Taylor and Maclaurin Series

In the previous two sections we discussed how to find power series representations for certain types of functions––specifically, functions related to geometric series. Here we discuss power series representations for other types of functions. In particular, we address the following questions: Which functions can be represented by power series and how do we find such representations? If we can find a power series representation for a particular function f

and the series converges on some interval, how do we prove that the series actually converges to f?

Overview of Taylor/Maclaurin Series

Consider a function f

that has a power series representation at x=a.

Then the series has the form

n=0cn(xa)n=c0+c1(xa)+c2(xa)2+.

What should the coefficients be? For now, we ignore issues of convergence, but instead focus on what the series should be, if one exists. We return to discuss convergence later in this section. If the series [link] is a representation for f

at x=a,

we certainly want the series to equal f(a)

at x=a.

Evaluating the series at x=a,

we see that

n=0cn(xa)n=c0+c1(aa)+c2(aa)2+=c0.

Thus, the series equals f(a)

if the coefficient c0=f(a).

In addition, we would like the first derivative of the power series to equal f(a)

at x=a.

Differentiating [link] term-by-term, we see that

ddx(n=0cn(xa)n)=c1+2c2(xa)+3c3(xa)2+.

Therefore, at x=a,

the derivative is

ddx(n=0cn(xa)n)=c1+2c2(aa)+3c3(aa)2+=c1.

Therefore, the derivative of the series equals f(a)

if the coefficient c1=f(a).

Continuing in this way, we look for coefficients cn such that all the derivatives of the power series [link] will agree with all the corresponding derivatives of f

at x=a.

The second and third derivatives of [link] are given by

d2dx2(n=0cn(xa)n)=2c2+3·2c3(xa)+4·3c4(xa)2+

and

d3dx3(n=0cn(xa)n)=3·2c3+4·3·2c4(xa)+5·4·3c5(xa)2+.

Therefore, at x=a,

the second and third derivatives

d2dx2(n=0cn(xa)n)=2c2+3·2c3(aa)+4·3c4(aa)2+=2c2

and

d3dx3(n=0cn(xa)n)=3·2c3+4·3·2c4(aa)+5·4·3c5(aa)2+=3·2c3

equal f(a)

and f(a),

respectively, if c2=f(a)2

and c3=f(a)3·2.

More generally, we see that if f

has a power series representation at x=a,

then the coefficients should be given by cn=f(n)(a)n!.

That is, the series should be

n=0f(n)(a)n!(xa)n=f(a)+f(a)(xa)+f(a)2!(xa)2+f(a)3!(xa)3+.

This power series for f

is known as the Taylor series for f

at a.

If a=0,

then this series is known as the Maclaurin series for f.

Definition

If f

has derivatives of all orders at x=a,

then the Taylor series for the function f

at a

is

n=0f(n)(a)n!(xa)n=f(a)+f(a)(xa)+f(a)2!(xa)2++f(n)(a)n!(xa)n+.

The Taylor series for f

at 0 is known as the Maclaurin series for f.

Later in this section, we will show examples of finding Taylor series and discuss conditions under which the Taylor series for a function will converge to that function. Here, we state an important result. Recall from [link] that power series representations are unique. Therefore, if a function f

has a power series at a,

then it must be the Taylor series for f

at a.

Uniqueness of Taylor Series

If a function f

has a power series at a that converges to f

on some open interval containing a, then that power series is the Taylor series for f

at a.

The proof follows directly from [link].

To determine if a Taylor series converges, we need to look at its sequence of partial sums. These partial sums are finite polynomials, known as Taylor polynomials.

Visit the MacTutor History of Mathematics archive to read brief biographies of Brook Taylor and Colin Maclaurin and how they developed the concepts named after them.

Taylor Polynomials

The nth partial sum of the Taylor series for a function f

at a

is known as the nth Taylor polynomial. For example, the 0th, 1st, 2nd, and 3rd partial sums of the Taylor series are given by

p0(x)=f(a),p1(x)=f(a)+f(a)(xa),p2(x)=f(a)+f(a)(xa)+f(a)2!(xa)2,p3(x)=f(a)+f(a)(xa)+f(a)2!(xa)2+f(a)3!(xa)3,

respectively. These partial sums are known as the 0th, 1st, 2nd, and 3rd Taylor polynomials of f

at a,

respectively. If a=0,

then these polynomials are known as Maclaurin polynomials for f.

We now provide a formal definition of Taylor and Maclaurin polynomials for a function f.

Definition

If f

has n derivatives at x=a,

then the nth Taylor polynomial for f

at a

is

pn(x)=f(a)+f(a)(xa)+f(a)2!(xa)2+f(a)3!(xa)3++f(n)(a)n!(xa)n.

The nth Taylor polynomial for f

at 0 is known as the nth Maclaurin polynomial for f.

