1997/03/21 by Bang‐Yen Chen, L. Demopoulos, Joeri Van der Veken +1
Physics and Astronomy · #Antisymmetric relation #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #Field (mathematics) #Gravitation #Gravitational collapse #Gravitational field #Mathematical physics #Physical chemistry #Physics #Pure mathematics #Relativity and Gravitational Theory #Simple (philosophy) #Space (punctuation) #Space time #Theoretical physics #gr-qc
paper · pdf · doi:10.1088/0264-9381/24/3/003
published as Class.Quant.Grav.24:551-564,2007 · REVTeX 3.0 with epsf macros and AMS symbols, 3 pages, 1 figure
arxiv created 1997/03/21 · openalex publication_date 2006/12/19 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We consider a simple, physical approach to the problem of marginally trapped surfaces in the Nonsymmetric Gravitational Theory (NGT). We apply this approach to a particular spherically symmetric, Wyman sector gravitational field, consisting of a pulse in the antisymmetric field variable. We demonstrate that marginally trapped surfaces do exist for this choice of initial data.