Double Integrals in Polar - Calculus 3

  1. A double integral in Cartesian coordinates has the form ∫0a∫0a2−x2g(x2+y2) dy dx\int_0^a \int_0^{\sqrt{a^2-x^2}} g(x^2+y^2) \, dy \, dx where a>0a > 0. After converting to polar coordinates and evaluating, the result is π2∫0ar⋅g(r2) dr\frac{\pi}{2}\int_0^a r \cdot g(r^2) \, dr. What relationship must hold between the original integral and the converted form?
    Answer: The conversion is correct as stated, with no additional conditions needed When you encounter double integrals with limits involving expressions like a2−x2\sqrt{a^2-x^2}, you're looking at a region that's naturally suited for polar coordinates. The key insight is understanding what happens during the coordinate transformation. Let's trace through this conversion step by step. The original integral ∫0a∫0a2−x2g(x2+y2) dy dx\int_0^a \int_0^{\sqrt{a^2-x^2}} g(x^2+y^2) \, dy \, dx describes integration over a quarter-circle of radius aa in the first quadrant (since y=a2−x2y = \sqrt{a^2-x^2} is the upper half of x2+y2=a2x^2 + y^2 = a^2). In polar coordinates, this region becomes 0≤r≤a0 \leq r \leq a and 0≤θ≤π20 \leq \theta \leq \frac{\pi}{2}. The function g(x2+y2)g(x^2+y^2) naturally becomes g(r2)g(r^2), and we include the Jacobian rr. The integral becomes ∫0π/2∫0ag(r2)⋅r dr dθ\int_0^{\pi/2} \int_0^a g(r^2) \cdot r \, dr \, d\theta. Since g(r2)g(r^2) doesn't depend on θ\theta, we can factor out the θ\theta integration: ∫0π/2dθ∫0ar⋅g(r2) dr=π2∫0ar⋅g(r2) dr\int_0^{\pi/2} d\theta \int_0^a r \cdot g(r^2) \, dr = \frac{\pi}{2}\int_0^a r \cdot g(r^2) \, dr. Option A is wrong because g(x2+y2)g(x^2+y^2) being independent of θ\theta is automatic—it's a consequence of the function's form, not an additional requirement. Option B is incorrect because we need no special properties of g(u)g(u) beyond what's given. Option D is wrong because the factor π2\frac{\pi}{2} correctly accounts for the θ\theta integration. Study tip: When converting to polar coordinates, always check that your new limits match the original region's geometry, and remember that radially symmetric integrands automatically satisfy any θ\theta-independence requirements.
  2. A region RR is described in polar coordinates as {(r,θ):0≤θ≤π/2, θ≤r≤π−θ}\{(r,\theta) : 0 \leq \theta \leq \pi/2, \, \theta \leq r \leq \pi - \theta\}. When computing ∬Rr dA\iint_R r \, dA, what is the correct integral setup and what geometric shape does this region represent?
    Answer: ∫0π/2∫θπ−θr2 dr dθ\int_0^{\pi/2} \int_{\theta}^{\pi - \theta} r^2 \, dr \, d\theta; the region is bounded by two spirals When working with double integrals in polar coordinates, you need to carefully set up both the integral bounds and the differential area element. The key is remembering that dA=r dr dθdA = r \, dr \, d\theta in polar coordinates, so when integrating a function f(r,θ)f(r,\theta), you compute ∬Rf(r,θ)⋅r dr dθ\iint_R f(r,\theta) \cdot r \, dr \, d\theta. For the integral ∬Rr dA\iint_R r \, dA, you're integrating the function f(r,θ)=rf(r,\theta) = r. This becomes ∬Rr⋅r dr dθ=∬Rr2 dr dθ\iint_R r \cdot r \, dr \, d\theta = \iint_R r^2 \, dr \, d\theta. The bounds come directly from the region description: θ\theta ranges from 00 to π/2\pi/2, and for each θ\theta, rr ranges from θ\theta to π−θ\pi - \theta. This gives us ∫0π/2∫θπ−θr2 dr dθ\int_0^{\pi/2} \int_{\theta}^{\pi - \theta} r^2 \, dr \, d\theta. To understand the geometry, note that the boundaries are r=θr = \theta and r=π−θr = \pi - \theta. These aren't straight lines through the origin (which would have the form θ=constant\theta = \text{constant}), but rather curves where the radial distance depends on the angle. These are spiral-like curves that create a region between them. Answer choice A has the correct integral setup but misidentifies the geometric shape. Choice C correctly identifies the spiral boundaries but incorrectly uses rr instead of r2r^2 in the integrand, forgetting the rr factor from dAdA. Choice D has wrong θ\theta bounds and misidentifies the geometry. Study tip: Always remember that dA=r dr dθdA = r \, dr \, d\theta in polar coordinates, and distinguish between radial curves (r=g(θ)r = g(\theta)) and angular lines (θ=constant\theta = \text{constant}) when visualizing regions.