We now show how to use this definition to find several Taylor polynomials for f(x)=lnx

at x=1.

Finding Taylor Polynomials

Find the Taylor polynomials p0,p1,p2

and p3

for f(x)=lnx

at x=1.

Use a graphing utility to compare the graph of f

with the graphs of p0,p1,p2

and p3.

To find these Taylor polynomials, we need to evaluate f

and its first three derivatives at x=1.

f(x)=lnxf(1)=0f(x)=1xf(1)=1f(x)=1x2f(1)=−1f(x)=2x3f(1)=2

Therefore,

p0(x)=f(1)=0,p1(x)=f(1)+f(1)(x1)=x1,p2(x)=f(1)+f(1)(x1)+f(1)2(x1)2=(x1)12(x1)2,p3(x)=f(1)+f(1)(x1)+f(1)2(x1)2+f(1)3!(x1)3=(x1)12(x1)2+13(x1)3.

The graphs of y=f(x)

and the first three Taylor polynomials are shown in [link].

This graph has four curves. The first is the function f(x)=ln(x). The second function is psub1(x)=x-1. The third is psub2(x)=(x-1)-1/2(x-1)^2. The fourth is psub3(x)=(x-1)-1/2(x-1)^2 +1/3(x-1)^3. The curves are very close around x = 1.

Find the Taylor polynomials p0,p1,p2

and p3

for f(x)=1x2

at x=1.

p0(x)=1;p1(x)=12(x1);p2(x)=12(x1)+3(x1)2;p3(x)=12(x1)+3(x1)24(x1)3
Hint

Find the first three derivatives of f

and evaluate them at x=1.

We now show how to find Maclaurin polynomials for ex, sinx,

and cosx.

As stated above, Maclaurin polynomials are Taylor polynomials centered at zero.

Finding Maclaurin Polynomials

For each of the following functions, find formulas for the Maclaurin polynomials p0,p1,p2

and p3.

Find a formula for the nth Maclaurin polynomial and write it using sigma notation. Use a graphing utilty to compare the graphs of p0,p1,p2

and p3

with f.

  1. f(x)=ex
  2. f(x)=sinx
  3. f(x)=cosx
  1. Since f(x)=ex,

    we know that

    f(x)=f(x)=f(x)==f(n)(x)=ex

    for all positive integers n. Therefore,


    f(0)=f(0)=f(0)==f(n)(0)=1

    for all positive integers n. Therefore, we have


    p0(x)=f(0)=1,p1(x)=f(0)+f(0)x=1+x,p2(x)=f(0)+f(0)x+f(0)2!x2=1+x+12x2,p3(x)=f(0)+f(0)x+f(0)2x2+f(0)3!x3=1+x+12x2+13!x3,pn(x)=f(0)+f(0)x+f(0)2x2+f(0)3!x3++f(n)(0)n!xn=1+x+x22!+x33!++xnn!=k=0nxkk!.

    The function and the first three Maclaurin polynomials are shown in [link].


    This graph has four curves. The first is the function f(x)=e^x. The second function is psub0(x)=1. The third is psub1(x) which is an increasing line passing through y=1. The fourth function is psub3(x) which is a curve passing through y=1. The curves are very close around y= 1.

  2. For f(x)=sinx,

    the values of the function and its first four derivatives at

    x=0

    are given as follows:


    f(x)=sinxf(0)=0f(x)=cosxf(0)=1f(x)=sinxf(0)=0f(x)=cosxf(0)=−1f(4)(x)=sinxf(4)(0)=0.

    Since the fourth derivative is

    sinx,

    the pattern repeats. That is,

    f(2m)(0)=0

    and

    f(2m+1)(0)=(−1)m

    for

    m0.

    Thus, we have


    p0(x)=0,p1(x)=0+x=x,p2(x)=0+x+0=x,p3(x)=0+x+013!x3=xx33!,p4(x)=0+x+013!x3+0=xx33!,p5(x)=0+x+013!x3+0+15!x5=xx33!+x55!,

    and for

    m0,
    p2m+1(x)=p2m+2(x)=xx33!+x55!+(−1)mx2m+1(2m+1)!=k=0m(−1)kx2k+1(2k+1)!.

    Graphs of the function and its Maclaurin polynomials are shown in [link].


    This graph has four curves. The first is the function f(x)=sin(x). The second function is psub1(x). The third is psub3(x). The fourth function is psub5(x). The curves are very close around x=0.

  3. For f(x)=cosx,

    the values of the function and its first four derivatives at

    x=0

    are given as follows:


    f(x)=cosxf(0)=1f(x)=sinxf(0)=0f(x)=cosxf(0)=−1f(x)=sinxf(0)=0f(4)(x)=cosxf(4)(0)=1.

