DYNAMICS OF MATTER IN A COMPACTIFIED KALUZA–KLEIN MODEL

Author:

LACQUANITI VALENTINO123,MONTANI GIOVANNI145

Affiliation:

1. International Center for Relativistic Astrophysics (ICRA), Physics Department (G9), University of Rome, "La Sapienza," Piazzale Aldo Moro 5, 00185 Rome, Italy

2. Physics Department "E. Amaldi," University of Rome, "Roma Tre," via della Vasca Navale 84, I-00146, Rome, Italy

3. LAPTH, 9, Chemin de Bellevue BP 110, 74941 Annecy Le Vieux Cedex, France

4. ENEA, C. R. Frascati (Department F.P.N.), via E. Fermi 45, I-00044, Frascati, Rome, Italy

5. ICRANET, C. C. Pescara, Piazzale della Repubblica 10, I-65100, Pescara, Italy

Abstract

A long-standing problem in Kaluza–Klein models is the description of matter dynamics. Within the 5D model, the dimensional reduction of the geodesic motion for a 5D free test particle formally restores electrodynamics, but the reduced 4D particle shows a charge–mass ratio that is upper-bounded, such that it cannot fit in with any kind of elementary particle. At the same time, from the quantum dynamics viewpoint, there is the problem of the generation of huge massive modes. We present a criticism against the 5D geodesic approach and face the hypothesis that in Kaluza–Klein space the geodesic motion does not deal with the real dynamics of the test particle. We propose a new approach: starting from the conservation equation for the 5D matter tensor, within the Papapetrou multipole expansion, we prove that the 5D dynamical equation differs from the 5D geodesic one. Our new equation provides right coupling terms without bounding and in such a scheme the tower of massive modes is removed.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

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