A5 - Radiative spacetimes and approximation methods

Summary

Introduction

The workshop consisted of an introductory overview and of seven specialized talks. The talks were selected among twenty-five submitted abstracts and were presented in an order consistent with the three subsequently discussed categories, i.e. from rigourous mathematical results about approximation methods, to definition of approximation methods, to physical results obtained by approximation methods. This order was chosen to emphasize the following easily forgotten fact. Ideally, physics should connect the mathematical axioms defining our theories to the results of observations or experiments by means of a tight chain of deductions. However, in practice, this chain of deductions often contains gaps, and one of the main sources of gaps lies in the use of mathematically ill justified approximation methods as substitutes for the exact theories. In order to bridge the latter gap one needs, on the one hand, some clear algorithmic definition of the approximation methods used together with a formal study of the structure of its successive terms, and, on the other hand, mathematical theorems proving that the formal sequence defined by the ‘approximation method’ is either convergent, or asymptotic, to some exact solution. Progress on both aspects has recently been obtained, and has been reported, or quoted, during the workshop.

Talks presented at the workshop fell into three categories. Talks on mathematical results about approximation methods showed instances where the conceptually important gap between mathematics and the use of approximation methods by physicists can be closed, or narrowed.