Asymptotic behavior of FRW cosmologies with many scalar fields

The dynamical evolution of FRW cosmologies conformally coupled to a finite set of scalar fields is studied. The scalar fields interact between them and we also consider a self-interaction term. lt is proved that when (Formula presented) and (Formula presented) only one physical asymptotic behavior i...

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Autor principal: Castagnino, Mario Alberto
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2002
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
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100 1 |a Castagnino, Mario Alberto 
245 1 0 |a Asymptotic behavior of FRW cosmologies with many scalar fields 
260 |c 2002 
504 |a Castagnino, M., Giacomini, H., Lara, L., (2000) Phys. Rev. D, 61, p. 107302 
504 |a Castagnino, M., Giacomini, H., Lara, L., (2001) Phys. Rev. D, 63, p. 44003 
504 |a Calzetta, E., El Hasi, C., (1993) Class. Quantum Grav., 10, p. 1825 
504 |a (1995) Phys. Rev. D, 51, p. 2713 
504 |a Bombelli, L., Castagnino, M., Lombardo, F., (1998) J. Math. Phys., 39, p. 6040 
504 |a (1999) Mod. Phys. Lett. A, 14, p. 537 
504 |a Amendola, L., Litterio, M., Occhionero, F., (1990) Int. J. Mod. Phys. A, 5, p. 3861 
504 |a Amendola, L., (2000) Phys. Rev. D, 62, p. 43511 
504 |a Gunzig, E., Faraoni, V., Figueiredo, A., Rocha Filho, T., Brenig, L., (2000) Class. Quantum Grav., 17, p. 1783 
504 |a Gunzig, E., Saa, A., Brenig, L., Figueiredo, A., Rocha Filho, T., (2001) Phys. Rev. D, 63, p. 67301 
504 |a Easther, R., Maeda, K., (1999) Class. Quantum Grav., 16, p. 1637 
504 |a Cornish, N., Lewin, J., (1996) Phys. Rev. D, 53, p. 3022 
504 |a Caldwell, R., Dave, R., Steinhard, P., (1998) Phys. Rev. Lett., 80, p. 1582 
504 |a Chirikov, B.V., (1979) Phys. Rep., 52, p. 265 
504 |a S. Strogatz, Nonlinear Dynamics and Chaos (Addison-Wesley, New York, 1994); E. Atlee Jackson, Perspectives of Nonlinear Dynamics (Cambridge University Press, Cambridge, England, 1991) 
506 |2 openaire  |e Política editorial 
520 3 |a The dynamical evolution of FRW cosmologies conformally coupled to a finite set of scalar fields is studied. The scalar fields interact between them and we also consider a self-interaction term. lt is proved that when (Formula presented) and (Formula presented) only one physical asymptotic behavior is possible: the radius of the universe expands forever. When (Formula presented) either we have the just described behavior or the universe will ultimately collapse in a finite time. But we also give evidence that an oscillatory chaotic behavior is possible in this case if a fine-tuning between the initial conditions is satisfied. © 2001 The American Physical Society.  |l eng 
593 |a Instituto de Astronomia y Fisica del Espacio, Casilla de Correos 67, Sucursal 28, Buenos Aires, 1428, Argentina 
593 |a Laboratoire de Mathematique et Physique Theorique, CNRS (UPRES-A6083), Universite de Tours-Parc de Grandmont, Tours, 37200, France 
593 |a Departamento de Fisica, FCEIA, UNR, Av. Pellegini 250, Rosario, 2000, Argentina 
773 0 |d 2002  |g v. 65  |k n. 2  |p Phys Rev D Part Fields Gravit Cosmol  |x 15507998  |t Physical Review D - Particles, Fields, Gravitation and Cosmology 
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