Extension of Interesting Question I raised about 'Momentum' K of a Geodestic g at the J.A. Wheeler Astro physics School with possible numerical modeling of Deformations of Light Cones
Abstract
Description
I present the background of a question I asked Richard Matzner at the John Wheeler astrophysics school in Erice, at the Majorana institute of scientific culture during May 31st -June 8th. with an extension of the question to the issue of possible light cone deformation. This possibly has relevance to the stability of numerical algorithms used in modeling gravitational waves from Schwartzshield metric solutions of black holes and similar objects. This involves the so called momentum K of a geodestic g, with its re casting in a Kerr shield co ordinates of the Schwartzshield metric. for two black holes which have anti parallel spins but which exhibit spin coupling between them.
7 pages, no figures. Issue in part answered by Richard Matzner at a gathering in the Ettoire Majorana centre of scientific culture, May 31st- June 8th, in honor of J.A.Wheeler, with inclusion of a question showed Dr. Matzner but which was not answered by him due to time limitations in the gathering
7 pages, no figures. Issue in part answered by Richard Matzner at a gathering in the Ettoire Majorana centre of scientific culture, May 31st- June 8th, in honor of J.A.Wheeler, with inclusion of a question showed Dr. Matzner but which was not answered by him due to time limitations in the gathering