Italian school of algebraic geometry

In relation with the history of mathematics, the Italian school of algebraic geometry refers to the work over half a century or more (flourishing roughly 1885-1935) done internationally in birational geometry, particularly on algebraic surfaces. There were in the region of 30 to 40 leading mathematicians who made major contributions; about half of those being in fact Italian. There is no question that the leadership fell to the group in Rome of Guido Castelnuovo, Federigo Enriques and Francesco Severi; who were involved in some of the deepest discoveries, as well as setting the style. The fashion and foundational attitude changed in algebraic geometry from 1950 onwards, leading to an axiomatisation and some acrimony as to the status of some results. For a while it may have seemed that the tradition of the Italian school would possibly be lost, in the sense that the old papers had become hard to read for the new generation of geometers. The essentials were in fact transmitted, in particular through Zariski s students; and some of the areas opened up, such as moduli spaces for curves, have been at the centre of recent work related to Physics. Very many of the fundamental concepts in algebraic geometry still bear the names of those of the Italian school.

The emphasis on algebraic surfaces — algebraic variety of dimension of an algebraic variety two — followed on from an essentially complete geometric theory of algebraic curves (dimension 1). The position in around 1870 was that the curve theory had incorporated with Brill-Noether theory the Riemann-Roch theorem in all its refinements (via the detailed geometry of the theta-divisor).

The school and others by around 1960. The form of the Riemann-Roch theorem on a surface was also worked out.

Qualification of what was actually proved is necessary because of the foundational difficulties. These included intensive use of birational models in dimension 3 of surfaces that can have non-singular models only when embedded in higher-dimensional projective space. That is, the theory wasn t posed in an intrinsic way. To get round that, a sophisticated theory of handling a linear system of divisors was developed (in effect, a line bundle theory for hyperplane sections of putative embeddings in projective space). Many of the modern techniques were found, in embryo form, and in some cases the articulation of those exceeded the available technical language.

The roll of honour of the school includes the following major Italians: Albanese, Bertini, Campedelli, Guido Castelnuovo, Oscar Chisini, Federigo Enriques, De Franchis, Del Pezzo, Beniamino Segre, Corrado Segre, Francesco Severi, Guido Zappa (with contributions also from Luigi Cremona, Gino Fano, Rosati, Torelli, Veronese). Elsewhere it involved H. F. Baker and P. Duval (UK), A. B. Coble and Oscar Zariski (USA), Charles �mile Picard (France), Lucien Godeaux (Belgium), G. Humbert, Schubert and Max Noether, and later Erich Kähler (Germany), H. G. Zeuthen (Denmark). These figures were all involved in algebraic geometry, rather than the pursuit of projective geometry as synthetic geometry, which during the period under discussion was a huge (in volume terms) but secondary subject (when judged by its importance as research).

The new algebraic geometry that would succeed the Italian school was distinguished also by the intensive use of algebraic topology. The founder of that tendency was Henri Poincaré; during the 1930s it was developed by Lefschetz, Hodge and J. A. Todd. The modern synthesis brought together their work, that of the Henri Cartan school, and of W.L. Chow and Kunihiko Kodaira, with the traditional material.