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Article: Numerical solution of time-dependent gravitational Schrodinger equation.
- Article from:
- Progress in Physics
- Article date:
- April 1, 2007
- Author:
CopyrightCOPYRIGHT 2007 Progress in Physics. This material is published under license from the publisher through the Gale Group, Farmington Hills, Michigan. All inquiries regarding rights should be directed to the Gale Group. (Hide copyright information)
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In recent years, there are attempts to describe quantization of planetary distance based on time-independent gravitational Schrodinger equation, including Rubcic & Rubcic's method and also Nottale's Scale Relativity method. Nonetheless, there is no solution yet for time-dependent gravitational Schrodinger equation (TDGSE). In the present paper, a numerical solution of time-dependent gravitational Schrodinger equation is presented, apparently for the first time. These numerical solutions lead to gravitational Bohr-radius, as expected. In the subsequent section, we also discuss plausible extension of this gravitational Schrodinger equation to include the effect of phion ...