Geometric series
A geometric series is a mathematical series formed by a sequence of terms where each term after the first is obtained by multiplying the preceding term by a fixed, nonzero constant known as the common ratio r.[1] The general form of an infinite geometric series is \sum_{n=0}^{\infty} a r^n, where a is the first term.[2] The sum of the first n terms of a finite geometric series, denoted S_n, is calculated using the formula S_n = a \frac{1 - r^n}{1 - r} for r \neq 1.[1] For the infinite case, the series converges to the sum S = \frac{a}{1 - r} if and only if the absolute value of the common ratio satisfies |r| < 1; otherwise, it diverges.[2] This convergence criterion is a cornerstone of series analysis in calculus, distinguishing geometric series from other types like harmonic or p-series.[1] Historically, geometric series trace their origins to ancient Greek mathematics, with early appearances in Zeno's paradoxes of the 5th century BCE, such as the Achilles and the tortoise dilemma, which implicitly relies on the summation of an infinite geometric series to resolve apparent contradictions in motion and infinity.[3] These paradoxes highlighted the need for rigorous understanding of infinite sums, paving the way for later developments in analysis by mathematicians like Archimedes and, in the modern era, Isaac Newton and Gottfried Wilhelm Leibniz.[3] Beyond pure mathematics, geometric series find extensive applications across disciplines due to their ability to model exponential growth and decay processes.[4] In finance, they underpin calculations of compound interest, where periodic returns form a geometric progression.[4] In physics and biology, they describe phenomena like radioactive decay and population growth under constant multiplication rates, and in engineering, signal attenuation.[5][6][7] Additionally, in computer science, geometric series appear in analyzing the time complexity of recursive algorithms.[8]Definition and Fundamentals
Definition
A geometric series is the sum of the terms of a geometric progression, which is a sequence of numbers where each term after the first is found by multiplying the previous one by a fixed, non-zero constant called the common ratio.[9] The underlying geometric progression takes the form a, ar, ar^2, ar^3, \dots, where a is the first term and r is the common ratio, with the general term given by ar^{k} for k = 0, 1, 2, \dots.[1] For the finite case, a geometric series consists of a finite number of terms from this progression, expressed as the partial sum S_n = \sum_{k=0}^{n-1} ar^k, where n denotes the number of terms; equivalently, it may start the index at 1 as \sum_{k=1}^{n} ar^{k-1}.[2] In the infinite case, the geometric series is the sum over infinitely many terms, S = \sum_{k=0}^{\infty} ar^k, or alternatively \sum_{k=1}^{\infty} ar^{k-1}, and is understood as the limit of the partial sums S_n as n approaches infinity, provided this limit exists.[1] Notation for partial sums often uses S_n to emphasize the finite approximation to the infinite series.[9]Examples
A classic example of a finite geometric series is the sum of the first four terms of the sequence 1, 2, 4, 8, where the first term is 1 and the common ratio is 2; this series totals 15. To illustrate the terms and partial sums, consider the following table for this series:| Term number | Term value | Partial sum |
|---|---|---|
| 1 | 1 | 1 |
| 2 | 2 | 3 |
| 3 | 4 | 7 |
| 4 | 8 | 15 |
| Term number | Term value | Partial sum |
|---|---|---|
| 1 | 1 | 1 |
| 2 | \frac{1}{2} | 1.5 |
| 3 | \frac{1}{4} | 1.75 |
| 4 | \frac{1}{8} | 1.875 |
| \dots | \dots | approaching 2 |