FP6Individual fellowship2005–2007

IDEA · Integrable difference equations and their applications

FP6 — Marie Curie Actions (Human Resources and Mobility)

Duration
2005-04-01 → 2007-03-31
EU contribution
€161,995
Participants
1
Scheme
EIF

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Results in brief

Final Activity Report Summary - IDEA (Integrable Difference Equations and their Applications)

Since antiquity people asked the question whether the substance of the universe was discrete or continuous. It is a paradox that corpuscle theory in the Newtonian approach led to the development of differential equations by demanding the notion of continuity in their definition. In contrast, the theory of difference, i.e. discrete, equations remains a less developed subject, even in this day and age, in spite of the recent explosion of interest in this theory which was caused by its significance for computer science and information technology. The subject of the project lied on the interface between the theory of discrete equations on the one hand and the theory of nonlinear integrable equations on the other. In the domain of differential equations such systems were often referred to as soliton equations, which once again highlighted an interesting connection with corpuscle theory, since solitons are particle-like solutions of nonlinear partial differential equations which remarkably also exhibit particle-like collision properties. In the discrete domain, analogues of systems exhibiting such solutions were developed in the past two decades and these discoveries very much brought back the issue of difference equations into the limelight. The main objective of the project was to develop further the theory of nonlinear integrable difference equations and push them in the direction of equations relevant to the theory of gravity, i.e. Einstein’s theory of general relativity, where under special circumstances the governing equations were known to be integrable, such as the celebrated Ernst equation which described gravitational waves. One of the main guiding principles of relativity is the freedom of changing the variables entering the equations, and this principle has been a major deficiency of the discrete theory. The most important achievement of the project was related to this issue. We showed how to compensate the apparent lack of possibility to changing the independent variables in the case of difference integrable equations. This would eventually make possible the raise of the discrete theory, by means of integrable examples, to the same level as the continuous theory, in the ultimate endeavour to build a fundamental theory describing the physics of discrete space-time.

Data: CORDIS, © European Union

Project objective

In the past decade the theory of discrete integrable systems described by difference equations has emerged as the most prominent direction of research within the field of integrability. The study of difference equations constituting the exact analogues of integrable differential equations have fundamentally contributed to mathematics by opening new fields of research, e.g. in difference geometry and the theory of non-linear special functions.This proposal concerns both linear difference equations that possess a class of Darboux symmetry transformations and non-linear difference equations that are compatibility conditions for a set of the linear equations. Whilst most of the activity in the field has concentrated on equations of hyperbolic type, the emphasis of the proposal lies in the study of equations of elliptic type, which forms almost unchartered territory, although importantly first paradigms in this direction has been constructed by the applicant. The structure of integrable difference equations of the latter type is expected to be richer, and thus more fundamental, than of their continuous counterparts, and this will form the principal object of investigation.In particular, this project endeavours to find discrete (difference) integrable analogues of the equations that describe:i) Axisymmetric, stationary, vacuum Einstein fields (Ernst equation),ii) stationary, vacuum Einstein-Maxwell fields (Ernst-Maxwell-Weyl equations), both through the consideration of auto-Backlund and Darboux transformations.An important problem is the question of classification of such systems. Experience with discrete systems suggests that this problem is tractable and can be formulated in a precise way. To resolve this problem the theory of reductions of discrete integrable systems will be further developed. An aim is to gain insight in integrable reductions of Einstein's equations of General Relativity, using discrete Ernst equations as toy model of discrete gravity.

Original text from CORDIS.

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Data: CORDIS, © European Union