    Since the fourth derivative is

    sinx,

    the pattern repeats. In other words,

    f(2m)(0)=(−1)m

    and

    f(2m+1)=0

    for

    m0.

    Therefore,


    p0(x)=1,p1(x)=1+0=1,p2(x)=1+012!x2=1x22!,p3(x)=1+012!x2+0=1x22!,p4(x)=1+012!x2+0+14!x4=1x22!+x44!,p5(x)=1+012!x2+0+14!x4+0=1x22!+x44!,

    and for

    n0,
    p2m(x)=p2m+1(x)=1x22!+x44!+(−1)mx2m(2m)!=k=0m(−1)kx2k(2k)!.

    Graphs of the function and the Maclaurin polynomials appear in [link].


    This graph has four curves. The first is the function f(x)=cos(x). The second function is psub0(x). The third is psub2(x). The fourth function is psub4(x). The curves are very close around y=1

Find formulas for the Maclaurin polynomials p0,p1,p2

and p3

for f(x)=11+x.

Find a formula for the nth Maclaurin polynomial. Write your anwer using sigma notation.

p0(x)=1;p1(x)=1x;p2(x)=1x+x2;p3(x)=1x+x2x3;pn(x)=1x+x2x3++(−1)nxn=k=0n(−1)kxk
Hint

Evaluate the first four derivatives of f

and look for a pattern.

Taylor’s Theorem with Remainder

Recall that the nth Taylor polynomial for a function f

at a is the nth partial sum of the Taylor series for f

at a. Therefore, to determine if the Taylor series converges, we need to determine whether the sequence of Taylor polynomials {pn}

converges. However, not only do we want to know if the sequence of Taylor polynomials converges, we want to know if it converges to f.

To answer this question, we define the remainder Rn(x)

as

Rn(x)=f(x)pn(x).

For the sequence of Taylor polynomials to converge to f,

we need the remainder Rn to converge to zero. To determine if Rn converges to zero, we introduce Taylor’s theorem with remainder. Not only is this theorem useful in proving that a Taylor series converges to its related function, but it will also allow us to quantify how well the nth Taylor polynomial approximates the function.

Here we look for a bound on \|Rn\|.

Consider the simplest case: n=0.

Let p0 be the 0th Taylor polynomial at a for a function f.

The remainder R0 satisfies

R0(x)=f(x)p0(x)=f(x)f(a).

If f

is differentiable on an interval I containing a and x, then by the Mean Value Theorem there exists a real number c between a and x such that f(x)f(a)=f(c)(xa).

Therefore,

R0(x)=f(c)(xa).

Using the Mean Value Theorem in a similar argument, we can show that if f

is n times differentiable on an interval I containing a and x, then the nth remainder Rn satisfies

Rn(x)=f(n+1)(c)(n+1)!(xa)n+1

for some real number c between a and x. It is important to note that the value c in the numerator above is not the center a, but rather an unknown value c between a and x. This formula allows us to get a bound on the remainder Rn. If we happen to know that \|f(n+1)(x)\|

is bounded by some real number M on this interval I, then

\|Rn(x)\|M(n+1)!\|xa\|n+1

for all x in the interval I.

We now state Taylor’s theorem, which provides the formal relationship between a function f

and its nth degree Taylor polynomial pn(x).

This theorem allows us to bound the error when using a Taylor polynomial to approximate a function value, and will be important in proving that a Taylor series for f

converges to f.

Taylor’s Theorem with Remainder

Let f

be a function that can be differentiated n+1

times on an interval I containing the real number a. Let pn be the nth Taylor polynomial of f

at a and let

Rn(x)=f(x)pn(x)

be the nth remainder. Then for each x in the interval I, there exists a real number c between a and x such that

Rn(x)=f(n+1)(c)(n+1)!(xa)n+1.

If there exists a real number M such that \|f(n+1)(x)\|M

for all xI,

then

\|Rn(x)\|M(n+1)!\|xa\|n+1

for all x in I.

Proof

Fix a point xI

and introduce the function g such that

g(t)=f(x)f(t)f(t)(xt)f(t)2!(xt)2f(n)(t)n!(xt)nRn(x)(xt)n+1(xa)n+1.

We claim that g satisfies the criteria of Rolle’s theorem. Since g is a polynomial function (in t), it is a differentiable function. Also, g is zero at t=a

and t=x

because

g(a)=f(x)f(a)f(a)(xa)f(a)2!(xa)2++f(n)(a)n!(xa)nRn(x)=f(x)pn(x)Rn(x)=0,g(x)=f(x)f(x)00=0.

Therefore, g satisfies Rolle’s theorem, and consequently, there exists c between a and x such that g(c)=0.

We now calculate g.

Using the product rule, we note that

ddt[f(n)(t)n!(xt)n]=f(n)(t)(n1)!(xt)n1+f(n+1)(t)n!(xt)n.

