Heegner number

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Template:Short description In number theory, Heegner numbers are square-free positive integers d such that the imaginary quadratic field ℚ(−d) has class number 1. Equivalently, the ring of algebraic integers of ℚ(−d) has unique factorization.Template:Sfnp

The determination of such numbers is a special case of the class number problem, and they underlie several striking results in number theory.

According to the Stark–Heegner theorem there are precisely nine Heegner numbers: Template:Block indent This result was conjectured by Gauss and proved up to minor flaws by Kurt Heegner in 1952. Alan Baker and Harold Stark independently proved the result in 1966, and Stark further indicated that the gap in Heegner's proof was minor.Template:Sfnp

Euler's prime-generating polynomial

Euler's prime-generating polynomial

n2+n+41,

which gives distinct primes for n=0,...,39, is relatedTemplate:How to the Heegner number 163=4⋅41−1 by the discriminant of the polynomial.

Rabinowitsch[1] proved that the polynomial

n2+n+p

gives primes for n=0,…,p−2 if and only if its discriminant 1−4p is the negative of a Heegner number.

1, 2, and 3 are not of the required form, so the Heegner numbers that work are 7, 11, 19, 43, 67, 163, yielding prime generating functions of Euler's form for 2, 3, 5, 11, 17, 41; these latter numbers are called lucky numbers of Euler by F. Le Lionnais.[2]

Almost integers and Ramanujan's constant

Ramanujan's constant is the transcendental number[3] eπ163, which is an almost integer:[4] eπ163=262537412640768743.99999999999925…≈6403203+744.

This number was discovered in 1859 by the mathematician Charles Hermite.Template:Sfnp In a 1975 April Fools' Day article in Scientific American magazine,Template:Sfnp "Mathematical Games" columnist Martin Gardner made the hoax claim that the number was in fact an integer, and that the Indian mathematical genius Srinivasa Ramanujan had predicted it—hence its name.

Details

This coincidence is explained by complex multiplication and the q-expansion of the j-invariant. In what follows, j(z) denotes the j-invariant of the complex number z. Briefly, j(1+−d2) is an integer for d a Heegner number, and eπd≈−j(1+−d2)+744 via the q-expansion.

If τ is a quadratic irrational, then its j-invariant j(τ) is an algebraic integer of degree |Cl(ℚ(τ))|, the class number of ℚ(τ) and the minimal (monic integral) polynomial it satisfies is called the 'Hilbert class polynomial'. Thus if the imaginary quadratic extension ℚ(τ) has class number 1 (so d is a Heegner number), the j-invariant is an integer.

The q-expansion of j, with its Fourier series expansion written as a Laurent series in terms of q=e2πiτ, begins as: j(τ)=1q+744+196884q+⋯.

The coefficients cn asymptotically grow as ln⁡(cn)∼4πn+O(ln⁡(n)), and the low order coefficients grow more slowly than 200000n, so for q≪1200000, j is very well approximated by its first two terms. Setting τ=1+−1632 yields q=−e−π163∴1q=−eπ163. Now j(1+−1632)=(−640320)3, so, (−640320)3=−eπ163+744+O(e−π163). Or, eπ163=6403203+744+O(e−π163) where the linear term of the error is,Template:Wbr −196884eπ163≈−1968846403203+744≈−0.00000000000075Template:Pb explaining why eπ163 is within approximately the above of being an integer.

Pi formulas

The Chudnovsky brothers found in 1987 that 1π=1264032032∑k=0∞(6k)!(163⋅3344418k+13591409)(3k)!(k!)3(−640320)3k, a proof of which uses the fact that j(1+−1632)=−6403203. For similar formulas, see the Ramanujan–Sato series.

Other Heegner numbers

For the four largest Heegner numbers, the approximations one obtains[5] are as follows. eπ19≈0000963+744−0.22eπ43≈0009603+744−0.00022eπ67≈0052803+744−0.0000013eπ163≈6403203+744−0.00000000000075

Alternatively,[6] eπ19≈123(32−1)300+744−0.22eπ43≈123(92−1)300+744−0.00022eπ67≈123(212−1)30+744−0.0000013eπ163≈123(2312−1)3+744−0.00000000000075 where the reason for the squares is due to certain Eisenstein series. For Heegner numbers d<19, one does not obtain an almost integer; even d=19 is not noteworthy.[7] The integer j-invariants are highly factorisable, which follows from the form

123(n2−1)3=(22⋅3⋅(n−1)⋅(n+1))3,

and factor as, j(1+−192)=0000−963=−(25⋅3)3j(1+−432)=000−9603=−(26⋅3⋅5)3j(1+−672)=00−52803=−(25⋅3⋅5⋅11)3j(1+−1632)=−6403203=−(26⋅3⋅5⋅23⋅29)3.

