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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Formato: | Capítulo de libro |
Lenguaje: | Inglés |
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2002
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024 | 7 | |2 scopus |a 2-s2.0-85038266643 | |
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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 | ||
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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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856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.65.023509 |x doi |y DOI |
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