Fibonacci Sequence
FIBONACCI SEQUENCE
The Fibonacci sequence is defined by the recurrence
Thus each new term is obtained by adding the two previous terms.
The historical notes in this section follow Graham, Knuth, and Patashnik, Concrete Mathematics, Second Edition, Section 6.6.
The sequence is named after Leonardo Fibonacci, who introduced these numbers to Western European mathematics in 1202. Edouard Lucas studied the sequence extensively in the nineteenth century and helped popularize the term Fibonacci numbers. One of his amazing results was to use properties of Fibonacci numbers to prove that the 39-digit Mersenne number is prime.
Fibonacci numbers appear in many different parts of mathematics. One famous early identity is due to the French astronomer Jean-Dominique Cassini, who presented it in 1680 [Cassini1733]:
For example, when , this gives
This identity is a first sign that the simple recurrence defining the Fibonacci sequence hides a rich algebraic structure.
Another important property is that Fibonacci numbers can be used to represent integers in a special way. Every positive integer can be written uniquely as a sum of nonconsecutive Fibonacci numbers. This result is known as Zeckendorf's theorem. For example,
In Fibonacci notation, this is
The condition that the Fibonacci numbers are nonconsecutive is essential for uniqueness: we are not allowed to use two neighboring Fibonacci numbers in the same representation.
The Fibonacci recurrence is linear, so it is natural to look first for solutions of the simpler form
with . If this sequence satisfies the same recurrence , then
Dividing by gives the characteristic equation
By the quadratic formula, the two roots are
The number is the golden ratio.
Both sequences and satisfy the Fibonacci recurrence. Since the recurrence is linear, adding two solutions, or multiplying a solution by a constant, produces another solution. Therefore every sequence of the form
also satisfies it. We now choose and so that the initial values agree with and .
From , we get
so . From , we get
But
BINET'S FORMULA
Substituting these constants gives Binet's formula:
This closed formula was first published by Leonhard Euler in 1765 [Euler1765]. It was later rediscovered by Jacques Binet in 1843 [Binet1843], which is why the formula is now commonly called Binet's formula.
References
- [GrahamKnuthPatashnik1994]Graham, Ronald L.; Knuth, Donald E.; Patashnik, Oren. \textit{Concrete Mathematics: A Foundation for Computer Science}. Second edition. Addison-Wesley, 1994.
- [Cassini1733]Cassini, Jean-Dominique. ``Une nouvelle progression de nombres.'' \textit{Histoire de l'Academie Royale des Sciences}, Paris, volume 1, 201. Presented in 1680 and published in 1733.
- [Euler1765]Euler, Leonhard. ``Observationes analyticae.'' \textit{Novi commentarii academiae scientiarum imperialis Petropolitanae} 11 (1765), 124--143. Reprinted in \textit{Opera Omnia}, series 1, volume 15, 50--69.
- [Binet1843]Binet, Jacques. ``Memoire sur l'integration des equations lineaires aux differences finies, d'un ordre quelconque, a coefficients variables.'' \textit{Comptes Rendus hebdomadaires des seances de l'Academie des Sciences} (Paris) 17 (1843), 559--567.