Overview
Integrating vector-valued functions works component by component. Each component gets integrated separately using standard integration techniques.
General form:
∫⟨f(t),g(t)⟩dt=⟨∫f(t)dt,∫g(t)dt⟩
Indefinite Integrals with Initial Conditions
When you’re finding
r(t) from
r′(t), integrate each component and then use the initial conditions to solve for the constants.
Example 1: Exponential Components
Given: r′(t)=⟨6e3t,4e2t⟩ and
r(0)=⟨3,2⟩ Integrate the x-component: x(t)=∫6e3tdtThis needs
u-substitution, since we have
3t in the exponent. Let
u=3t, so
du=3dt, meaning
dt=3du:
x(t)=∫6eu⋅3du=∫2eudu=2eu+c1=2e3t+c1Integrate the y-component: y(t)=∫4e2tdtLet
u=2t, so
du=2dt, meaning
dt=2du:
y(t)=∫4eu⋅2du=∫2eudu=2eu+c2=2e2t+c2Apply the initial conditions r(0)=⟨3,2⟩:
For the
x-component:
3=2e3(0)+c1=2(1)+c1=2+c1, so
c1=1For the
y-component:
2=2e2(0)+c2=2(1)+c2=2+c2, so
c2=0Final answer:
r(t)=⟨2e3t+1,2e2t⟩
Indefinite Integrals Without Initial Conditions
When no initial condition is given, the constants of integration just stay in the answer.
Example 2: Trig and Inverse Trig Integrals
Find
∫⟨sec2(t),1+t21⟩dtIntegrate the x-component: x(t)=∫sec2(t)dt=tan(t)+c1Integrate the y-component, recognizing the inverse tangent derivative:
y(t)=∫1+t21dt=arctan(t)+c2Final answer:
r(t)=⟨tan(t)+c1,arctan(t)+c2⟩
Definite Integrals
For definite integrals, evaluate each component separately over the given interval.
General form:
∫ab⟨f(t),g(t)⟩dt=⟨∫abf(t)dt,∫abg(t)dt⟩Example 3: Polynomial Components
Evaluate
∫−22⟨t2,t4⟩dt ∫−22t2dt=[3t3]−22=38−3−8=38+38=316∫−22t4dt=[5t5]−22=532−5−32=532+532=564Final answer:
⟨316,564⟩Example 4: Fractional Exponents
Evaluate
∫−11⟨t3,t1/5⟩dt ∫−11t3dt=[4t4]−11=41−41=0∫−11t1/5dt=[6/5t6/5]−11=[65t6/5]−11=65(1)−65(1)=0Note that
(−1)6/5=[(−1)1/5]6=(−1)6=1, since the even power makes it positive.
Final answer:
⟨0,0⟩
Parametric Form
The same methods work when the rates come as two separate equations,
dtdx and
dtdy, instead of one vector. Integrate each one, then use the starting point to find each constant.
Example 5: Parametric Initial Value Problem
Given: dtdx=3t2−2 and
dtdy=t+11 for
t≥0, and the particle is at
(1,4) when
t=0. Find
x(t) and
y(t).
x(t)=∫(3t2−2)dt=t3−2t+c1Since
x(0)=1:
1=0−0+c1, so
c1=1 y(t)=∫t+11dt=ln(t+1)+c2No absolute value is needed, since
t+1>0 for
t≥0. Since
y(0)=4:
4=ln(1)+c2=0+c2, so
c2=4Final answer:
x(t)=t3−2t+1y(t)=ln(t+1)+4Example 6: No Antiderivative You Can Find
Some rates, like
sin(t2), don’t have an antiderivative you can write down. Then skip the general solution and use the Fundamental Theorem of Calculus with the starting value:
x(b)=x(a)+∫abdtdxdty(b)=y(a)+∫abdtdydtGiven: dtdy=sin(t2) and
y(0)=1. Find
y(2).
y(2)=1+∫02sin(t2)dt≈1+0.805=1.805The integral is done on a calculator. AP free-response questions about particle motion use this setup a lot (more in Topic 9.6).
Important Notes
Constants of integration:
- Each component gets its own constant:
c1,
c2, and so on
- These constants are generally different values
- Use the initial conditions to solve for each one separately
Common integration techniques you’ll need:
-
u-substitution for chain rule cases
- Recognizing inverse trig derivatives
- The power rule for polynomials
- Exponential function integration
Symmetry in definite integrals:
- Odd functions over symmetric intervals
[−a,a] integrate to zero
- Even functions over symmetric intervals may not cancel
Key Takeaways
- Component-wise integration: ∫⟨f(t),g(t)⟩dt=⟨∫f(t)dt,∫g(t)dt⟩
- Each component integrates independently using standard calculus techniques
- The constants of integration are different for each component: c1, c2, and so on
- Initial conditions r(t0)=⟨x0,y0⟩ give you separate equations for each constant
- u-substitution is required when there’s a chain rule involved, like with e3t
- Recognize the inverse trig derivatives: ∫1+t21dt=arctan(t)+C
- Definite integrals: evaluate each component over [a,b] and combine the results
- Parametric form works the same way: integrate dtdx and dtdy separately. If you can’t find an antiderivative, use x(b)=x(a)+∫abdtdxdt (and the same for y)