Eisenstein integer

Last updated

In mathematics, the Eisenstein integers (named after Gotthold Eisenstein), occasionally also known [1] as Eulerian integers (after Leonhard Euler), are the complex numbers of the form

Contents

where a and b are integers and

is a primitive (hence non-real) cube root of unity.

Eisenstein integers as the points of a certain triangular lattice in the complex plane Eisenstein integer lattice.png
Eisenstein integers as the points of a certain triangular lattice in the complex plane

The Eisenstein integers form a triangular lattice in the complex plane, in contrast with the Gaussian integers, which form a square lattice in the complex plane. The Eisenstein integers are a countably infinite set.

Properties

The Eisenstein integers form a commutative ring of algebraic integers in the algebraic number field Q(ω) – the third cyclotomic field. To see that the Eisenstein integers are algebraic integers note that each z = a + is a root of the monic polynomial

In particular, ω satisfies the equation

The product of two Eisenstein integers a + and c + is given explicitly by

The 2-norm of an Eisenstein integer is just its squared modulus, and is given by

which is clearly a positive ordinary (rational) integer.

Also, the complex conjugate of ω satisfies

The group of units in this ring is the cyclic group formed by the sixth roots of unity in the complex plane: {±1, ±ω, ±ω2}, the Eisenstein integers of norm 1.

Euclidean domain

The ring of Eisenstein integers forms a Euclidean domain whose norm N is given by the square modulus, as above:

A division algorithm, applied to any dividend α and divisor β ≠ 0, gives a quotient κ and a remainder ρ smaller than the divisor, satisfying:

Here, α, β, κ, ρ are all Eisenstein integers. This algorithm implies the Euclidean algorithm, which proves Euclid's lemma and the unique factorization of Eisenstein integers into Eisenstein primes.

One division algorithm is as follows. First perform the division in the field of complex numbers, and write the quotient in terms of ω:

for rational a, bQ. Then obtain the Eisenstein integer quotient by rounding the rational coefficients to the nearest integer:

Here may denote any of the standard rounding-to-integer functions.

The reason this satisfies N(ρ) < N(β), while the analogous procedure fails for most other quadratic integer rings, is as follows. A fundamental domain for the ideal Z[ω]β = Zβ + Zωβ, acting by translations on the complex plane, is the 60°–120° rhombus with vertices 0, β, ωβ, β + ωβ. Any Eisenstein integer α lies inside one of the translates of this parallelogram, and the quotient κ is one of its vertices. The remainder is the square distance from α to this vertex, but the maximum possible distance in our algorithm is only , so . (The size of ρ could be slightly decreased by taking κ to be the closest corner.)

Eisenstein primes

Small Eisenstein primes. Those on the green axes are associate to a natural prime of the form 3n + 2. All others have an absolute value equal to 3 or square root of a natural prime of the form 3n + 1. EisensteinPrimes-01.svg
Small Eisenstein primes. Those on the green axes are associate to a natural prime of the form 3n + 2. All others have an absolute value equal to 3 or square root of a natural prime of the form 3n + 1.
Eisenstein primes in a larger range Eisenstein primes.svg
Eisenstein primes in a larger range

If x and y are Eisenstein integers, we say that x divides y if there is some Eisenstein integer z such that y = zx. A non-unit Eisenstein integer x is said to be an Eisenstein prime if its only non-unit divisors are of the form ux, where u is any of the six units. They are the corresponding concept to the Gaussian primes in the Gaussian integers.

There are two types of Eisenstein prime.

In the second type, factors of 3, and are associates: , so it is regarded as a special type in some books. [2] [3]

The first few Eisenstein primes of the form 3n − 1 are:

2, 5, 11, 17, 23, 29, 41, 47, 53, 59, 71, 83, 89, 101, ... (sequence A003627 in the OEIS ).

Natural primes that are congruent to 0 or 1 modulo 3 are not Eisenstein primes: [4] they admit nontrivial factorizations in Z[ω]. For example:

3 = −(1 + 2ω)2
7 = (3 + ω)(2 − ω).

