Series Expansion: every key term you need (+ practice quiz)
30 flashcard terms for AP Calculus BC Unit 10, written to match the course framework. Study them here, then drill them as interactive flashcards, or test yourself with the 27-question quiz — free, no account needed.
|R_n(x)| ≤ M|x-a|^(n+1)/(n+1)! where M bounds |f^(n+1)| on the interval between a and x.
Choosing M
M must bound the (n+1)st derivative on the whole interval, not just at the center; sine and cosine always allow M=1.
Alternating Bound vs Lagrange
If the Taylor series alternates with decreasing terms, the simpler alternating bound applies; otherwise use Lagrange.
Operations on Series
Series may be added, multiplied, substituted into, differentiated, and integrated term by term within the common interval of convergence.
Finding a Series by Substitution
To expand e^(-x²), substitute -x² into the e^u series rather than differentiating repeatedly — far faster and less error-prone.
Evaluating Limits with Series
Replacing functions by their first few Maclaurin terms resolves 0/0 limits without repeated L'Hôpital passes.
Approximating Integrals with Series
Functions like sin(x)/x or e^(-x²) with no elementary antiderivative can be integrated term by term to any desired accuracy.
Coefficient Extraction
The coefficient of (x-a)^n in a Taylor series equals f^(n)(a)/n!, so f^(n)(a) = n!·c_n — a common exam question in reverse.
Radius of Convergence of a Taylor Series
Determined by the ratio test on the coefficients; for real functions it often equals the distance to the nearest point where the function misbehaves.
Degree Needed for an Accuracy Goal
Set the error bound less than the target tolerance and solve for the smallest n, testing integer values since the inequality is rarely solvable in closed form.
Taylor Polynomials from a Table of Derivatives
AP problems frequently give f(a), f'(a), f''(a), f'''(a) and ask you to build P_3 directly, dividing each by the appropriate factorial.
Series and Function Identity
A Taylor series equals its function only where the remainder tends to zero; for e^x, sin x, and cos x this holds everywhere.