Consequently,

g(t)=f(t)+[f(t)f(t)(xt)]+[f(t)(xt)f(t)2!(xt)2]++[f(n)(t)(n1)!(xt)n1f(n+1)(t)n!(xt)n]+(n+1)Rn(x)(xt)n(xa)n+1.

Notice that there is a telescoping effect. Therefore,

g(t)=f(n+1)(t)n!(xt)n+(n+1)Rn(x)(xt)n(xa)n+1.

By Rolle’s theorem, we conclude that there exists a number c between a and x such that g(c)=0.

Since

g(c)=f(n+1)(c)n!(xc)n+(n+1)Rn(x)(xc)n(xa)n+1

we conclude that

f(n+1)(c)n!(xc)n+(n+1)Rn(x)(xc)n(xa)n+1=0.

Adding the first term on the left-hand side to both sides of the equation and dividing both sides of the equation by n+1,

we conclude that

Rn(x)=f(n+1)(c)(n+1)!(xa)n+1

as desired. From this fact, it follows that if there exists M such that \|f(n+1)(x)\|M

for all x in I, then

\|Rn(x)\|M(n+1)!\|xa\|n+1.

Not only does Taylor’s theorem allow us to prove that a Taylor series converges to a function, but it also allows us to estimate the accuracy of Taylor polynomials in approximating function values. We begin by looking at linear and quadratic approximations of f(x)=x3

at x=8

and determine how accurate these approximations are at estimating 113.

Using Linear and Quadratic Approximations to Estimate Function Values

Consider the function f(x)=x3.

  1. Find the first and second Taylor polynomials for f

    at

    x=8.

    Use a graphing utility to compare these polynomials with

    f

    near

    x=8.
  2. Use these two polynomials to estimate 113.
  3. Use Taylor’s theorem to bound the error.
  1. For f(x)=x3,

    the values of the function and its first two derivatives at

    x=8

    are as follows:


    f(x)=x3f(8)=2f(x)=13x2/3f(8)=112f(x)=−29x5/3f(8)=1144.

    Thus, the first and second Taylor polynomials at

    x=8

    are given by


    p1(x)=f(8)+f(8)(x8)=2+112(x8)p2(x)=f(8)+f(8)(x8)+f(8)2!(x8)2=2+112(x8)1288(x8)2.

    The function and the Taylor polynomials are shown in [link].


    This graph has four curves. The first is the function f(x)=cube root of x. The second function is psub1(x). The third is psub2(x). The curves are very close around x=8.

  2. Using the first Taylor polynomial at x=8,

    we can estimate


    113p1(11)=2+112(118)=2.25.

    Using the second Taylor polynomial at

    x=8,

    we obtain


    113p2(11)=2+112(118)1288(118)2=2.21875.
  3. By [link], there exists a c in the interval (8,11)

    such that the remainder when approximating

    113

    by the first Taylor polynomial satisfies


    R1(11)=f(c)2!(118)2.

    We do not know the exact value of c, so we find an upper bound on

    R1(11)

    by determining the maximum value of

    f

    on the interval

    (8,11).

    Since

    f(x)=29x5/3,

    the largest value for

    \|f(x)\|

    on that interval occurs at

    x=8.

    Using the fact that

    f(8)=1144,

    we obtain


    \|R1(11)\|1144·2!(118)2=0.03125.

    Similarly, to estimate

    R2(11),

    we use the fact that


    R2(11)=f(c)3!(118)3.

    Since

    f(x)=1027x8/3,

    the maximum value of

    f

    on the interval

    (8,11)

    is

    f(8)0.0014468.

    Therefore, we have


    \|R2(11)\|0.00114683!(118)30.0065104.

Find the first and second Taylor polynomials for f(x)=x

at x=4.

Use these polynomials to estimate 6.

Use Taylor’s theorem to bound the error.


p1(x)=2+14(x4);p2(x)=2+14(x4)164(x4)2;p1(6)=2.5;p2(6)=2.4375; \|R1(6)\|0.0625;\|R2(6)\|0.015625
Hint

Evaluate f(4),f(4),

and f(4).

Approximating sin *x* Using Maclaurin Polynomials

From [link]b., the Maclaurin polynomials for sinx

are given by

p2m+1(x)=p2m+2(x)=xx33!+x55!x77!++(−1)mx2m+1(2m+1)!

for m=0,1,2,.

  1. Use the fifth Maclaurin polynomial for sinx

    to approximate

    sin(π18)

    and bound the error.

  2. For what values of x does the fifth Maclaurin polynomial approximate sinx

    to within 0.0001?

  1. The fifth Maclaurin polynomial is
    p5(x)=xx33!+x55!.

    Using this polynomial, we can estimate as follows:


    sin(π18)p5(π18)=π1813!(π18)3+15!(π18)50.173648.

