
Description:
Hip calculus discussion, with problems and solutions.
Contents:
Properties of Log
There are some properties of logarithms that you absolutely must know to get through calculus. Most students shriek or faint when they see a logarithm, but if you learn these simple rules they become much easier to work with. Get a little practice, and you’ll be on your way to mastering logarithms!
All you really need to know are two rules: first, logs turn multiplication into addition:
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Second, taking the log of a power turns into multiplication by the exponent:
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From these, we can deduce a rule for quotients:

Here’s an exercise: how could I have shown the third rule if I only knew the first two?
To get more examples of problems with logs, take a look at the 99 calculus solutions manual.

Limits That Don’t Exist
Integration by Parts
Textbook Rental
Integrating the Natural Logarithm
You’ll probably see this integral someday:
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It looks so simple, and you think, “gee, I probably was supposed to memorize that” or “oh I can do that, it looks so easy.” But then you don’t remember the antiderivative and get stuck. Cause, heck, what can you do with just anyway? It doesn’t decompose into anything nicer.
The trick is to use integration by parts. Let’s look at it backwards:
If we were really smart or really lucky, we might approach this problem by saying
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(Is this really true? Use the product rule to show it.) Then we can integrate both sides:
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Now using the Fundamental theorem of calculus, the integral on the left is just equal to . Solving for , we get
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Yay!

Remembering One Trig Identity
Some Facts About Complex Numbers
Euler’s Formula
In the last post we talked about two important trig identities. I said you should memorize them (and you probably should), but what if you forget? I want to talk about a powerful way to derive trig identities by remembering just a couple of facts. This is great if you’re forgetful like me! To get started, though, we need to look at a wonderful formula discovered by Leonhard Euler. It’s called, appropriately enough, Euler’s Formula:
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