In general, if a natural prime p is 1 modulo 3 and can therefore be written as p = a2ab + b2, then it factorizes over Z[ω] as

p = (a + )((ab) − ).

Some non-real Eisenstein primes are

2 + ω, 3 + ω, 4 + ω, 5 + 2ω, 6 + ω, 7 + ω, 7 + 3ω.

Up to conjugacy and unit multiples, the primes listed above, together with 2 and 5, are all the Eisenstein primes of absolute value not exceeding 7.

As of October 2023, the largest known real Eisenstein prime is the tenth-largest known prime 10223 × 231172165 + 1, discovered by Péter Szabolcs and PrimeGrid. [5] With one exception,[ clarification needed ] all larger known primes are Mersenne primes, discovered by GIMPS. Real Eisenstein primes are congruent to 2 mod 3, and all Mersenne primes greater than 3 are congruent to 1 mod 3; thus no Mersenne prime is an Eisenstein prime.

Eisenstein series

The sum of the reciprocals of all Eisenstein integers excluding 0 raised to the fourth power is 0: [6] so is a root of j-invariant. In general if and only if . [7]

The sum of the reciprocals of all Eisenstein integers excluding 0 raised to the sixth power can be expressed in terms of the gamma function: where E are the Eisenstein integers and G6 is the Eisenstein series of weight 6. [8]

Quotient of C by the Eisenstein integers

The quotient of the complex plane C by the lattice containing all Eisenstein integers is a complex torus of real dimension 2. This is one of two tori with maximal symmetry among all such complex tori.[ citation needed ] This torus can be obtained by identifying each of the three pairs of opposite edges of a regular hexagon.

Identifying each of the three pairs of opposite edges of a regular hexagon. Wrapped hexagon topology.png
Identifying each of the three pairs of opposite edges of a regular hexagon.

The other maximally symmetric torus is the quotient of the complex plane by the additive lattice of Gaussian integers, and can be obtained by identifying each of the two pairs of opposite sides of a square fundamental domain, such as [0, 1] × [0, 1].

See also

Notes

  1. Both Surányi, László (1997). Algebra. TYPOTEX. p. 73. and Szalay, Mihály (1991). Számelmélet. Tankönyvkiadó. p. 75. call these numbers "Euler-egészek", that is, Eulerian integers. The latter claims Euler worked with them in a proof.
  2. Weisstein, Eric W. "Eisenstein integer". MathWorld .
  3. Cox, David A. (1997-05-08). Primes of the Form x2+ny2: Fermat, Class Field Theory and Complex Multiplication (PDF). p. 77. ISBN   0-471-19079-9.
  4. " is reducible in iff ".
  5. "Largest Known Primes". The Prime Pages . Retrieved 2023-02-27.
  6. "What are the zeros of the j-function?".
  7. "Show that , and , ".
  8. "Entry 0fda1b – Fungrim: The Mathematical Functions Grimoire". fungrim.org. Retrieved 2023-06-22.

Related Research Articles

The propagation constant of a sinusoidal electromagnetic wave is a measure of the change undergone by the amplitude and phase of the wave as it propagates in a given direction. The quantity being measured can be the voltage, the current in a circuit, or a field vector such as electric field strength or flux density. The propagation constant itself measures the dimensionless change in magnitude or phase per unit length. In the context of two-port networks and their cascades, propagation constant measures the change undergone by the source quantity as it propagates from one port to the next.

<span class="mw-page-title-main">Winding number</span> Number of times a curve wraps around a point in the plane

In mathematics, the winding number or winding index of a closed curve in the plane around a given point is an integer representing the total number of times that the curve travels counterclockwise around the point, i.e., the curve's number of turns. For certain open plane curves, the number of turns may be a non-integer. The winding number depends on the orientation of the curve, and it is negative if the curve travels around the point clockwise.