    To estimate the error, use the fact that the sixth Maclaurin polynomial is

    p6(x)=p5(x)

    and calculate a bound on

    R6(π18).

    By [link], the remainder is


    R6(π18)=f(7)(c)7!(π18)7

    for some c between 0 and

    π18.

    Using the fact that

    \|f(7)(x)\|1

    for all x, we find that the magnitude of the error is at most


    17!·(π18)79.8×10−10.
  2. We need to find the values of x such that
    17!\|x\|70.0001.

    Solving this inequality for x, we have that the fifth Maclaurin polynomial gives an estimate to within 0.0001 as long as

    \|x\|<0.907.

Use the fourth Maclaurin polynomial for cosx

to approximate cos(π12).

0.96593

Hint

The fourth Maclaurin polynomial is p4(x)=1x22!+x44!.

Now that we are able to bound the remainder Rn(x),

we can use this bound to prove that a Taylor series for f

at a converges to f.

Representing Functions with Taylor and Maclaurin Series

We now discuss issues of convergence for Taylor series. We begin by showing how to find a Taylor series for a function, and how to find its interval of convergence.

Finding a Taylor Series

Find the Taylor series for f(x)=1x

at x=1.

Determine the interval of convergence.

For f(x)=1x,

the values of the function and its first four derivatives at x=1

are

f(x)=1xf(1)=1f(x)=1x2f(1)=−1f(x)=2x3f(1)=2!f(x)=3·2x4f(1)=−3!f(4)(x)=4·3·2x5f(4)(1)=4!.

That is, we have f(n)(1)=(−1)nn!

for all n0.

Therefore, the Taylor series for f

at x=1

is given by

n=0f(n)(1)n!(x1)n=n=0(−1)n(x1)n.

To find the interval of convergence, we use the ratio test. We find that

\|an+1\|\|an\|=\|(−1)n+1(x1)n+1\|\|(−1)n(x1)n\|=\|x1\|.

Thus, the series converges if \|x1\|<1.

That is, the series converges for 0<x<2.

Next, we need to check the endpoints. At x=2,

we see that

n=0(−1)n(21)n=n=0(−1)n

diverges by the divergence test. Similarly, at x=0,

n=0(−1)n(01)n=n=0(−1)2n=n=01

diverges. Therefore, the interval of convergence is (0,2).

Find the Taylor series for f(x)=12x

at x=2

and determine its interval of convergence.

n=0(2x2n+2 )n.

The interval of convergence is (0,4).

Hint
f(n)(2)=(−1)nn!2n+1

We know that the Taylor series found in this example converges on the interval (0,2),

but how do we know it actually converges to f?

We consider this question in more generality in a moment, but for this example, we can answer this question by writing

f(x)=1x=11(1x).

That is, f

can be represented by the geometric series n=0(1x)n.

Since this is a geometric series, it converges to 1x

as long as \|1x\|<1.

Therefore, the Taylor series found in [link] does converge to f(x)=1x

on (0,2).

We now consider the more general question: if a Taylor series for a function f

converges on some interval, how can we determine if it actually converges to f?

To answer this question, recall that a series converges to a particular value if and only if its sequence of partial sums converges to that value. Given a Taylor series for f

at a, the nth partial sum is given by the nth Taylor polynomial pn. Therefore, to determine if the Taylor series converges to f,

we need to determine whether

limnpn(x)=f(x).

Since the remainder Rn(x)=f(x)pn(x),

the Taylor series converges to f

if and only if

limnRn(x)=0.

We now state this theorem formally.

Convergence of Taylor Series

Suppose that f

has derivatives of all orders on an interval I containing a. Then the Taylor series

n=0f(n)(a)n!(xa)n

converges to f(x)

for all x in I if and only if

limnRn(x)=0

for all x in I.

With this theorem, we can prove that a Taylor series for f

at a converges to f

if we can prove that the remainder Rn(x)0.

To prove that Rn(x)0,

we typically use the bound

\|Rn(x)\|M(n+1)!\|xa\|n+1

from Taylor’s theorem with remainder.

In the next example, we find the Maclaurin series for ex and sinx

and show that these series converge to the corresponding functions for all real numbers by proving that the remainders Rn(x)0

for all real numbers x.

Finding Maclaurin Series

For each of the following functions, find the Maclaurin series and its interval of convergence. Use [link] to prove that the Maclaurin series for f

converges to f

on that interval.

  1. ex
  2. sinx
  1. Using the nth Maclaurin polynomial for ex found in [link]a., we find that the Maclaurin series for ex is given by
    n=0xnn!.

