Surface integrals and heat flow

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Homework Help Overview

The problem involves calculating the rate of heat flow outward across the surface of a spherical star, where the temperature is inversely proportional to the distance from the center. The conductivity of the star is given, and the temperature function is provided as a scalar function.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants express confusion regarding the application of conductivity in the context of surface integrals and the scalar nature of the temperature function. Some suggest using spherical coordinates and Gauss' theorem, while others question how to derive a vector heat field from the scalar temperature field.

Discussion Status

The discussion is ongoing, with participants exploring various mathematical approaches, including the divergence theorem and the gradient of the temperature function. Some guidance has been offered regarding the formulation of the heat field and the application of Gauss' theorem, but no consensus has been reached on the next steps.

Contextual Notes

Participants note a time constraint, as the problem is due in a short time frame. There is also mention of a lack of familiarity with the necessary concepts, particularly regarding conductivity and surface integrals.

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Homework Statement



The temperature u in a star of conductivity 6 is inversely proportional to the distance from the center:

u = \frac{3}{\sqrt{x^{2} + y^{2} + z^{2}}}

If the star is a sphere of radius 3, find the rate of heat flow outward across the surface of the star.

Homework Equations


The Attempt at a Solution



I really don't know what to do here - I have not learned about "conductivity" in terms of taking surface integrals and every example problem my teacher has done has involved a force function, yet this seems to only give a scalar temperature function.

So, I am thoroughly confused as to where to start?
 
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im doing the exact same one , it is due in 7 hrs
im lost too but

you know z^2+y^2+x^2 = r^2 so plug that into the eq. and solve for u.

after that I am lost
 
That looks to me like you need Gauss' theorem:
\int\int\int \nabla \cdot \vec{f} dV= \int\int \vec{f}\cdot \vec{n}dS
where the first integral is over a bounded region and the second over the surface of that area. The right side is the flow across the surface and so the integrand is the rate of heat flow across the surface.
 
you mean divergence theorem? but what is the vector field?
 
can you make a vector heat field from your scalar tempertaure field?

any differential conduction equations that might hep?
 
the gradient.

then what?

use DIV theorem and spherical coordinates?
 
right so you get the heat field from something like

\vec{q} = -k \nabla u

and
u(r) = \frac{3}{r}

now try the left hand integral given by Halls in Gauss's theorem, i think this is effectively summing up all the heat generated by the star, which in steady state will also be the amount leaving the surface of the star (by the way does the form of the field look familiar? maybe you can think of the temperature as the potential)

knowing the surface area of the star & due to the spherical symmetry of the heat field, you should be able to work back to the integrand on the right
 
Last edited:

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