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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Autor principal: Domenech, Graciela
Otros Autores: Levinas, M., Umérez, N.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Kluwer Academic Publishers-Plenum Publishers 1991
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
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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. 
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