<span class="mw-page-title-main">Bending</span> Strain caused by an external load

In applied mechanics, bending characterizes the behavior of a slender structural element subjected to an external load applied perpendicularly to a longitudinal axis of the element.

<span class="mw-page-title-main">Duffing equation</span> Non-linear second order differential equation and its attractor

The Duffing equation, named after Georg Duffing (1861–1944), is a non-linear second-order differential equation used to model certain damped and driven oscillators. The equation is given by where the (unknown) function is the displacement at time t, is the first derivative of with respect to time, i.e. velocity, and is the second time-derivative of i.e. acceleration. The numbers and are given constants.

In mathematics, in particular in algebraic geometry and differential geometry, Dolbeault cohomology (named after Pierre Dolbeault) is an analog of de Rham cohomology for complex manifolds. Let M be a complex manifold. Then the Dolbeault cohomology groups depend on a pair of integers p and q and are realized as a subquotient of the space of complex differential forms of degree (p,q).

<span class="mw-page-title-main">Lemniscate elliptic functions</span> Mathematical functions

In mathematics, the lemniscate elliptic functions are elliptic functions related to the arc length of the lemniscate of Bernoulli. They were first studied by Giulio Fagnano in 1718 and later by Leonhard Euler and Carl Friedrich Gauss, among others.

A quasiprobability distribution is a mathematical object similar to a probability distribution but which relaxes some of Kolmogorov's axioms of probability theory. Quasiprobabilities share several of general features with ordinary probabilities, such as, crucially, the ability to yield expectation values with respect to the weights of the distribution. However, they can violate the σ-additivity axiom: integrating over them does not necessarily yield probabilities of mutually exclusive states. Indeed, quasiprobability distributions also have regions of negative probability density, counterintuitively, contradicting the first axiom. Quasiprobability distributions arise naturally in the study of quantum mechanics when treated in phase space formulation, commonly used in quantum optics, time-frequency analysis, and elsewhere.

In the theory of general relativity, a stress–energy–momentum pseudotensor, such as the Landau–Lifshitz pseudotensor, is an extension of the non-gravitational stress–energy tensor that incorporates the energy–momentum of gravity. It allows the energy–momentum of a system of gravitating matter to be defined. In particular it allows the total of matter plus the gravitating energy–momentum to form a conserved current within the framework of general relativity, so that the total energy–momentum crossing the hypersurface of any compact space–time hypervolume vanishes.

The Newman–Penrose (NP) formalism is a set of notation developed by Ezra T. Newman and Roger Penrose for general relativity (GR). Their notation is an effort to treat general relativity in terms of spinor notation, which introduces complex forms of the usual variables used in GR. The NP formalism is itself a special case of the tetrad formalism, where the tensors of the theory are projected onto a complete vector basis at each point in spacetime. Usually this vector basis is chosen to reflect some symmetry of the spacetime, leading to simplified expressions for physical observables. In the case of the NP formalism, the vector basis chosen is a null tetrad: a set of four null vectors—two real, and a complex-conjugate pair. The two real members often asymptotically point radially inward and radially outward, and the formalism is well adapted to treatment of the propagation of radiation in curved spacetime. The Weyl scalars, derived from the Weyl tensor, are often used. In particular, it can be shown that one of these scalars— in the appropriate frame—encodes the outgoing gravitational radiation of an asymptotically flat system.

Cubic reciprocity is a collection of theorems in elementary and algebraic number theory that state conditions under which the congruence x3 ≡ p (mod q) is solvable; the word "reciprocity" comes from the form of the main theorem, which states that if p and q are primary numbers in the ring of Eisenstein integers, both coprime to 3, the congruence x3p is solvable if and only if x3q is solvable.

In many-body theory, the term Green's function is sometimes used interchangeably with correlation function, but refers specifically to correlators of field operators or creation and annihilation operators.

A ratio distribution is a probability distribution constructed as the distribution of the ratio of random variables having two other known distributions. Given two random variables X and Y, the distribution of the random variable Z that is formed as the ratio Z = X/Y is a ratio distribution.