    To determine the interval of convergence, we use the ratio test. Since


    \|an+1\|\|an\|=\|x\|n+1(n+1)!·n!\|x\|n=\|x\|n+1,

    we have


    limn\|an+1\|\|an\|=limn\|x\|n+1=0

    for all x. Therefore, the series converges absolutely for all x, and thus, the interval of convergence is

    (,).

    To show that the series converges to ex for all x, we use the fact that

    f(n)(x)=ex

    for all

    n0

    and ex is an increasing function on

    (,).

    Therefore, for any real number b, the maximum value of ex for all

    \|x\|b

    is eb. Thus,


    \|Rn(x)\|eb(n+1)!\|x\|n+1.

    Since we just showed that


    n=0\|x\|nn!

    converges for all x, by the divergence test, we know that


    limn\|x\|n+1(n+1)!=0

    for any real number x. By combining this fact with the squeeze theorem, the result is

    limnRn(x)=0.
  2. Using the nth Maclaurin polynomial for sinx

    found in [link]b., we find that the Maclaurin series for

    sinx

    is given by


    n=0(−1)nx2n+1(2n+1)!.

    In order to apply the ratio test, consider


    \|an+1\|\|an\|=\|x\|2n+3(2n+3)!·(2n+1)!\|x\|2n+1=\|x\|2(2n+3)(2n+2).

    Since


    limn\|x\|2(2n+3)(2n+2)=0

    for all x, we obtain the interval of convergence as

    (,).

    To show that the Maclaurin series converges to

    sinx,

    look at

    Rn(x).

    For each x there exists a real number c between 0 and x such that


    Rn(x)=f(n+1)(c)(n+1)!xn+1.

    Since

    \|f(n+1)(c)\|1

    for all integers n and all real numbers c, we have


    \|Rn(x)\|\|x\|n+1(n+1)!

    for all real numbers x. Using the same idea as in part a., the result is

    limnRn(x)=0

    for all x, and therefore, the Maclaurin series for

    sinx

    converges to

    sinx

    for all real x.

Find the Maclaurin series for f(x)=cosx.

Use the ratio test to show that the interval of convergence is (,).

Show that the Maclaurin series converges to cosx

for all real numbers x.

n=0(−1)nx2n(2n)!

By the ratio test, the interval of convergence is (,).

Since \|Rn(x)\|\|x\|n+1(n+1)!,

the series converges to cosx

for all real x.

Hint

Use the Maclaurin polynomials for cosx.

Proving that *e* is Irrational

In this project, we use the Maclaurin polynomials for ex to prove that e is irrational. The proof relies on supposing that e is rational and arriving at a contradiction. Therefore, in the following steps, we suppose e=r/s

for some integers r and s where s0.

  1. Write the Maclaurin polynomials p0(x),p1(x),p2(x),p3(x),p4(x)

    for ex. Evaluate

    p0(1),p1(1),p2(1),p3(1),p4(1)

    to estimate e.

  2. Let Rn(x)

    denote the remainder when using

    pn(x)

    to estimate ex. Therefore,

    Rn(x)=expn(x),

    and

    Rn(1)=epn(1).

    Assuming that

    e=rs

    for integers r and s, evaluate

    R0(1),R1(1),R2(1),R3(1),R4(1).
  3. Using the results from part 2, show that for each remainder R0(1),R1(1),R2(1),R3(1),R4(1),

    we can find an integer k such that

    kRn(1)

    is an integer for

    n=0,1,2,3,4.
  4. Write down the formula for the nth Maclaurin polynomial pn(x)

    for ex and the corresponding remainder

    Rn(x).

    Show that

    sn!Rn(1)

    is an integer.

  5. Use Taylor’s theorem to write down an explicit formula for Rn(1).

    Conclude that

    Rn(1)0,

    and therefore,

    sn!Rn(1)0.
  6. Use Taylor’s theorem to find an estimate on Rn(1).

    Use this estimate combined with the result from part 5 to show that

    \|sn!Rn(1)\|<sen+1.

    Conclude that if n is large enough, then

    \|sn!Rn(1)\|<1.

    Therefore,

    sn!Rn(1)

    is an integer with magnitude less than 1. Thus,

    sn!Rn(1)=0.

    But from part 5, we know that

    sn!Rn(1)0.

    We have arrived at a contradiction, and consequently, the original supposition that e is rational must be false.

Key Concepts

Key Equations


n=0f(n)(a)n!(xa)n=f(a)+f(a)(xa)+f(a)2!(xa)2++f(n)(a)n!(xa)n+

In the following exercises, find the Taylor polynomials of degree two approximating the given function centered at the given point.

f(x)=1+x+x2

at a=1

f(x)=1+x+x2

at a=−1

f(−1)=1;f(−1)=−1;f(−1)=2;f(x)=1(x+1)+(x+1)2
f(x)=cos(2x)

at a=π

f(x)=sin(2x)

at a=π2

f(x)=2cos(2x);f(x)=−4sin(2x);p2(x)=−2(xπ2)
f(x)=x

at a=4

f(x)=lnx

at a=1

f(x)=1x;f(x)=1x2;p2(x)=0+(x1)12(x1)2
f(x)=1x

at a=1

f(x)=ex

at a=1

p2(x)=e+e(x1)+e2(x1)2

In the following exercises, verify that the given choice of n in the remainder estimate \|Rn\|M(n+1)!(xa)n+1,

where M is the maximum value of \|f(n+1)(z)\|

on the interval between a and the indicated point, yields \|Rn\|11000.

