Flux across hemispheres and paraboloids Let S be the hemispherex2 + y2 + z2 = a2, for z ≥ 0, and let T be the paraboloid z = a - (x2 + y2)/a, for z ≥ 0, where a > 0. Assume the surfaces have outward normal vectors.a. Verify that S and T have the same base (x2 + y2 ≤ a2) and thesame high point (0, 0, a).b. Which surface has the greater area?c. Show that the flux of the radial field F = ⟨x, y, z⟩ across S is 2πa3.d. Show that the flux of the radial field F = ⟨x, y, z⟩ across T is 3πa3/2.

Algebra & Trigonometry with Analytic Geometry
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ISBN:9781133382119
Author:Swokowski
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Chapter8: Applications Of Trigonometry
Section8.3: Vectors
Problem 60E
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Flux across hemispheres and paraboloids Let S be the hemisphere
x2 + y2 + z2 = a2, for z ≥ 0, and let T be the paraboloid z = a - (x2 + y2)/a, for z ≥ 0, where a > 0. Assume the surfaces have outward normal vectors.
a. Verify that S and T have the same base (x2 + y2a2) and the
same high point (0, 0, a).
b. Which surface has the greater area?
c. Show that the flux of the radial field F = ⟨x, y, z⟩ across S is 2πa3.
d. Show that the flux of the radial field F = ⟨x, y, z⟩ across T is 3πa3/2.

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Step 1

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Given:

The equation of the hemisphere is x2 + y2 + z2 = a2, for z  0 and 

The  equation of the paraboloid is z = a - (x2 + y2)a, for z  0, where a > 0.

 

Flux across hemispheres and paraboloids:

The flux across a surface is a measure of the flow of a vector field through the surface. The flux across hemispheres and paraboloids can be found using the divergence theorem or by direct computation using surface integrals.

  1. Flux across a hemisphere:

Consider a hemisphere with the radius R centred at the origin. The unit outward normal vector to the hemisphere is given by n = (x, y, z)R. The flux of a vector field F = (F1, F2, F3) across the hemisphere is given by:

flux = F · n dS

Where the integral is taken over the surface of the hemisphere. Using spherical coordinates, the surface element can be expressed as dS=R2sinθdθdφ, and the unit outward normal vector is given by n = (sin θ cos φ, sin θ sin φ, cos θ). Thus, the flux can be shown as:

flux =02π0πF·nR2sinθdθdφ

To evaluate the integral, we need to express the vector field F in terms of spherical coordinates. For example, if F=(x2,y2,z2), then F·n=(x3+y3+z3)R3. Substituting this expression in the above integral and evaluating the integrals gives the flux across the hemisphere.

  1. Flux across a paraboloid:

Consider a paraboloid of revolution z=x2+y2, bounded by a circle of radius R in the xy-plane. The unit outward normal vector to the paraboloid is given by n=(2x,2y,-1)(1+4x2+4y2). The flux of a vector field F = (F1, F2, F3) across the paraboloid is given by:

flux = F · n dS

Where the integral is taken over the surface of the paraboloid. Using cylindrical coordinates, the surface element can be expressed as dS=(1+r2)rdrdθ, and the unit outward normal vector is given by n=(2rcosθ,2rsinθ,-1)(1+4r2). Thus, the flux can be shown as:

flux =0R02πF·n(1+r2)rdrdθ

To evaluate the integral, we need to express the vector field F in terms of cylindrical coordinates. For example, suppose F = (x, y, z), then F·n=-z(1+4r2). Substituting this expression in the above integral and evaluating the integrals gives the flux across the paraboloid.

Step 2

a. To verify that S and T have the same base and high point, we can set z = a in the equation of the hemisphere and in the equation of the paraboloid and then solve for x and y. We have:

For the hemisphere:

x2+y2+a2=a2, which simplifies to x2+y2=0. This means that the base of the hemisphere is the point (0, 0) and the high point is (0, 0, a).

For the paraboloid:

z=a-(x2+y2)a=a-r2a, where r2=x2+y2. Setting z = a gives, which is the equation of a circle of radius a in the xy-plane. Therefore, the base of the paraboloid is the circle x2+y2=a2 and the high point is (0, 0, a).

Thus, S and T have the same base (the circle x2+y2=a2) and the same high point (0, 0, a).

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