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Calculus Level 3

A vector field is defined as follows

F = z 2 x i ^ + ( y 3 3 + sin z ) j ^ + ( x 2 z + y 2 ) k ^ {\vec{\textbf{F}}}= z^{2} x \hat{\textbf{i}} + \left(\frac{y^{3}}{3} +\sin z \right) \hat{\textbf{j}} +\left(x^{2} z +y^{2}\right) \hat{\textbf{k}} .

If the flux of this field through the top half of the sphere , x 2 + y 2 + z 2 = 4 x^{2} +y^{2} +z^{2} =4 , can be written as A π B \frac{A \pi}{B} , where A A and B B are co-prime integers find A+B

Note: the surface in question is not a closed one.

use positive orientation


The answer is 89.

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1 solution

Steven Chase
Dec 20, 2019

Nice to see some vector calc problems being posted. I will use the divergence theorem.

V ( F ) d V = S ( F n ) d S \int \int \int_V (\nabla \cdot \vec{F}) \, dV = \int \int_S (\vec{F} \cdot \vec{n}) \, dS

The above means that the volume integral of the vector field divergence over the interior of a closed surface is equal to the flux of the vector field over the surface. But for this, a closed surface is required, so I will add a disk of radius 2 2 in the x y xy plane to the top of the sphere, and the two of them together form a closed surface.

To evaluate the left side of the integral equation, calculate the vector field divergence:

F = ( x , y , z ) ( z 2 x , y 3 3 + sin z , x 2 z + y 2 ) = z 2 + y 2 + x 2 = r 2 \nabla \cdot \vec{F} = \Big( \frac{\partial}{\partial{x}}, \frac{\partial}{\partial{y}}, \frac{\partial}{\partial{z}} \Big) \cdot \Big( z^2 x, \frac{y^3}{3} + \sin z, x^2 z + y^2 \Big) = z^2 + y^2 + x^2 = r^2

The triple integral of the divergence is then:

V r 2 d V = 0 π / 2 0 2 π 0 2 r 4 sin ϕ d r d θ d ϕ = 64 5 π = Ψ t o t a l \int \int \int_V r^2 \, dV = \int_0^{\pi/2} \int_0^{2 \pi} \int_0^2 r^4 \sin \phi \, dr \, d \theta \, d \phi = \frac{64}{5} \pi = \Psi_{total}

The above result is the total flux over the closed surface. Now find the flux over the bottom surface (the disk). On the disk, we have:

F = ( 0 , y 3 3 , y 2 ) n = ( 0 , 0 , 1 ) F n = y 2 \vec{F} = \Big( 0, \frac{y^3}{3} , y^2 \Big) \\ \vec{n} = (0, 0, -1) \\ \vec{F} \cdot \vec{n} = -y^2

The flux over the disk is:

d i s k y 2 d S = d i s k r 2 sin 2 θ ( r d r d θ ) = 0 2 π 0 2 r 3 sin 2 θ d r d θ = 4 π \int \int_{disk} -y^2 \, dS = \int \int_{disk} -r^2 \sin^2 \theta \, (r \, dr \, d\theta) = \int_0^{2 \pi} \int_0^2 -r^3 \sin^2 \theta \, dr \, d\theta = - 4 \pi

Now equate the two fluxes to the total flux:

Ψ t o t a l = Ψ d i s k + Ψ h a l f s p h e r e 64 5 π = 4 π + Ψ h a l f s p h e r e 64 5 π = 20 5 π + Ψ h a l f s p h e r e Ψ h a l f s p h e r e = 84 5 π \Psi_{total} = \Psi_{disk} + \Psi_{half sphere} \\ \frac{64}{5} \pi = - 4 \pi + \Psi_{half sphere} \\ \frac{64}{5} \pi = - \frac{20}{5} \pi + \Psi_{half sphere} \\ \Psi_{half sphere} = \frac{84}{5} \pi

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