Cosmological models arising from generalized scalar field potentials

We find exact solutions for isotropic cosmological models containing a self-interacting scalar field possessing an interaction potential of a general class. In particular, we consider the combination of exponential potentials arising from a perturbation expansion in superstring theories. We also con...

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Autor principal: Chimento, L.P
Otros Autores: Méndez, V., Zuccalá, N.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 1999
Acceso en línea:Registro en Scopus
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100 1 |a Chimento, L.P. 
245 1 0 |a Cosmological models arising from generalized scalar field potentials 
260 |c 1999 
270 1 0 |m Chimento, L.P.; Departamento de Física, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina 
506 |2 openaire  |e Política editorial 
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504 |a Chimento, L.P., Cossarini, A.E., Zuccalá, N.A., (1998) Class. Quantum Grav., 15, p. 57 
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520 3 |a We find exact solutions for isotropic cosmological models containing a self-interacting scalar field possessing an interaction potential of a general class. In particular, we consider the combination of exponential potentials arising from a perturbation expansion in superstring theories. We also consider a general class of potentials that give rise to power-law and polynomial chaotic inflation, as well as the intermediate inflationary models. We compute the scalar and tensor perturbations produced in those models and use the exact solutions obtained to examine the consistency of the first-order slow-roll expansion.  |l eng 
593 |a Departamento de Física, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina 
593 |a Facultat de Ciencies de la Salut, Univ. Internacional de Catalunya, c/gomera s/n. Sant Cugat del Valles, 08190 Barcelona, Spain 
700 1 |a Méndez, V. 
700 1 |a Zuccalá, N. 
773 0 |d 1999  |g v. 16  |h pp. 3749-3763  |k n. 11  |p Classical Quantum Gravity  |x 02649381  |w (AR-BaUEN)CENRE-326  |t Classical and Quantum Gravity 
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