2 0 M ay 2 00 4 Hilbert ’ s “ World Equations ” and His Vision of a Unified Science ∗
نویسنده
چکیده
In summer 1923, a year after his lectures on the ‘New Foundation of Mathematics’ and half a year before the republication of his two notes on the ‘Foundations of Physics,’ Hilbert delivered a trilogy of lectures in Hamburg. In these lectures, Hilbert expounds in an unusually explicit manner his epistemological perspective on science as a subdiscipline of an all embracing science of mathematics. The starting point of Hilbert’s considerations is the claim that the class of gravitational and electromagnetic field equations implied by his original variational formulation of 1915 provides valid candidate ‘world equations,’ even in view of attempts at unified field theories á la Weyl and Eddington based on the concept of the affine connection. We give a discussion of Hilbert’s lectures and, in particular, examine his claim that Einstein in his 1923 papers on affine unified field theory only arrived at Hilbert’s original 1915 theory. We also briefly comment on Hilbert’s philosophical viewpoints expressed in these lectures.
منابع مشابه
Bessel Type Inequalities in Hilbert C-modules
X iv :0 90 5. 40 67 v1 [ m at h. FA ] 2 5 M ay 2 00 9 BESSEL TYPE INEQUALITIES IN HILBERT C-MODULES S. S. DRAGOMIR, M. KHOSRAVI AND M. S. MOSLEHIAN Abstract. Regarding the generalizations of the Bessel inequality in Hilbert spaces which are due to Bombiari and Boas–Bellman, we obtain a version of the Bessel inequality and some generalizations of this inequality in the framework of Hilbert C∗-mo...
متن کاملar X iv : m at h - ph / 0 40 50 01 v 1 3 M ay 2 00 4 A nonlinear singular perturbation problem
Let F (u ε) + ε(u ε − w) = 0 (1) where F is a nonlinear operator in a Hilbert space H, w ∈ H is an element, and ε > 0 is a parameter. Assume that F (y) = 0, and F ′ (y) is not a boundedly invertible operator. Sufficient conditions are given for the existence of the solution to (1.1) and for the convergence lim ε→0 u ε − y = 0. An example of applications is considered. In this example F is a non...
متن کامل2 00 5 Einstein , Hilbert and Equations of Gravitation
• The history of the equations of gravitational field is of particular interest because they are related to two famous names: Albert Einstein and David Hilbert, and because the circumstances of their invention bear sometimes almost detective character. One of the early references is the book " Einstein, Hilbert and the Theory of Gravitation " by a renowned historian of science J. Mehra [1], whe...
متن کامل. pl as m - p h ] 1 4 M ay 2 00 5 Two - fluid tokamak equilibria with reversed magnetic shear and sheared flow 1
X iv :p hy si cs /0 50 51 01 v1 [ ph ys ic s. pl as m -p h] 1 4 M ay 2 00 5 Two-fluid tokamak equilibria with reversed magnetic shear and sheared flow 1 G. Poulipoulis, G. N. Throumoulopoulos, H. Tasso University of Ioannina, Association Euratom Hellenic Republic, Section of Theoretical Physics, GR 451 10 Ioannina, Greece Max-Planck-Institut für Plasmaphysik, Euratom Association, D-85748 Garchi...
متن کاملar X iv : m at h / 00 12 25 1 v 2 [ m at h . A G ] 3 0 M ay 2 00 1 Euler Characteristics of Theta Divisors of Jacobians for Spectral Curves
We show how to calculate the Euler characteristic of an affine Jacobi variety of a spectral curve from its defining equations. 0 Membre du CNRS 1 Laboratoire associé au CNRS.
متن کامل