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  • 7/23/2019 Chap12_Sec2 [Compatibility Mode]

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    VECTOR FUNCTIONS

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    VECTOR FUNCTIONS

    Later in this chapter, we are going to use

    vector functions to describe the motion of

    planets and other objects through space.

    Here, we prepare the way by developing

    the calculus of vector functions.

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    12.2

    Derivatives and Integrals

    of Vector Functions

    In this section, we will learn how to:

    Develop the calculus of vector functions.

    VECTOR FUNCTIONS

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    The derivative r of a vector function

    is defined in much the same way as for

    real-valued functions.

    DERIVATIVES

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    if this limit exists.

    DERIVATIVE

    0

    ( ) ( )'( ) lim

    h

    d t h t t

    dt h

    + = =

    r r rr

    Equation 1

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    The geometric significance

    of this definition is shown asfollows.

    DERIVATIVE

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    If the points Pand Q have position

    vectors r(t) and r(t + h), then represents

    the vector r(t + h) r(t).

    This can thereforebe regarded as

    a secant vector.

    SECANT VECTOR

    PQuuur

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    If h > 0, the scalar multiple (1/h)(r(t + h) r(t))

    has the same direction as r(t + h) r(t).

    As h 0, it appears

    that this vector

    approaches a vector

    that lies on the

    tangent line.

    DERIVATIVES

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    For this reason, the vector r(t) is called

    the tangent vector to the curve defined by r

    at the point P,

    provided:

    r(t) exists

    r(t) 0

    TANGENT VECTOR

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    The tangent line to Cat Pis defined to be

    the line through Pparallel to the tangent

    vector r(t).

    TANGENT LINE

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    We will also have occasion to consider

    the unit tangent vector:

    UNIT TANGENT VECTOR

    '( )( )| '( ) |

    tT tt

    = rr

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    The following theorem gives us

    a convenient method for computing

    the derivative of a vector function r:

    Just differentiate each component of r.

    DERIVATIVES

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    If r(t) = f(t), g(t), h(t) = f(t) i + g(t)j + h(t) k,

    where f, g, and h are differentiable functions,

    then:

    r(t) = f(t), g(t), h(t)

    = f(t) i + g(t)j + h(t) k

    DERIVATIVES Theorem 2

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    DERIVATIVES Proof

    0

    0

    0

    0 0 0

    '( )

    1lim [ ( ) ( )]

    1lim ( ), ( ), ( ), ( ), ( ), ( )

    ( ) ( ) ( ) ( ) ( ) ( )lim , ,

    ( ) ( ) ( ) ( ) ( ) ( )lim , lim , lim

    t

    t

    t

    t t t

    t

    t t t

    t

    f t t g t t h t t f t g t h tt

    f t t f t g t t g t h t t h tt t t

    f t t f t g t t g t h t t h t

    t t

    = +

    = + + +

    + + + =

    + + + =

    r

    r r

    '( ), '( ), '( )t

    f t g t h t

    =

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    a. Find the derivative of

    r(t) = (1 + t3) i + tetj + sin 2t k

    b. Find the unit tangent vector at the point

    where t= 0.

    DERIVATIVES Example 1

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    According to Theorem 2, we differentiate

    each component of r:

    r(t) = 3t2 i + (1 t)etj + 2 cos 2t k

    DERIVATIVES Example 1 a

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    As r(0) = i and r(0) =j + 2k, the unit tangent

    vector at the point (1, 0, 0) is:

    DERIVATIVES Example 1 b

    '(0) 2

    (0) | '(0) | 1 4

    1 2

    5 5

    +

    = = +

    = +

    r j k

    T r

    k

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    For the curve ,

    find r(t) and sketch the position vector r(1)

    and the tangent vector r(1).

    DERIVATIVES Example 2

    ( ) (2 )t t t= + r i j

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    We have:

    and

    DERIVATIVES Example 2

    1'( )2

    1'(1)

    2

    tt

    =

    =

    r i j

    r i j

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    The curve is a plane curve.

    Elimination of the parameter from

    the equations , y = 2 t gives:

    y = 2 x2, x 0

    DERIVATIVES Example 2

    x t=

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    The position vector r(1) = i +j starts

    at the origin.

    The tangent vector r(1)

    starts at the

    corresponding point

    (1, 1).

    DERIVATIVES Example 2

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    Find parametric equations for the tangent line

    to the helix with parametric equations

    x = 2 cos t y = sin t z = t

    at the point (0, 1, /2).

    DERIVATIVES Example 3

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    The vector equation of the helix is:

    r(t) = 2 cos t, sin t, t

    Thus,

    r

    (t) =

    2 sin t, cos t, 1

    DERIVATIVES Example 3

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    The parameter value corresponding to

    the point (0, 1, /2) is t= /2.

    So, the tangent vector there is:

    r(/2) = 2, 0, 1

    DERIVATIVES Example 3

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    The tangent line is the line through

    (0, 1, /2) parallel to the vector 2, 0, 1.

    So, by Equations 2 in Section 12.5,

    its parametric equations are:

    DERIVATIVES

    2 12

    x t y z t

    = = = +

    Example 3

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    The helix and the tangent line in

    the Example 3 are shown.

    DERIVATIVES

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    Just as for real-valued functions,

    the second derivative of a vector function r

    is the derivative of r, that is, r = (r).

