A height function is a function that quantifies the complexity of mathematical objects. In Diophantine geometry, height functions quantify the size of solutions to Diophantine equations and are typically functions from a set of points on algebraic varieties (or a set of algebraic varieties) to the real numbers. For instance, the classical or naive height over the rational numbers is typically defined to be the maximum of the numerators and denominators of the coordinates (e.g. 7 for the coordinates (3/7, 1/2)), but in a logarithmic scale.
Significance Height functions allow mathematicians to count objects, such as rational points, that are otherwise infinite in quantity. For instance, the set of rational numbers of naive height (the maximum of the numerator and denominator when expressed in lowest terms) below any given constant is finite despite the set of rational numbers being infinite. In this sense, height functions can be used to prove asymptotic results such as Baker's theorem in transcendental number theory which was proved by Alan Baker (1966, 1967a, 1967b). In other cases, height functions can distinguish some objects based on their complexity. For instance, the subspace theorem proved by Wolfgang M. Schmidt (1972) demonstrates that points of small height (i.e. small complexity) in projective space lie in a finite number of hyperplanes and generalizes Siegel's theorem on integral points and solution of the S-unit equation. Height functions were crucial to the proofs of the Mordell–Weil theorem and Faltings' theorem by Weil (1929) and Faltings (1983) respectively. Several outstanding unsolved problems about the heights of rational points on algebraic varieties, such as the Manin conjecture and Vojta's conjecture, have far-reaching implications for problems in Diophantine approximation, Diophantine equations, arithmetic geometry, and mathematical logic.
History An early form of height function was proposed by Giambattista Benedetti (c. 1563), who argued that the consonance of a musical interval could be measured by the product of its numerator and denominator (in reduced form); see Giambattista Benedetti § Music. Heights in Diophantine geometry were initially developed by André Weil and Douglas Northcott beginning in the 1920s. Innovations in 1960s were the Néron–Tate height and the realization that heights were linked to projective representations in much the same way that ample line bundles are in other parts of algebraic geometry. In the 1970s, Suren Arakelov developed Arakelov heights in Arakelov theory. In 1983, Faltings developed his theory of Faltings heights in his proof of Faltings' theorem.
Height functions in Diophantine geometry
Naive height Classical or naive height is defined in terms of ordinary absolute value on homogeneous coordinates. It is typically a logarithmic scale and therefore can be viewed as being proportional to the "algebraic complexity" or number of bits needed to store a point. It is typically defined to be the logarithm of the maximum absolute value of the vector of coprime integers obtained by multiplying through by a lowest common denominator. This may be used to define height on a point in projective space over Q, or of a polynomial, regarded as a vector of coefficients, or of an algebraic number, from the height of its minimal polynomial. The naive height of a rational number x = p/q (in lowest terms) is
multiplicative height H ( p / q ) = max { | p | , | q | } {\displaystyle H(p/q)=\max\{|p|,|q|\}}
logarithmic height: h ( p / q ) = log H ( p / q ) {\displaystyle h(p/q)=\log H(p/q)}
Therefore, the naive multiplicative and logarithmic heights of 4/10 are 5 and log(5), for example. The naive height H of an elliptic curve E given by y2 = x3 + Ax + B is defined to be H(E) = log max(4|A|3, 27|B|2).
Néron–Tate height
The Néron–Tate height, or canonical height, is a quadratic form on the Mordell–Weil group of rational points of an abelian variety defined over a global field. It is named after André Néron, who first defined it as a sum of local heights, and John Tate, who defined it globally in an unpublished work.
Weil height Let X be a projective variety over a number field K. Let L be a line bundle on X. One defines the Weil height on X with respect to L as follows. First, suppose that L is very ample. A choice of basis of the space Γ ( X , L ) {\displaystyle \Gamma (X,L)} of global sections defines a morphism ϕ from X to projective space, and for all points p on X, one defines
h L ( p ) := h ( ϕ ( p ) ) {\displaystyle h_{L}(p):=h(\phi (p))} , where h is the naive height on projective space. For fixed X and L, choosing a different basis of global sections changes h L {\displaystyle h_{L}} , but only by a bounded function of p. Thus h L {\displaystyle h_{L}} is well-defined up to addition of a function that is O(1). In general, one can write L as the difference of two very ample line bundles L1 and L2 on X and define h L := h L 1 − h L 2 , {\displaystyle h_{L}:=h_{L_{1}}-h_{L_{2}},}
which again is well-defined up to O(1).
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