Dissipative cosmological solutions

The exact general solution to the Einstein equations in a homogeneous Universe with a full causal viscous fluid source for the bulk viscosity index m = 1/2 is found. We have investigated the asymptotic stability of Friedmann and de Sitter solutions, the former is stable for m ≥ 1/2 and the latter fo...

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Autor principal: Chimento, L.P
Otros Autores: Jakubi, A.S
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 1997
Acceso en línea:Registro en Scopus
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100 1 |a Chimento, L.P. 
245 1 0 |a Dissipative cosmological solutions 
260 |c 1997 
270 1 0 |m Chimento, L.P.; Departamento de Física, Fac. de Ciencias Exactas y Naturales, Pabellón I, 1428 Buenos Aires, Argentina 
506 |2 openaire  |e Política editorial 
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504 |a Chimento, L.P., Jakubi, A.S., (1993) Class. Quantum Grav., 10, p. 2047 
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504 |a Belinskii, V.A., Nikomarov, E.S., Khalatnikov, I.M., (1979) Sov. Phys.-JETP, 50, p. 213 
504 |a Chimento, L.P., Two scalar field cosmologies (1996) Proc. 1st Mexican School on Gravitation and Mathematical Physics (1994), , Singapore: World Scientific 
504 |a Chimento, L.P., (1996) J. Math. Phys., , at press 
504 |a Aguirregabiria, J.M., Chimento, L.P., (1996) Class. Quantum Grav., 13, p. 3197 
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520 3 |a The exact general solution to the Einstein equations in a homogeneous Universe with a full causal viscous fluid source for the bulk viscosity index m = 1/2 is found. We have investigated the asymptotic stability of Friedmann and de Sitter solutions, the former is stable for m ≥ 1/2 and the latter for m ≤ 1/2. The comparison with results of the truncated theory is made. For m = 1/2, it was found that families of solutions with extrema no longer remain in the full case and they are replaced by asymptotically Minkowski evolutions. These solutions are monotonic.  |l eng 
593 |a Departamento de Física, Fac. de Ciencias Exactas y Naturales, Pabellón I, 1428 Buenos Aires, Argentina 
700 1 |a Jakubi, A.S. 
773 0 |d 1997  |g v. 14  |h pp. 1811-1820  |k n. 7  |p Classical Quantum Gravity  |x 02649381  |w (AR-BaUEN)CENRE-326  |t Classical and Quantum Gravity 
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