  3. The integral ∫02π∫13r2cos⁡(r) dr dθ\int_0^{2\pi} \int_1^{3} r^2 \cos(r) \, dr \, d\theta can be evaluated by recognizing that one part factors out. However, if the region of integration were changed to π6≤θ≤π3\frac{\pi}{6} \leq \theta \leq \frac{\pi}{3} and sec⁡θ≤r≤3\sec\theta \leq r \leq 3, what would be the new integral setup?
    Answer: ∫π/6π/3∫sec⁡θ3r2cos⁡(r) dr dθ\int_{\pi/6}^{\pi/3} \int_{\sec\theta}^3 r^2 \cos(r) \, dr \, d\theta When you encounter double integrals in polar coordinates, pay careful attention to how the region of integration is described and how it translates into integral bounds. The original integral uses a simple rectangular region in polar coordinates: rr goes from 1 to 3, and θ\theta goes from 0 to 2π2\pi. The new region has θ\theta bounded by π6≤θ≤π3\frac{\pi}{6} \leq \theta \leq \frac{\pi}{3} and rr bounded by sec⁡θ≤r≤3\sec\theta \leq r \leq 3. The key insight is recognizing that sec⁡θ=1cos⁡θ\sec\theta = \frac{1}{\cos\theta}, which represents the distance from the origin to a vertical line in Cartesian coordinates. When setting up the integral, you simply use the bounds as given: the outer integral has limits π6\frac{\pi}{6} to π3\frac{\pi}{3} for θ\theta, and the inner integral has limits sec⁡θ\sec\theta to 33 for rr. The integrand r2cos⁡(r)r^2\cos(r) remains unchanged because we're integrating over the same type of region, just with different boundaries. Looking at the wrong answers: (A) incorrectly uses cos⁡θ\cos\theta instead of sec⁡θ=1cos⁡θ\sec\theta = \frac{1}{\cos\theta}. (B) writes out 1cos⁡θ\frac{1}{\cos\theta} explicitly, which is mathematically equivalent to sec⁡θ\sec\theta but unnecessarily complicated. (D) incorrectly includes an extra cos⁡θ\cos\theta factor in the integrand, which would change the function being integrated entirely. Study tip: When converting between polar coordinate descriptions, remember that sec⁡θ=1cos⁡θ\sec\theta = \frac{1}{\cos\theta} and always preserve the original integrand unless you're changing coordinate systems entirely.
  4. A region RR in the first quadrant is bounded by y=xy = x, y=0y = 0, and x2+y2=4x^2 + y^2 = 4. When setting up ∬Rf(x,y) dA\iint_R f(x,y) \, dA in polar coordinates, which description correctly identifies the region's boundaries?
    Answer: 0≤θ≤π/40 \leq \theta \leq \pi/4 and 0≤r≤20 \leq r \leq 2 When converting double integrals to polar coordinates, you need to carefully analyze how each boundary curve translates from Cartesian to polar form, then determine the proper order of integration. Let's examine each boundary of region RR. The curve y=0y = 0 corresponds to the positive xx-axis, giving θ=0\theta = 0. The line y=xy = x has slope 1, so tan⁡θ=1\tan\theta = 1, which means θ=π/4\theta = \pi/4. The circle x2+y2=4x^2 + y^2 = 4 becomes r2=4r^2 = 4, or r=2r = 2. Since we're in the first quadrant bounded by these three curves, θ\theta ranges from 00 to π/4\pi/4, and rr extends from the origin (r=0r = 0) to the circle (r=2r = 2). Answer D correctly captures this: 0≤θ≤π/40 \leq \theta \leq \pi/4 and 0≤r≤20 \leq r \leq 2. Answer A incorrectly suggests rr starts at 2cos⁡θ+sin⁡θ\frac{2}{\cos\theta + \sin\theta} rather than 0. This expression would represent some inner boundary that doesn't exist in our region. Answer B limits rr to 2/cos⁡θ2/\cos\theta, which represents the vertical line x=2x = 2, not our actual boundary. Answer C extends θ\theta to π/2\pi/2, which would include the entire first quadrant rather than just the triangular sector below y=xy = x. Study tip: Always sketch the region first, then systematically convert each boundary curve to polar coordinates. Pay special attention to whether rr starts from the origin or from an inner boundary—this is a common source of errors in polar integration setup.