These transcendental numbers, in addition to being closely approximated by integers (which are simply algebraic numbers of degree 1), can be closely approximated by algebraic numbers of degree 3,[8] eπ19≈x24−24.00031;x3−2x−2=0eπ43≈x24−24.00000031;x3−2x2−2=0eπ67≈x24−24.0000000019;x3−2x2−2x−2=0eπ163≈x24−24.0000000000000011;x3−6x2+4x−2=0

The roots of the cubics can be exactly given by quotients of the Dedekind eta function η(τ), a modular function involving a 24th root, and which explains the 24 in the approximation. They can also be closely approximated by algebraic numbers of degree 4,[9] eπ19≈35(3−2(1−9624+13⋅19))−2−12.00006…eπ43≈35(9−2(1−96024+73⋅43))−2−12.000000061…eπ67≈35(21−2(1−528024+313⋅67))−2−12.00000000036…eπ163≈35(231−2(1−64032024+24133⋅163))−2−12.00000000000000021…

If x denotes the expression within the parenthesis (e.g. x=3−2(1−9624+13⋅19)), it satisfies respectively the quartic equations x4−004⋅3x3+000023(96+3)x2−00000023⋅3(96−6)x−3=0x4−004⋅9x3+00023(960+3)x2−0000023⋅9(960−6)x−3=0x4−04⋅21x3+0023(5280+3)x2−00023⋅21(5280−6)x−3=0x4−4⋅231x3+23(640320+3)x2−23⋅231(640320−6)x−3=0

Note the reappearance of the integers n=3,9,21,231 as well as the fact that 26⋅3(−(1−9624)2+12⋅3⋅19)=96226⋅3(−(1−96024)2+72⋅3⋅43)=960226⋅3(−(1−528024)2+312⋅3⋅67)=5280226⋅3(−(1−64032024)2+24132⋅3⋅163)=6403202 which, with the appropriate fractional power, are precisely the j-invariants.

Similarly for algebraic numbers of degree 6, eπ19≈(5x)3−6.000010…eπ43≈(5x)3−6.000000010…eπ67≈(5x)3−6.000000000061…eπ163≈(5x)3−6.000000000000000034…

where the xs are given respectively by the appropriate root of the sextic equations, 5x6−000096x5−10x3+1=05x6−000960x5−10x3+1=05x6−005280x5−10x3+1=05x6−640320x5−10x3+1=0

with the j-invariants appearing again. These sextics are not only algebraic, they are also solvable in radicals as they factor into two cubics over the extension ℚ5 (with the first factoring further into two quadratics). These algebraic approximations can be exactly expressed in terms of Dedekind eta quotients. As an example, let τ=1+−1632, then, eπ163=(eπi24η(τ)η(2τ))24−24.00000000000000105…eπ163=(eπi12η(τ)η(3τ))12−12.00000000000000021…eπ163=(eπi6η(τ)η(5τ))6−6.000000000000000034…

where the eta quotients are the algebraic numbers given above.

Class 2 numbers

The three numbers 88, 148, 232, for which the imaginary quadratic field ℚ[−d] has class number 2, are not Heegner numbers but have certain similar properties in terms of almost integers. For instance,[10] eπ88+8744≈000025089522−0.077…eπ148+8744≈001991486482−0.00097…eπ232+8744≈245912577522−0.0000078… and eπ22−24≈00(6+42)6+0.00011…eπ37+24≈(12+237)6−0.0000014…eπ58−24≈(27+529)6−0.0000000011…

Consecutive primes

Given an odd prime p, if one computes k2 mod p for k=0,1,…,p−12 (this is sufficient because (p−k)2≡k2 (mod p)), one gets consecutive composites, followed by consecutive primes, if and only if p is a Heegner number[11] Template:Xref.[12]

Notes

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References

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  1. ↑ Rabinovitch, Georg "Eindeutigkeit der Zerlegung in Primzahlfaktoren in quadratischen Zahlkörpern." Proc. Fifth Internat. Congress Math. ( Cambridge) 1, 418–421, 1913.
  2. ↑ Le Lionnais, F. Les nombres remarquables. Paris: Hermann, pp. 88 and 144, 1983.
  3. ↑ Template:MathWorld gives eπd,d∈Z∗, based on Nesterenko, Yu. V. "On Algebraic Independence of the Components of Solutions of a System of Linear Differential Equations." Izv. Akad. Nauk SSSR, Ser. Mat. 38, 495–512, 1974. English translation in Math. USSR 8, 501–518, 1974.
  4. ↑ Ramanujan Constant – from Wolfram MathWorld
  5. ↑ These can be checked by computing eπd−7443 on a calculator, and 196884eπd for the linear term of the error.
  6. ↑ Template:Cite web
  7. ↑ The absolute deviation of a random real number (picked uniformly from [[Unit interval|Template:Closed-closed]], say) is a uniformly distributed variable on Template:Closed-closed, so it has absolute average deviation and median absolute deviation of 0.25, and a deviation of 0.22 is not exceptional.
  8. ↑ Template:Cite web
  9. ↑ Template:Cite web
  10. ↑ Template:Cite web
  11. ↑ Template:Cite web
  12. ↑ Template:Cite journal