Wall–Sun–Sun prime
Named after | Donald Dines Wall, Zhi Hong Sun and Zhi Wei Sun |
---|---|
Publication year | 1992 |
No. of known terms | 0 |
Conjectured no. of terms | Infinite |
In number theory, a Wall–Sun–Sun prime or Fibonacci–Wieferich prime is a certain kind of prime number which is conjectured to exist, although none are known.
Definition
Let be a prime number. When each term in the sequence of Fibonacci numbers is reduced modulo , the result is a periodic sequence. The (minimal) period length of this sequence is called the Pisano period and denoted . Since , it follows that p divides . A prime p such that p2 divides is called a Wall–Sun–Sun prime.
Equivalent definitions
If denotes the rank of apparition modulo (i.e., is the smallest positive index such that divides ), then a Wall–Sun–Sun prime can be equivalently defined as a prime such that divides .
For a prime p ≠ 2, 5, the rank of apparition is known to divide , where the Legendre symbol has the values
This observation gives rise to an equivalent characterization of Wall–Sun–Sun primes as primes such that divides the Fibonacci number .[1]
A prime is a Wall–Sun–Sun prime if and only if .
A prime is a Wall–Sun–Sun prime if and only if , where is the -th Lucas number.[2]: 42
McIntosh and Roettger establish several equivalent characterizations of Lucas–Wieferich primes.[3] In particular, let ; then the following are equivalent:
Existence
In a study of the Pisano period , Donald Dines Wall determined that there are no Wall–Sun–Sun primes less than . In 1960, he wrote:[4]
The most perplexing problem we have met in this study concerns the hypothesis . We have run a test on digital computer which shows that for all up to ; however, we cannot prove that is impossible. The question is closely related to another one, "can a number have the same order mod and mod ?", for which rare cases give an affirmative answer (e.g., ; ); hence, one might conjecture that equality may hold for some exceptional .
It has since been conjectured that there are infinitely many Wall–Sun–Sun primes.[5]
In 2007, Richard J. McIntosh and Eric L. Roettger showed that if any exist, they must be > 2×1014.[3] Dorais and Klyve extended this range to 9.7×1014 without finding such a prime.[6]
In December 2011, another search was started by the PrimeGrid project,[7] however it was suspended in May 2017.[8] In November 2020, PrimeGrid started another project that searches for Wieferich and Wall–Sun–Sun primes simultaneously.[9] The project ended in December 2022, definitely proving that any Wall–Sun–Sun prime must exceed (about ).[10]
History
Wall–Sun–Sun primes are named after Donald Dines Wall,[4][11] Zhi Hong Sun and Zhi Wei Sun; Z. H. Sun and Z. W. Sun showed in 1992 that if the first case of Fermat's Last Theorem was false for a certain prime p, then p would have to be a Wall–Sun–Sun prime.[12] As a result, prior to Andrew Wiles' proof of Fermat's Last Theorem, the search for Wall–Sun–Sun primes was also the search for a potential counterexample to this centuries-old conjecture.
Generalizations
A tribonacci–Wieferich prime is a prime p satisfying h(p) = h(p2), where h is the least positive integer satisfying [Th,Th+1,Th+2] ≡ [T0, T1, T2] (mod m) and Tn denotes the n-th tribonacci number. No tribonacci–Wieferich prime exists below 1011.[13]
A Pell–Wieferich prime is a prime p satisfying p2 divides Pp−1, when p congruent to 1 or 7 (mod 8), or p2 divides Pp+1, when p congruent to 3 or 5 (mod 8), where Pn denotes the n-th Pell number. For example, 13, 31, and 1546463 are Pell–Wieferich primes, and no others below 109 (sequence A238736 in the OEIS). In fact, Pell–Wieferich primes are 2-Wall–Sun–Sun primes.
Near-Wall–Sun–Sun primes
A prime p such that with small |A| is called near-Wall–Sun–Sun prime.[3] Near-Wall–Sun–Sun primes with A = 0 would be Wall–Sun–Sun primes. PrimeGrid recorded cases with |A| ≤ 1000.[14] A dozen cases are known where A = ±1 (sequence A347565 in the OEIS).
Wall–Sun–Sun primes with discriminant D
Wall–Sun–Sun primes can be considered for the field with discriminant D. For the conventional Wall–Sun–Sun primes, D = 5. In the general case, a Lucas–Wieferich prime p associated with (P, Q) is a Wieferich prime to base Q and a Wall–Sun–Sun prime with discriminant D = P2 – 4Q.[1] In this definition, the prime p should be odd and not divide D.
