Summation of series
Summation of series
Basic Concepts
- Series refers to the sum of terms in a sequence. An arithmetic series has a constant difference between terms, whereas a geometric series has a constant ratio.
Arithmetic Series
- The sum of the first n terms of an arithmetic series can be found using the formula:
- Sₙ = n/2 (2a + (n - 1)d) where a is the first term, and d the common difference.
- If the last term is known, another form is
- Sₙ = n/2 (a + l) where l represents the last term.
Geometric Series
- The sum of the first n terms of a finite geometric series is given by
- Sₙ = a (1 - rⁿ) / (1 - r), when the common ratio r is not 1.
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For infinite geometric series, when r < 1, the sum of the series is - S = a / (1 - r)
Sigma Notation
- Sigma (Σ) notation is a shorthand way of expressing a series. If Σaᵢ from i=m to n, then we add up the terms aᵢ for i=m to i=n.
Convergence and Divergence
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A series converges if the sum of its terms approaches a finite value. It diverges if the sum of its terms approaches infinity, or does not approach any value.
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A necessary condition for a geometric series to converge is r < 1.
Series Tests
- Two prominent series tests are the Comparison Test and the Ratio Test. The comparison test looks at how terms of the series compare to those of a known series, while the ratio test calculates the limit of the ratio of consecutive terms.
Maclaurin and Taylor Series
- A Maclaurin series is a Taylor series expansion of a function about 0. The general formula of a Maclaurin series is
- f(x) = f(0) + f’(0)x / 1! + f’‘(0)x² / 2! + …
- A Taylor series can provide an approximations for some functions. The general formula is
- f(x) = f(a) + f’(a)(x - a) / 1! + f’‘(a)(x - a)² / 2! + …