  5. The double integral ∫02∫04−x2xy dy dx\int_0^2 \int_0^{\sqrt{4-x^2}} xy \, dy \, dx is converted to polar coordinates. Which of the following represents the equivalent integral?
    Answer: ∫0π/2∫02r3cos⁡θsin⁡θ dr dθ\int_0^{\pi/2} \int_0^2 r^3 \cos\theta \sin\theta \, dr \, d\theta The region of integration is the first quadrant portion of the disk x2+y2≤4x^2 + y^2 \leq 4, so 0≤θ≤π/20 \leq \theta \leq \pi/2 and 0≤r≤20 \leq r \leq 2. Converting: x=rcos⁡θx = r\cos\theta, y=rsin⁡θy = r\sin\theta, dx dy=r dr dθdx\,dy = r\,dr\,d\theta. The integrand becomes xy⋅r=(rcos⁡θ)(rsin⁡θ)⋅r=r3cos⁡θsin⁡θxy \cdot r = (r\cos\theta)(r\sin\theta) \cdot r = r^3\cos\theta\sin\theta. Choice B forgets the Jacobian factor rr in the integrand. Choice C uses incorrect θ\theta-limits (should be π/2\pi/2, not π\pi). Choice D uses incorrect rr-limits (radius is 2, not 4).
  6. Consider the integral ∬Rex2+y2 dA\iint_R e^{x^2+y^2} \, dA where RR is the annular region 1≤x2+y2≤91 \leq x^2 + y^2 \leq 9. After converting to polar coordinates, the integral becomes ∫02π∫13rer2 dr dθ\int_0^{2\pi} \int_1^3 re^{r^2} \, dr \, d\theta. What is the value of this integral?
    Answer: π(e9−e)\pi(e^9 - e) The integral separates as ∫02πdθ∫13rer2 dr=2π∫13rer2 dr\int_0^{2\pi} d\theta \int_1^3 re^{r^2} \, dr = 2\pi \int_1^3 re^{r^2} \, dr. For the rr-integral, use substitution u=r2u = r^2, so du=2r drdu = 2r\,dr and r dr=12dur\,dr = \frac{1}{2}du. When r=1r = 1, u=1u = 1; when r=3r = 3, u=9u = 9. Thus ∫13rer2 dr=12∫19eu du=12(e9−e1)\int_1^3 re^{r^2} \, dr = \frac{1}{2}\int_1^9 e^u \, du = \frac{1}{2}(e^9 - e^1). The full integral is 2π⋅12(e9−e)=π(e9−e)2\pi \cdot \frac{1}{2}(e^9 - e) = \pi(e^9 - e). Choice B misses the 12\frac{1}{2} from substitution. Choice C incorrectly divides by 2. Choice D forgets the 2π2\pi factor.
  7. The integral ∫0π/3∫04cos⁡θr3sin⁡θ dr dθ\int_0^{\pi/3} \int_0^{4\cos\theta} r^3 \sin\theta \, dr \, d\theta represents the evaluation of ∬Ry⋅f(x,y) dA\iint_R y \cdot f(x,y) \, dA in polar coordinates for some function ff. What is f(x,y)f(x,y)?
