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Review for Test #1
To adequately prepare for this test, you should be able to:
For the Chapter 1 material, you need to be able to:
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Explain the significance of any of the seven physical approximations we
made
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Derive the mean free path as the inverse of the macroscopic cross section
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Expand the directional dimension of the scattering cross section in Legendre
polynomials, using the orthogonality condition to arrive at the coefficients
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Use the total derivative flux with respect to distance traveled (d(psi)/ds)
is equivalent to the Omega dot Del psi. I will expect
you do expand the total derivative FULLY (in terms of all of the dependent
variables of flux and explain why some of the terms disappear in Cartesian
coordinates.
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List the explicit and implicit boundary condition types we studied -- void,
surface source, reflected, albedo, white, periodic.
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Develop the streaming operator in spherical coordinates as done in the
example in the notes.
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Demonstrate the equivalence of a conservative and non-conservative version
of the streaming operator for any curvilinear coordinate system.
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Explain the use of spherical harmonic moments and spherical harmonic distributions
to represent the scattering source term.
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Explain why source problems must be subcritical.
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Develop the k-effective (lambda) or time-absorption (alpha) eigenvalues,
showing how the Boltzmann Equation is modified for each of them and indicating
the range of values corresponding to subcriticality, criticality, and supercriticality.
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Develop the adjoint of any of the forward Boltzmann sub-operators -- L1,
L2, L3, or L4 -- as was done in class.
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Explain through use of the definition of the adjoint -- <a,Lb>=<b,L*a>
-- that either the forward or adjoint solution can be used to find a detector
response. Included in this is a description of how it is done (each
way) and examples of when one method would be preferred over the other.
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