A hydrogen-like atom (or hydrogenic atom) is any atom or ion with a single valence electron. These atoms are isoelectronic with hydrogen. Examples of hydrogen-like atoms include, but are not limited to, hydrogen itself, all alkali metals such as Rb and Cs, singly ionized alkaline earth metals such as Ca+ and Sr+ and other ions such as He+, Li2+, and Be3+ and isotopes of any of the above. A hydrogen-like atom includes a positively charged core consisting of the atomic nucleus and any core electrons as well as a single valence electron. Because helium is common in the universe, the spectroscopy of singly ionized helium is important in EUV astronomy, for example, of DO white dwarf stars.

In arithmetic, a complex-base system is a positional numeral system whose radix is an imaginary or complex number.

A product distribution is a probability distribution constructed as the distribution of the product of random variables having two other known distributions. Given two statistically independent random variables X and Y, the distribution of the random variable Z that is formed as the product is a product distribution.

The table of chords, created by the Greek astronomer, geometer, and geographer Ptolemy in Egypt during the 2nd century AD, is a trigonometric table in Book I, chapter 11 of Ptolemy's Almagest, a treatise on mathematical astronomy. It is essentially equivalent to a table of values of the sine function. It was the earliest trigonometric table extensive enough for many practical purposes, including those of astronomy. Since the 8th and 9th centuries, the sine and other trigonometric functions have been used in Islamic mathematics and astronomy, reforming the production of sine tables. Khwarizmi and Habash al-Hasib later produced a set of trigonometric tables.

<span class="mw-page-title-main">Vibration of plates</span>

The vibration of plates is a special case of the more general problem of mechanical vibrations. The equations governing the motion of plates are simpler than those for general three-dimensional objects because one of the dimensions of a plate is much smaller than the other two. This permits a two-dimensional plate theory to give an excellent approximation to the actual three-dimensional motion of a plate-like object.

In mathematics, infinite compositions of analytic functions (ICAF) offer alternative formulations of analytic continued fractions, series, products and other infinite expansions, and the theory evolving from such compositions may shed light on the convergence/divergence of these expansions. Some functions can actually be expanded directly as infinite compositions. In addition, it is possible to use ICAF to evaluate solutions of fixed point equations involving infinite expansions. Complex dynamics offers another venue for iteration of systems of functions rather than a single function. For infinite compositions of a single function see Iterated function. For compositions of a finite number of functions, useful in fractal theory, see Iterated function system.

Vasiliev equations are formally consistent gauge invariant nonlinear equations whose linearization over a specific vacuum solution describes free massless higher-spin fields on anti-de Sitter space. The Vasiliev equations are classical equations and no Lagrangian is known that starts from canonical two-derivative Frønsdal Lagrangian and is completed by interactions terms. There is a number of variations of Vasiliev equations that work in three, four and arbitrary number of space-time dimensions. Vasiliev's equations admit supersymmetric extensions with any number of super-symmetries and allow for Yang–Mills gaugings. Vasiliev's equations are background independent, the simplest exact solution being anti-de Sitter space. It is important to note that locality is not properly implemented and the equations give a solution of certain formal deformation procedure, which is difficult to map to field theory language. The higher-spin AdS/CFT correspondence is reviewed in Higher-spin theory article.

In supersymmetry, eleven-dimensional supergravity is the theory of supergravity in the highest number of dimensions allowed for a supersymmetric theory. It contains a graviton, a gravitino, and a 3-form gauge field, with their interactions uniquely fixed by supersymmetry. Discovered in 1978 by Eugène Cremmer, Bernard Julia, and Joël Scherk, it quickly became a popular candidate for a theory of everything during the 1980s. However, interest in it soon faded due to numerous difficulties that arise when trying to construct physically realistic models. It came back to prominence in the mid-1990s when it was found to be the low energy limit of M-theory, making it cruical for understanding various aspects of string theory.