Stable inflationary dissipative cosmologies

The stability of the de Sitter era of cosmic expansion in spatially curved homogeneous isotropic universes is studied. The source of the gravitational field is an imperfect fluid such that the parameters that characterize it may change with time. In this way we extend our previous analysis for spati...

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Autor principal: Chimento, L.P
Otros Autores: Jakubi, A.S, Pavon, D.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: World Scientific Publishing Co. Pte Ltd 2000
Acceso en línea:Registro en Scopus
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100 1 |a Chimento, L.P. 
245 1 0 |a Stable inflationary dissipative cosmologies 
260 |b World Scientific Publishing Co. Pte Ltd  |c 2000 
270 1 0 |m Chimento, L.P.; Departamento de Física, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina; email: chimento@df.uba.ar 
506 |2 openaire  |e Política editorial 
504 |a Chimento, L.P., Jakubi, A., Pavón, D., (1999) Class. Quantum Grav., 16, p. 1625 
504 |a Israel, W., (1976) Ann. Phys. N.Y., 100, p. 310 
504 |a Pavón, D., Jou, D., Casas-Vázquez, (1982) Ann. Inst. H. Poincaré, A36, p. 79. , J 
504 |a Hiscock, W.A., Lindblom, L., (1983) Ann. Phys. N.Y., 151, p. 466 
504 |a Hiscock, W.A., Lindblom, L., (1988) Contemporary Mathematics, 71, p. 181 
504 |a Barrow, J.D., (1988) Nucl. Phys., B310, p. 743 
504 |a Barrow, J.D., (1990) The Formation and Evolution of Cosmic Strings, , ed G. W. Gibbons, S. W. Hawking and T.Vachaspati Cambridge University Press, Cambridge 
504 |a Eckart, C., (1940) Phys. Rev., 58, p. 919 
504 |a Bartelmann, M., (1998) Astron. Astrophys., 330, p. 1 
504 |a Silk, J., Seven Paradigms in Structure Formation, , Report astro-ph/9903402 
504 |a Coble, K., Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Pithon V Results, , Report astro-ph/9902195 
504 |a Pavón, D., Bafaluy, J., Jou, D., (1991) Class. Quantum Grav., 8, p. 347 
504 |a Chimento, L.P., Jakubi, A.S., (1993) Class. Quantum Grav., 10, p. 2047 
504 |a Maartens, R., (1997) Hanno Rund Workshop on Relativity and Thermodynamics, , ed. S. D. Maharaj Natal University, Natal, Report astro-ph/9609119 
504 |a Zimdahl, W., (1996) Phys. Rev., D53, p. 5483 
504 |a Chimento, L.P., Jakubi, A.S., (1997) Class. Quantum Grav., 14, p. 1811 
504 |a Cesari, L., (1963) Asymptotic Behavior and Stability Problems in Ordinary Differential Equations, , Springer, Berlin 
504 |a Chimento, L.P., Jakubi, A.S., (1996) Proc. First Mexican School on Gravitation and Mathematical Physics, , World Scientific, Singapore 
504 |a Zimdahl, W., Pavón, D., Maartens, R., (1997) Phys. Rev., D55, p. 4681 
504 |a Zimdahl, W., Pavón, D., (1998) Phys. Rev., D58, p. 103506 
504 |a Zimdahl, W., Pavón, D., (1993) Phys. Lett., A176, p. 57 
504 |a Gross, D., Perry, M.J., Yaffe, L.G., (1982) Phys. Rev., D25, p. 330 
504 |a Kapusta, J.I., (1984) Phys. Rev., D30, p. 831 
504 |a Chimento, L.P., (1997) J. Math. Phys., 38, p. 2565 
504 |a Hu, B.L., (1982) Phys. Lett., A90, p. 375 
504 |a Zel'dovich, Y.B., (1970) JETP Lett., 12, p. 307 
520 3 |a The stability of the de Sitter era of cosmic expansion in spatially curved homogeneous isotropic universes is studied. The source of the gravitational field is an imperfect fluid such that the parameters that characterize it may change with time. In this way we extend our previous analysis for spatially-flat spaces as well as the work of Barrow.  |l eng 
593 |a Departamento de Física, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina 
593 |a Departament de Física, Univ. Autónoma de Barcelona, 08193 Bellaterra, Spain 
700 1 |a Jakubi, A.S. 
700 1 |a Pavon, D. 
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