    For instance, the second derivative

    of the function in Example 3 is:

    r(t) =2 cos t, sin t, 0

    SECOND DERIVATIVE

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    The next theorem shows that

    the differentiation formulas for real-valued

    functions have their counterparts for

    vector-valued functions.

    DIFFERENTIATION RULES

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    Suppose:

    u and v are differentiable vector functions

    c is a scalar

    fis a real-valued function

    DIFFERENTIATION RULES Theorem 3

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    Then,

    DIFFERENTIATION RULES

    1. [ ( ) ( )] ( ) ( )

    2. [ ( )] ( )

    3. [ ( ) ( )] '( ) ( ) ( ) ( )

    dt t t t

    dt

    d c t c t dt

    df t t f t t f t t

    dt

    + = +

    =

    = +

    u v u' v'

    u u'

    u u u'

    Theorem 3

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    DIFFERENTIATION RULES Theorem 3

    ( )

    4. [ ( ) ( )] ( ) ( ) ( ) ( )

    5. [ ( ) ( )] ( ) ( ) ( ) ( )

    6. [ ( ( ))] '( ) ( ) (Chain Rule)

    dt t t t t t

    dt

    dt t t t t t

    dt

    d f t f t f tdt

    = +

    = +

    =

    u v u' v u v'

    u v u' v u v'

    u u'

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    This theorem can be proved either:

    Directly from Definition 1

    By using Theorem 2 and the corresponding

    differentiation formulas for real-valued functions

    DIFFERENTIATION RULES

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    The proof of Formula 4 follows.

    The remaining are left as exercises.

    DIFFERENTIATION RULES

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    Let

    u(t) = f1(t), f2(t), f3(t)

    v(t) = g1(t), g2(t), g3(t)

    Then,

    FORMULA 4 Proof

    1 1 2 2 3 3

    3

    1

    ( ) ? ( )

    ( ) ( ) ( ) ( ) ( ) ( )

    ( ) ( )i i

    i

    t t

    f t g t f t g t f t g t

    f t g t=

    = + +

    =

    u v

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    So, the ordinary Product Rule gives:

    FORMULA 4 Proof

    3

    1

    3

    1

    3

    1

    3 3

    1 1

    [ ( ) ( )] ( ) ( )

    [ ( ) ( )]

    [ '( ) ( ) ( ) '( )]

    '( ) ( ) ( ) '( )

    ( ) ( ) ( ) ( )

    i i

    i

    i i

    i

    i i i i

    i

    i i i i

    i i

    d dt t f t g t

    dt dt d

    f t g tdt

    f t g t f t g t

    f t g t f t g t

    t t t t

    =

    =

    =

    = =

    =

    =

    = +

    = +

    = +

    u v

    u' v u v'

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    Show that, if |r(t)| = c(a constant),

    then r(t) is orthogonal to r(t) for all t.

    DIFFERENTIATION RULES Example 4

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    Since

    r(t) r(t) = |r(t)|2 = c2

    and c2 is a constant,

    Formula 4 of Theorem 3 gives:

    DIFFERENTIATION RULES Example 4

    0 [ ( ) ( )]

    '( ) ( ) ( ) '( )2 '( ) ( )

    dt t

    dt

    t t t t

    t t

    =

    = + =

    r r

    r r r r

    r r

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    Thus,

    r(t) r(t) = 0

    This says that r(t) is orthogonal to r(t).

    DIFFERENTIATION RULES

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    Geometrically, this result says:

    If a curve lies on a sphere with center

    the origin, then the tangent vector r(t) is

    always perpendicular to the position vector r(t).

    DIFFERENTIATION RULES

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    The definite integral of a continuous vector

    function r(t) can be defined in much the same

    way as for real-valued functionsexcept that

    the integral is a vector.

    INTEGRALS

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    However, then, we can express

    the integral of rin terms of the integrals

    of its component functions f, g, and h

    as follows.

    We use the notation of Chapter 5.

    INTEGRALS

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    INTEGRALS

    *

    1

    * *

    1 1

    *

    1

    ( )

    lim ( )

    lim ( ) ( )

    ( )

    b

    a

    n

    in

    i

    n n

    i in

    i i

    n

    i

    i

    t dt

    t t

    f t t g t t

    h t t

    =

    = =

    =

    =

    = +

    +

    r

    r

    i j

    k

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    Thus,

    This means that we can evaluate an integral of a vector

    function by integrating each component function.

    INTEGRALS

    r(t)dta

    b

    = f(t)dta

    b

    i + g(t)dta

    b

    j + h(t)dta

    b

    k

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    We can extend the Fundamental Theorem

    of Calculus to continuous vector functions:

    Here, R is an antiderivative of r, that is, R(t) = r(t).

    We use the notation r(t) dtfor indefinite integrals(antiderivatives).

    INTEGRALS

    ]b

    a(t) ( ) ( ) ( )

    b

    adt t b a= = r R R R

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    If r(t) = 2 cos t i + sin tj + 2t k, then

    where:

    C is a vector constant of integration

    INTEGRALS Example 5

    r(t)dt = 2cos t dt( )i + sint dt( )j + 2t dt( )k= 2sin ti cos tj + t2k + C

    2

    2 200

    2

    ( ) [2sin cos ]

    2

    4

    t dt t t t

    = +

    = + +

    r i j k

    i j k