Chaos in classical cosmology (II)
We present a new dynamical calculation about the Friedman-Robertson-Walker universe considered as an autonomous Hamiltonian. The time evolution of this Hamiltonian presents numerical instabilities so we apply a symplectic integration via infinitesimal canonical transformations of the phase space tim...
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Formato: | Capítulo de libro |
Lenguaje: | Inglés |
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Kluwer Academic Publishers-Plenum Publishers
1995
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001 | PAPER-3671 | ||
003 | AR-BaUEN | ||
005 | 20250210090414.0 | ||
008 | 190411s1995 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-0000568867 | |
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100 | 1 | |a Blanco, S. | |
245 | 1 | 0 | |a Chaos in classical cosmology (II) |
260 | |b Kluwer Academic Publishers-Plenum Publishers |c 1995 | ||
270 | 1 | 0 | |m Blanco, S.; Departamento de Física, FCEyN, Universidad de Buenos Aires, Pabellón I, Ciudad Universitaria, Buenos Aires, 1428, Argentina |
504 | |a Barrow, J.D., (1982) Phys. Rep., 85, p. 1 | ||
504 | |a Kolb, E., Turner, M.S., (1988) The Early Universe, , Addison-Wesley, New York | ||
504 | |a Belinsky, V.A., Grishchuk, L.P., Khalatnikov, I.M., Zel'dovich, (1985) Phys. Lett., 155 B, p. 232 | ||
504 | |a Amendola, L., Litterio, M., Occhionero, F., THE PHASE-SPACE VIEW OF INFLATION I: THE NON-MINIMALLY COUPLED SCALAR FIELD (1990) International Journal of Modern Physics A, 5, p. 3861 | ||
504 | |a Calzetta, E., El Hasi, C., (1993) Class. Quant. Grav., 10, p. 1825 | ||
504 | |a Calzetta, E., El Hasi, C., (1995) Phys. Rev., 51 E, p. 2713 | ||
504 | |a Blanco, S., Domenech, G., El Hasi, C., Rosso, O.A., (1994) Gen. Rel. Grav., 26, p. 1131 | ||
504 | |a Arnold, V.I., (1989) Mathematical Methods of Classical Mechanics, , 2nd. ed., Springer-Verlag, New York | ||
504 | |a Goldstein, H., (1980) Classical Mechanics, , 2nd. ed., Addison-Wesley, New York | ||
504 | |a Miller, R.H., (1993) J. Comp. Phys., 93, p. 469 | ||
504 | |a Misner, C.W., Thorne, K.S., Wheeler, J.A., (1973) Gravitation, , W. H. Freeman, San Francisco | ||
504 | |a Gutzwiller, M.C., (1990) Chaos in Classical and Quantum Mechanics, , Springer-Verlag, Berlin | ||
504 | |a Tabor, M., (1989) Chaos and Integrability in Nonlinear Dynamic, , Wiley, New York | ||
504 | |a Stolovistzky, G., Hernando, J.A., Resonant structure of integrable and near-integrable two-dimensional systems (1990) Physical Review A, 41 A, p. 3026 | ||
504 | |a Channell, P.J., Scovel, C., (1990) Nonlinearity, 3, p. 231 | ||
506 | |2 openaire |e Política editorial | ||
520 | 3 | |a We present a new dynamical calculation about the Friedman-Robertson-Walker universe considered as an autonomous Hamiltonian. The time evolution of this Hamiltonian presents numerical instabilities so we apply a symplectic integration via infinitesimal canonical transformations of the phase space time evolution that preserves the Poincaré invariant. In this way, we have also obtained a sensitive improvement in the accuracy of the Hamiltonian constraint, as well as in the computing time. We confirm our previous results; in a spatially closed universe, the route to chaos is reached by sucessive breakage of the resonant tori due to the action of 1:1 resonances. © 1995 Plenum Publishing Corporation. |l eng | |
593 | |a Departamento de Física, FCEyN, Universidad de Buenos Aires, Pabellón I, Ciudad Universitaria, Buenos Aires, 1428, Argentina | ||
593 | |a Instituto de Astronomía y Física del Espacio, C.C. 67 Suc. 28, Buenos Aires, 1428, Argentina | ||
593 | |a Instituto de Cálculo, FCEyN, Universidad de Buenos Aires, Pabellón II, Ciudad Universitaria, Buenos Aires, 1428, Argentina | ||
700 | 1 | |a Costa, Andrea | |
700 | 1 | |a Rosso, O.A. | |
773 | 0 | |d Kluwer Academic Publishers-Plenum Publishers, 1995 |g v. 27 |h pp. 1295-1307 |k n. 12 |p Gen Relat Gravit |x 00017701 |w (AR-BaUEN)CENRE-369 |t General Relativity and Gravitation | |
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