Mathematics
Scientist
Antwerpen, Universitaire Instelling, Antwerp, Belgium; Queen Mary College, London, England
School of Mathematical Sciences, Queen Mary College, University of London; Physics Department, Universitaire Instelling
Antwerpen, Universitaire Instelling, Wilrijk, Belgium
Department Chimie Phys., Univ. Libre de Bruxelles, Belgium
Department of Phys., Univ. Instelling Antwerpen, Antwerpen, Belgium
Department of Appl. Math., Waterloo Univ., Ont., Canada
Department Chim.-Phys., Univ. Libre de Bruxelles, Belgium
Theoretical Astronomy Unit, School of Mathematical Sciences, Queen Mary College; Physics Department, Universitaire Instelling Antwerpen
Faculty of Applied Sciences, University of Gent, Jozef Plateaustraat 22, 9000 Gent, Belgium
Faculteit Toegepaste Wetenschappen, 9000 Gent, Belgium
Department of Applied Mathematics, University of Waterloo
Sch. of Math. Sci., Queen Mary & Westfield Coll., London, UK
Department Chimie-Phys., Univ. Libre de Bruxelles, Belgium
Universitaire Instetting Antwerpen
Queen Mary College, London, England; Antwerpen, Instelling Universitaire, Antwerp, Belgium
Faculty of Applied Sciences TW16, Gent University, Galglaan 2, 9000 Gent, Belgium
Department Natuurkunde, Antwerp Univ., Belgium
Department of Physics, University of Antwerp
Brussel, Vrije Universiteit, Brussels, Belgium
Astrofys. Inst., Vrije Univ. Brussel, Belgium
Antwerpen, Universitaire Instelling, Antwerp, Belgium
Service Chim.-Phys., Univ. Libre de Bruxelles, Belgium
Department of Mathematical Analysis IW16, Ghent University, Galglaan 2, 9000 Ghent, Belgium
Physics Department, Universitaire Instelling Antwerpen, B-2610 Antwerp, Belgium
Service Chimie-Physique, Université Libre de Bruxelles
Department of mathematical analysis, University of Ghent, Galglaan 2, Gent 9000, Belgium
A case of dual interpretation of Einstein-Maxwell fields.
A class of inhomogeneous cosmological models with separable metrics
A qualitative discussion of the Wils inhomogeneous stiff fluid cosmologies
Charged scalar-tensor spheres - General solutions
Classification Results on Purely Magnetic Perfect Fluid Models
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