Related papers: Classical limit of the Kepler problem and the cont…
This paper has been withdrawn.
This paper has been withdrawn due to an incorrect analysis in Section 4.
This paper has been withdrawn pending discussions
This paper has been withdrawn by the author, since the author does not have enough time to answer every questions on this result.
This paper has been withdrawn by the author due to a crucial error in eq.59. I apologize for the inconveniences.
This paper has been withdrawn because the content has been substantially improved in a later paper, arXiv:0806.1165.
Paper withdrawn by the author.
This paper has been withdrawn. A much-improved version can be found at hep-ph/0209176.
The original version of this paper has been withdrawn by the authors and merged with the revised version of astro-ph/9702014.
We derive the gravitational and electrostatic self-energies of a particle at rest in the background of a cosmic dispiration (topological defect), finding that the particle may experience potential steps, well potentials or potential…
This paper is withdrawn.
This paper has been withdrawn by the author due to inconsistency of the considered working hypothesis. The consistent treatment is presented in the last publications of the author.
For a quantum observable $A_\hbar$ depending on a parameter $\hbar$ we define the notion ``$A_\hbar$ converges in the classical limit''. The limit is a function on phase space. Convergence is in norm in the sense that $A_\hbar\to0$ is…
This paper has been withdrawn
This paper has been withdrawn by the author.
This is in fact an Erratum to the paper published in Physics Letters A221 (1996) 359. The reduced-phase-space discussion remains essentially valid in spite of the fact that many equations are changed. However, the analysis based on the…
This paper has been withdrawn by the authors due to numerical problems to get viable results.
This paper has been withdrawn at the request of one of the authors.
Paper withdrawn due to an error into the equations of the probability amplitudes.
The kinematical phase space of classical gravitational field is flat (affine) and unbounded. Because of this, field variables may tend to infinity leading to appearance of singularities, which plague Einstein's theory of gravity. The…