It is conjectured that for every natural number D, there are infinitely many Wall–Sun–Sun primes with discriminant D.
The case of corresponds to the k-Wall–Sun–Sun primes, for which Wall–Sun–Sun primes represent the special case k = 1. The k-Wall–Sun–Sun primes can be explicitly defined as primes p such that p2 divides the k-Fibonacci number , where Fk(n) = Un(k, −1) is a Lucas sequence of the first kind with discriminant D = k2 + 4 and is the Pisano period of k-Fibonacci numbers modulo p.[15] For a prime p ≠ 2 and not dividing D, this condition is equivalent to either of the following.
- p2 divides , where is the Kronecker symbol;
- Vp(k, −1) ≡ k (mod p2), where Vn(k, −1) is a Lucas sequence of the second kind.
The smallest k-Wall–Sun–Sun primes for k = 2, 3, ... are
See also
- Wieferich prime
- Wolstenholme prime
- Wilson prime
- PrimeGrid
- Fibonacci prime
- Pisano period
- Table of congruences
References
- ^ a b A.-S. Elsenhans, J. Jahnel (2010). "The Fibonacci sequence modulo p2 -- An investigation by computer for p < 1014". arXiv:1006.0824 [math.NT].
- ^ Andrejić, V. (2006). "On Fibonacci powers" (PDF). Univ. Beograd Publ. Elektrotehn. Fak. Ser. Mat. 17 (17): 38–44. doi:10.2298/PETF0617038A. S2CID 41226139.
- ^ a b c McIntosh, R. J.; Roettger, E. L. (2007). "A search for Fibonacci−Wieferich and Wolstenholme primes" (PDF). Mathematics of Computation. 76 (260): 2087–2094. Bibcode:2007MaCom..76.2087M. doi:10.1090/S0025-5718-07-01955-2.
- ^ a b Wall, D. D. (1960), "Fibonacci Series Modulo m", American Mathematical Monthly, 67 (6): 525–532, doi:10.2307/2309169, JSTOR 2309169
- ^ Klaška, Jiří (2007), "Short remark on Fibonacci−Wieferich primes", Acta Mathematica Universitatis Ostraviensis, 15 (1): 21–25.
- ^ Dorais, F. G.; Klyve, D. W. (2010). "Near Wieferich primes up to 6.7 × 1015" (PDF).
- ^ Wall–Sun–Sun Prime Search project at PrimeGrid
- ^ [1] at PrimeGrid
- ^ Message boards : Wieferich and Wall-Sun-Sun Prime Search at PrimeGrid
- ^ Subproject status at PrimeGrid
- ^ Crandall, R.; Dilcher, k.; Pomerance, C. (1997). "A search for Wieferich and Wilson primes". Mathematics of Computation. 66 (217): 447. Bibcode:1997MaCom..66..433C.
- ^ Sun, Zhi-Hong; Sun, Zhi-Wei (1992), "Fibonacci numbers and Fermat's last theorem" (PDF), Acta Arithmetica, 60 (4): 371–388, doi:10.4064/aa-60-4-371-388
- ^ Klaška, Jiří (2008). "A search for Tribonacci–Wieferich primes". Acta Mathematica Universitatis Ostraviensis. 16 (1): 15–20.
- ^ Reginald McLean and PrimeGrid, WW Statistics
- ^ S. Falcon, A. Plaza (2009). "k-Fibonacci sequence modulo m". Chaos, Solitons & Fractals. 41 (1): 497–504. Bibcode:2009CSF....41..497F. doi:10.1016/j.chaos.2008.02.014.
Further reading
- Crandall, Richard E.; Pomerance, Carl (2001). Prime Numbers: A Computational Perspective. Springer. p. 29. ISBN 0-387-94777-9.
- Saha, Arpan; Karthik, C. S. (2011). "A Few Equivalences of Wall–Sun–Sun Prime Conjecture". arXiv:1102.1636 [math.NT].
External links
- Chris Caldwell, The Prime Glossary: Wall–Sun–Sun prime at the Prime Pages.
- Weisstein, Eric W. "Wall–Sun–Sun prime". MathWorld.
- Richard McIntosh, Status of the search for Wall–Sun–Sun primes (October 2003)
- OEIS sequence A000129 (Primes p that divide their Pell quotients, where the Pell quotient of p is A000129(p - (2/p))/p and (2/p) is a Jacobi symbol)