Find the value of the Taylor polynomial pn of f

at the indicated point.

[T] 10;a=9,n=3

[T] (28)1/3;a=27,n=1

d2dx2x1/3=29x5/3−0.00092

when x28

so the remainder estimate applies to the linear approximation x1/3p1(27)=3+x2727,

which gives (28)1/33+127=3.037¯,

while (28)1/33.03658.

[T] sin(6);a=2π,n=5

[T] e2; a=0,n=9

Using the estimate 21010!<0.000283

we can use the Taylor expansion of order 9 to estimate ex at x=2.

as e2p9(2)=1+2+222+236++299!=7.3887

whereas e27.3891.

[T] cos(π5);a=0,n=4

[T] ln(2);a=1,n=1000

Since dndxn(lnx)=(−1)n1(n1)!xn,R100011001.

One has p1000(1)=n=11000(−1)n1n0.6936

whereas ln(2)0.6931.

Integrate the approximation sinttt36+t5120t75040

evaluated at πt to approximate 01sinπtπtdt.

Integrate the approximation ex1+x+x22++x6720

evaluated at −x2 to approximate 01ex2dx.

01(1x2+x42x66+x824x10120+x12720)dx =1133+15101742+199·24111120·11+113720·130.74683

whereas 01ex2dx0.74682.

In the following exercises, find the smallest value of n such that the remainder estimate \|Rn\|M(n+1)!(xa)n+1,

where M is the maximum value of \|f(n+1)(z)\|

on the interval between a and the indicated point, yields \|Rn\|11000

on the indicated interval.

f(x)=sinx

on [π,π],a=0

f(x)=cosx

on [π2,π2],a=0

Since f(n+1)(z)

is sinz

or cosz,

we have M=1.

Since \|x0\|π2,

we seek the smallest n such that πn+12n+1(n+1)!0.001.

The smallest such value is n=7.

The remainder estimate is R70.00092.

f(x)=e−2x

on [−1,1],a=0

f(x)=ex

on [−3,3],a=0

Since f(n+1)(z)=±ez

one has M=e3.

Since \|x0\|3,

one seeks the smallest n such that 3n+1e3(n+1)!0.001.

The smallest such value is n=14.

The remainder estimate is R140.000220.

In the following exercises, the maximum of the right-hand side of the remainder estimate \|R1\|max\|f(z)\|2R2

on [aR,a+R]

occurs at a or a±R.

Estimate the maximum value of R such that max\|f(z)\|2R20.1

on [aR,a+R]

by plotting this maximum as a function of R.

[T] ex approximated by 1+x,a=0

[T] sinx

approximated by x, a=0


This graph has a horizontal line at y=0.2. It also has a curve starting at the origin and concave up. The curve and the line intersect at the ordered pair (0.5966, 0.2).


Since sinx

is increasing for small x and since sinx=sinx,

the estimate applies whenever R2sin(R)0.2,

which applies up to R=0.596.

[T] lnx

approximated by x1,a=1

[T] cosx

approximated by 1,a=0


This graph has a horizontal line at y=0.2. It also has a curve starting at the origin and concave up. The curve and the line intersect at the ordered pair (0.44720, 0.2).


Since the second derivative of cosx

is cosx

and since cosx

is decreasing away from x=0,

the estimate applies when R2cosR0.2

or R0.447.

In the following exercises, find the Taylor series of the given function centered at the indicated point.

x4

at a=−1

1+x+x2+x3

at a=−1

(x+1)32(x+1)2+2(x+1)
sinx

at a=π

cosx

at a=2π

Values of derivatives are the same as for x=0

so cosx=n=0(−1)n(x2π)2n(2n)!

sinx

at x=π2

cosx

at x=π2

cos(π2)=0,sin(π2)=−1

so cosx=n=0(−1)n+1(xπ2)2n+1(2n+1)!,

which is also cos(xπ2).

ex

at a=−1

ex

at a=1

The derivatives are f(n)(1)=e

so ex=en=0(x1)nn!.

1(x1)2

at a=0

(Hint: Differentiate 11x.)

1(x1)3

at a=0

1(x1)3=(12)d2dx211x=n=0((n+2)(n+1)xn2)
F(x)=0xcos(t)dt;f(t)=n=0(−1)ntn(2n)!

at a=0

(Note: f

is the Taylor series of cos(t).)

