx , since

f (a + h, b) − f (a, b)
f~i = lim = fx
h→0 h
Directional Derivative of f at (a, b) in the Direction of a
Unit Vector ~u
If ~u = u1~i + u2~j is a unit vector, we define the directional
derivative,f~u , by

f (a + hu1 , b + hu2 ) − f (a, b)


f~u = lim
h→0 h
provided the limit exists.
Notice that if ~u = ~i , so u1 = 1, u2 = 0, then the directional
derivative is fx , since

f (a + h, b) − f (a, b)
f~i = lim = fx
h→0 h

Similarly, if ~u = ~j then the directional derivative f~j = fy .


What If We Do Not Have a Unit Vector?
We defined f~u for ~u a unit vector. If ~v is not a unit vector,~v 6= 0 ,
we construct a unit vector ~u = ~v /||~v || in the same direction as ~v
and define the rate of change of f in the direction of ~v as f~u .
What If We Do Not Have a Unit Vector?
We defined f~u for ~u a unit vector. If ~v is not a unit vector,~v 6= 0 ,
we construct a unit vector ~u = ~v /||~v || in the same direction as ~v
and define the rate of change of f in the direction of ~v as f~u .
Example
For each of the functions f , g, and h in the following figure,
decide whether the directional derivative at the indicated point
is positive, negative, or zero, in the direction of the vector
~v = ~i + 2~j, and in the direction of the vector w
~ = 2~i + ~j .
Computing Directional Derivatives
If f is differentiable, we will now see how to use local linearity to
find a formula for the directional derivative which does not
involve a limit.
Computing Directional Derivatives
If f is differentiable, we will now see how to use local linearity to
find a formula for the directional derivative which does not
involve a limit. If ~u is a unit vector, the definition of f~u says
f (a + hu1 , b + hu2 ) − f (a, b) ∆f
f~u = lim = lim
h→0 h h→0 h

where ∆f = f (a + hu1 , b + hu2 ) − f (a, b) is the change in f .


Computing Directional Derivatives
If f is differentiable, we will now see how to use local linearity to
find a formula for the directional derivative which does not
involve a limit. If ~u is a unit vector, the definition of f~u says
f (a + hu1 , b + hu2 ) − f (a, b) ∆f
f~u = lim = lim
h→0 h h→0 h

where ∆f = f (a + hu1 , b + hu2 ) − f (a, b) is the change in f . We


write ∆x for the change in x, so ∆x = (a + hu1 ) − a = hu1 ;
similarly ∆y = hu2 . Using local linearity, we have
∆f ≈ fx (a, b)∆x + fy (a, b)∆y = fx (a, b)hu1 + fy (a, b)hu2
Computing Directional Derivatives
If f is differentiable, we will now see how to use local linearity to
find a formula for the directional derivative which does not
involve a limit. If ~u is a unit vector, the definition of f~u says
f (a + hu1 , b + hu2 ) − f (a, b) ∆f
f~u = lim = lim
h→0 h h→0 h

where ∆f = f (a + hu1 , b + hu2 ) − f (a, b) is the change in f . We


write ∆x for the change in x, so ∆x = (a + hu1 ) − a = hu1 ;
similarly ∆y = hu2 . Using local linearity, we have
∆f ≈ fx (a, b)∆x + fy (a, b)∆y = fx (a, b)hu1 + fy (a, b)hu2
Thus, dividing by h gives
∆f fx (a, b)hu1 + fy (a, b)hu2
≈ = fx (a, b)u1 + fy (a, b)u2
h h
Computing Directional Derivatives
If f is differentiable, we will now see how to use local linearity to
find a formula for the directional derivative which does not
involve a limit. If ~u is a unit vector, the definition of f~u says
f (a + hu1 , b + hu2 ) − f (a, b) ∆f
f~u = lim = lim
h→0 h h→0 h

where ∆f = f (a + hu1 , b + hu2 ) − f (a, b) is the change in f . We


write ∆x for the change in x, so ∆x = (a + hu1 ) − a = hu1 ;
similarly ∆y = hu2 . Using local linearity, we have
∆f ≈ fx (a, b)∆x + fy (a, b)∆y = fx (a, b)hu1 + fy (a, b)hu2
Thus, dividing by h gives
∆f fx (a, b)hu1 + fy (a, b)hu2
≈ = fx (a, b)u1 + fy (a, b)u2
h h
This approximation becomes exact as h → 0, so we have the
following formula:
f~u = fx (a, b)u1 + fy (a, b)u2 .
Example
Calculate the directional derivative of f f (x, y) = x 2 − y 2 at
(0, 1) in the direction of the vector ~i − ~j.
The Directional Derivative and the Gradient

Notice that the expression for f~u can be written as a dot product
of ~u and a new vector:

f~u = fx (a, b)u1 + fy (a, b)u2 = grad f (a, b) · ~u .


where
grad f (a, b) = fx (a, b)~i + fy (a, b)~j
is a very important vector called the gradient of f at the point
(a, b).
The Directional Derivative and the Gradient

Notice that the expression for f~u can be written as a dot product
of ~u and a new vector:

f~u = fx (a, b)u1 + fy (a, b)u2 = grad f (a, b) · ~u .


where
grad f (a, b) = fx (a, b)~i + fy (a, b)~j
is a very important vector called the gradient of f at the point
(a, b).
Example
2
Find the gradient vector of f (x, y) = y 2 + ex at the point (1, 1).
Alternative Notation for the Gradient