    Answer: f(x,y)=x2+y2f(x,y) = x^2 + y^2 When converting double integrals from rectangular to polar coordinates, you need to recognize how the integrand transforms. The key is understanding that dA=dx dydA = dx \, dy becomes r dr dθr \, dr \, d\theta, and rectangular coordinates become x=rcos⁡θx = r\cos\theta and y=rsin⁡θy = r\sin\theta. Looking at the given integral ∫0π/3∫04cos⁡θr3sin⁡θ dr dθ\int_0^{\pi/3} \int_0^{4\cos\theta} r^3 \sin\theta \, dr \, d\theta, you can identify the components. The integrand is r3sin⁡θr^3 \sin\theta, which includes the required rr from the area element r dr dθr \, dr \, d\theta. This means the actual function being integrated is r2sin⁡θ⋅yr^2 \sin\theta \cdot y, where the yy factor comes from the problem statement saying we're evaluating ∬Ry⋅f(x,y) dA\iint_R y \cdot f(x,y) \, dA. Since y=rsin⁡θy = r\sin\theta and we have r2sin⁡θr^2 \sin\theta remaining after accounting for the yy factor and area element, we get r2=x2+y2r^2 = x^2 + y^2. Therefore, f(x,y)=x2+y2f(x,y) = x^2 + y^2. Answer choice A, f(x,y)=(x2+y2)3/2/yf(x,y) = (x^2 + y^2)^{3/2}/y, would give r3/sin⁡θr^3/\sin\theta in polar form, which doesn't match. Answer B, f(x,y)=x2+y2f(x,y) = \sqrt{x^2 + y^2}, converts to just rr, missing the r2r^2 we need. Answer C, f(x,y)=x2+y2−yf(x,y) = x^2 + y^2 - y, would produce r2−rsin⁡θr^2 - r\sin\theta, which is more complex than our integrand. Study tip: When working backwards from polar integrals, always separate out the rr from dAdA first, then convert the remaining expression using r2=x2+y2r^2 = x^2 + y^2 and the basic polar relationships.
  8. Consider evaluating ∬R(x2−y2) dA\iint_R (x^2 - y^2) \, dA over the region RR bounded by r=2+cos⁡θr = 2 + \cos\theta. In polar coordinates, the integrand x2−y2x^2 - y^2 becomes r2cos⁡(2θ)r^2\cos(2\theta). What is the complete setup for this integral?
    Answer: ∫02π∫02+cos⁡θr3cos⁡(2θ) dr dθ\int_0^{2\pi} \int_0^{2+\cos\theta} r^3 \cos(2\theta) \, dr \, d\theta When converting double integrals from Cartesian to polar coordinates, you need to handle three key components: the integrand transformation, the region bounds, and the crucial Jacobian factor. The integrand x2−y2x^2 - y^2 correctly transforms to r2cos⁡(2θ)r^2\cos(2\theta) using the identity x2−y2=r2(cos⁡2θ−sin⁡2θ)=r2cos⁡(2θ)x^2 - y^2 = r^2(\cos^2\theta - \sin^2\theta) = r^2\cos(2\theta). The region r=2+cos⁡θr = 2 + \cos\theta is a limaçon that completes one full loop as θ\theta goes from 00 to 2π2\pi, with rr ranging from 00 to 2+cos⁡θ2 + \cos\theta. The critical insight is the Jacobian factor. When converting dA=dx dydA = dx \, dy to polar coordinates, you must include rr in the area element: dA=r dr dθdA = r \, dr \, d\theta. This transforms our integrand from r2cos⁡(2θ)r^2\cos(2\theta) to r2cos⁡(2θ)⋅r=r3cos⁡(2θ)r^2\cos(2\theta) \cdot r = r^3\cos(2\theta), making the complete integral ∫02π∫02+cos⁡θr3cos⁡(2θ) dr dθ\int_0^{2\pi} \int_0^{2+\cos\theta} r^3 \cos(2\theta) \, dr \, d\theta. Choice A omits the Jacobian factor, keeping only r2cos⁡(2θ)r^2\cos(2\theta) instead of r3cos⁡(2θ)r^3\cos(2\theta). Choice C uses the correct integrand but wrong θ\theta bounds—00 to π\pi would give only half the limaçon. Choice D has the wrong trigonometric function, using sin⁡(2θ)\sin(2\theta) instead of cos⁡(2θ)\cos(2\theta). Study tip: Always remember the Jacobian! In polar coordinates, dAdA becomes r dr dθr \, dr \, d\theta, which adds an extra factor of rr to your integrand. This is the most commonly missed step in polar coordinate conversions.

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