Classical supersymmetric matter and cosmology
We show that supersymmetry may play an important role in giving a reasonable explanation of relevant cosmological features. We work in a classical N=1 supergravity scenario showing that supersymmetric matter leads, in the classical limit, to a fluid model acting as the source of the gravitational fi...
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Kluwer Academic Publishers-Plenum Publishers
1991
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024 | 7 | |2 scopus |a 2-s2.0-0011030250 | |
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100 | 1 | |a Domenech, Graciela | |
245 | 1 | 0 | |a Classical supersymmetric matter and cosmology |
260 | |b Kluwer Academic Publishers-Plenum Publishers |c 1991 | ||
270 | 1 | 0 | |m Domenech, G.; Institute de Astronomía y Física del Espacio (CONICET), C.C.67, Suc. 28, Buenos Aires, 1428, Argentina |
504 | |a La, D., Steinhardt, J., (1989) Phys. Rev. Lett., 62, p. 376 | ||
504 | |a Prigogine, L., Geheniau, J., Gunzig, E., Nardone, P., (1989) Gen. Rel. Grav., 21, p. 767 | ||
504 | |a Domenech, G., Levinas, M., Umérez, N., (1989) Phys. Lett., 137 A, p. 17 | ||
504 | |a Castagnino, M., Domenech, G., Levinas, M., Umérez, N., (1989) Class. Quant. Grav., 6, p. L1 | ||
504 | |a Green, M., Schwarz, J., Witten, E., (1987) Superstring Theory, , Cambridge University Press, Cambridge | ||
504 | |a van Nieuwenhuizen, P., (1981) Phys. Rep., 68, p. 189 | ||
504 | |a Weinberg, S., (1972) Gravitation and Cosmology, , Wiley, New York | ||
504 | |a Castagnino, M., Domenech, G., Levinas, M., Umérez, N., (1986) Phys. Lett., 179 B, p. 83 | ||
504 | |a Brandenberger, R., (1985) Rev. Mod. Phys., 57, p. 1 | ||
506 | |2 openaire |e Política editorial | ||
520 | 3 | |a We show that supersymmetry may play an important role in giving a reasonable explanation of relevant cosmological features. We work in a classical N=1 supergravity scenario showing that supersymmetric matter leads, in the classical limit, to a fluid model acting as the source of the gravitational field. The equation of state arises, in a natural way, as a consequence of the field equations. We study conditions for the matter dominated era and the existence of an inflationary solution. Using upper bounds of several red-shift experimental results we are able to give an estimate of the corresponding Hubble constant. © 1991 Plenum Publishing Corporation. |l eng | |
593 | |a Institute de Astronomía y Física del Espacio (CONICET), C.C.67, Suc. 28, Buenos Aires, 1428, Argentina | ||
593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Argentina | ||
593 | |a Departamento de Matemática, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Argentina | ||
700 | 1 | |a Levinas, M. | |
700 | 1 | |a Umérez, N. | |
773 | 0 | |d Kluwer Academic Publishers-Plenum Publishers, 1991 |g v. 23 |h pp. 683-690 |k n. 6 |p Gen Relat Gravit |x 00017701 |w (AR-BaUEN)CENRE-369 |t General Relativity and Gravitation | |
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