∂f ~ ∂f ~
You can think of ∂x i + ∂y j as the result of applying the vector
operator (pronounced “del”)
∂~ ∂
∇= i + ~j
∂x ∂y

to the function f .
Alternative Notation for the Gradient

∂f ~ ∂f ~
You can think of ∂x i + ∂y j as the result of applying the vector
operator (pronounced “del”)
∂~ ∂
∇= i + ~j
∂x ∂y

to the function f .
Thus, we get the alternative notation

grad f = ∇f
Alternative Notation for the Gradient

∂f ~ ∂f ~
You can think of ∂x i + ∂y j as the result of applying the vector
operator (pronounced “del”)
∂~ ∂
∇= i + ~j
∂x ∂y

to the function f .
Thus, we get the alternative notation

grad f = ∇f

If z = f (x, y ), we can write grad z or ∇z for grad f or for ∇f .


What Does the Gradient Tell Us?
The fact that f~u = ∇f · ~u enables us to see what the gradient
vector represents.
What Does the Gradient Tell Us?
The fact that f~u = ∇f · ~u enables us to see what the gradient
vector represents. Suppose θ is the angle between the vectors
∇f and ~u . At the point (a, b), we have

f~u = ∇f · ~u = ||∇f || ||~u || cos θ = ||∇f || cos θ.


What Does the Gradient Tell Us?
The fact that f~u = ∇f · ~u enables us to see what the gradient
vector represents. Suppose θ is the angle between the vectors
∇f and ~u . At the point (a, b), we have

f~u = ∇f · ~u = ||∇f || ||~u || cos θ = ||∇f || cos θ.

Imagine that ∇f is fixed and that ~u can rotate. The maximum


value of f~u occurs when cos θ = 1, so θ = 0 and ~u is pointing in
the direction of ∇f . Then

Maximum f~u = ||∇f || cos 0 = ||∇f ||.


What Does the Gradient Tell Us?
The fact that f~u = ∇f · ~u enables us to see what the gradient
vector represents. Suppose θ is the angle between the vectors
∇f and ~u . At the point (a, b), we have

f~u = ∇f · ~u = ||∇f || ||~u || cos θ = ||∇f || cos θ.

Imagine that ∇f is fixed and that ~u can rotate. The maximum


value of f~u occurs when cos θ = 1, so θ = 0 and ~u is pointing in
the direction of ∇f . Then

Maximum f~u = ||∇f || cos 0 = ||∇f ||.

The minimum value of f~u occurs when cos θ = −1, so θ = π and


~u is pointing in the direction opposite to ∇f . Then

Minimum f~u = ||∇f || cos π = −||∇f ||.


What Does the Gradient Tell Us?
The fact that f~u = ∇f · ~u enables us to see what the gradient
vector represents. Suppose θ is the angle between the vectors
∇f and ~u . At the point (a, b), we have

f~u = ∇f · ~u = ||∇f || ||~u || cos θ = ||∇f || cos θ.

Imagine that ∇f is fixed and that ~u can rotate. The maximum


value of f~u occurs when cos θ = 1, so θ = 0 and ~u is pointing in
the direction of ∇f . Then

Maximum f~u = ||∇f || cos 0 = ||∇f ||.

The minimum value of f~u occurs when cos θ = −1, so θ = π and


~u is pointing in the direction opposite to ∇f . Then

Minimum f~u = ||∇f || cos π = −||∇f ||.

When θ = π/2 or 3π/2, so cos θ = 0, the directional derivative


is zero.
The Gradient Vector and Contours

The following figure


shows that the gradient vector
at a point is perpendicular to
the contour through that point.
The Gradient Vector and Contours

The following figure


shows that the gradient vector
at a point is perpendicular to
the contour through that point.
If the contours represent
equally spaced f -values and f is
differentiable, local linearity tell
us that the contours of f around
the point (a, b) appear straight,
parallel, and equally spaced.
The Gradient Vector and Contours

The following figure


shows that the gradient vector
at a point is perpendicular to
the contour through that point.
If the contours represent
equally spaced f -values and f is
differentiable, local linearity tell
us that the contours of f around
the point (a, b) appear straight,
parallel, and equally spaced.
The greatest rate of
change is obtained by moving in
the direction that takes us to the
next contour in the shortest possible distance: that is, perpendicular
to the contour.
Geometric Properties of the Gradient Vector in the
Plane

If f is a differentiable function at the point (a, b) and


∇f (a, b) 6= 0 , then:
Geometric Properties of the Gradient Vector in the
Plane

If f is a differentiable function at the point (a, b) and


∇f (a, b) 6= 0 , then:
I The direction of ∇f (a, b) is
I Perpendicular to the contour of f through (a, b).
I In the direction of increasing f .
Geometric Properties of the Gradient Vector in the
Plane

If f is a differentiable function at the point (a, b) and


∇f (a, b) 6= 0 , then:
I The direction of ∇f (a, b) is
I Perpendicular to the contour of f through (a, b).
I In the direction of increasing f .
I The magnitude of the gradient vector, ||∇f || , is
I The maximum rate of change of f at that point.
I Large when the contours are close together and small
when they are far apart.
Example
An ant is on a metal plate whose temperature at (x, y) is
3x 2 y − y 3 degrees Celsius. When it is at the point (5, 1) it is
anxious to move in the direction in which the temperature drops
most rapidly. Give the unit vector in that direction.
Thank You

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