In the following exercises, compute the Taylor series of each function around x=1.

f(x)=2x
2x=1(x1)
f(x)=x3
f(x)=(x2)2
((x1)1)2=(x1)22(x1)+1
f(x)=lnx
f(x)=1x
11(1x)=n=0(−1)n(x1)n
f(x)=12xx2
f(x)=x4x2x21
xn=02n(1x)2n=n=02n(x1)2n+1+n=02n(x1)2n
f(x)=ex
f(x)=e2x
e2x=e2(x1)+2=e2n=02n(x1)nn!

[T] In the following exercises, identify the value of x such that the given series n=0an

is the value of the Maclaurin series of f(x)

at x.

Approximate the value of f(x)

using S10=n=010an.

n=01n!
n=02nn!
x=e2;S10=34,91347257.3889947
n=0(−1)n(2π)2n(2n)!
n=0(−1)n(2π)2n+1(2n+1)!
sin(2π)=0;S10=8.27×10−5

The following exercises make use of the functions S5(x)=xx36+x5120

and C4(x)=1x22+x424

on [π,π].

[T] Plot sin2x(S5(x))2

on [π,π].

Compare the maximum difference with the square of the Taylor remainder estimate for sinx.

[T] Plot cos2x(C4(x))2

on [π,π].

Compare the maximum difference with the square of the Taylor remainder estimate for cosx.


This graph has a concave up curve that is symmetrical about the y axis. The lowest point of the graph is the origin with the rest of the curve above the x-axis.


The difference is small on the interior of the interval but approaches 1

near the endpoints. The remainder estimate is \|R4\|=π51202.552.

[T] Plot \|2S5(x)C4(x)sin(2x)\|

on [π,π].

[T] Compare S5(x)C4(x)

on [−1,1]

to tanx.

Compare this with the Taylor remainder estimate for the approximation of tanx

by x+x33+2x515.


This graph has two curves. The solid curve is very flat and close to the x-axis. It passes through the origin. The second curve, a broken line, is concave down and symmetrical about the y-axis. It is very close to the x-axis between -3 and 3.


The difference is on the order of 10−4

on [−1,1]

while the Taylor approximation error is around 0.1

near ±1.

The top curve is a plot of tan2x(S5(x)C4(x))2

and the lower dashed plot shows t2(S5C4)2.

[T] Plot exe4(x)

where e4(x)=1+x+x22+x36+x424

on [0,2].

Compare the maximum error with the Taylor remainder estimate.

(Taylor approximations and root finding.) Recall that Newton’s method xn+1=xnf(xn)f(xn)

approximates solutions of f(x)=0

near the input x0.

  1. If f

    and

    g

    are inverse functions, explain why a solution of

    g(x)=a

    is the value

    f(a)off.
  2. Let pN(x)

    be the

    Nth

    degree Maclaurin polynomial of

    ex.

    Use Newton’s method to approximate solutions of

    pN(x)2=0

    for

    N=4,5,6.
  3. Explain why the approximate roots of pN(x)2=0

    are approximate values of

    ln(2).

a. Answers will vary. b. The following are the xn

values after 10

iterations of Newton’s method to approximation a root of pN(x)2=0:

for N=4,x=0.6939...;

for N=5,x=0.6932...;

for N=6,x=0.69315...;.

(Note: ln(2)=0.69314...)

c. Answers will vary.

In the following exercises, use the fact that if q(x)=n=1an(xc)n

converges in an interval containing c,

then limxcq(x)=a0

to evaluate each limit using Taylor series.

limx0cosx1x2
limx0ln(1x2)x2
ln(1x2)x21
limx0ex2x21x4
limx0+cos(x)12x
cos(x)12x(1x2+x24!)12x14

Glossary

Maclaurin polynomial
a Taylor polynomial centered at 0; the nth Taylor polynomial for f

at 0 is the nth Maclaurin polynomial for

f
Maclaurin series
a Taylor series for a function f

at

x=0

is known as a Maclaurin series for

f
Taylor polynomials
the nth Taylor polynomial for f

at

x=a

is

pn(x)=f(a)+f(a)(xa)+f(a)2!(xa)2++f(n)(a)n!(xa)n
Taylor series
a power series at a that converges to a function f

on some open interval containing a

Taylor’s theorem with remainder
for a function f

and the nth Taylor polynomial for

f

at

x=a,

the remainder

Rn(x)=f(x)pn(x)

satisfies

Rn(x)=f(n+1)(c)(n+1)!(xa)n+1

for some c between x and a; if there exists an interval I containing a and a real number M such that

\|f(n+1)(x)\|M

for all x in I, then

\|Rn(x)\|M(n+1)!\|xa\|n+1

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