Section
12.12
Worksheet:
Assignment: Exercises
pp. 806-808, #8, 18, 19, 30
(due Tuesday, 4/27).
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In what ways can we use the Taylor series to estimate the size of the errors
we're making in approximating a function with a Taylor polynomial of given
degree?
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In the optics example described at the end of the section, what motivated Gauss
to make his approximation?
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What is the ``punch line'' of Example 3, concerning Einstein's theory of
relativity?
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You've already seen Example 2: we did it, only using a polynomial approximation
of degree 7. Explain (again!) why only odd powers of x appear in the Taylor
series for .
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In which example is a binomial series approximation used?
Tue Apr 13 10:00:20 EDT 2004