Enlarged quintessence cosmology

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We show that the combination of a fluid with a bulk dissipative pressure and quintessence matter can simultaneously drive an accelerated expansion phase and solve the coincidence problem of our current Universe. We then study some scenarios compatible with the observed cosmic acceleration. ©2000 The...

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Autor principal: Chimento, L.P
Otros Autores: Jakubi, A.S, Pavón, D.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2000
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Chimento, L.P. 
245 1 0 |a Enlarged quintessence cosmology 
260 |c 2000 
270 1 0 |m Chimento, L.P.; Departamento de fi'Sica, Universidad de Buenos Aires, 142S Buenos Aires, Argentina; email: chimento@df.uba.ar 
506 |2 openaire  |e Política editorial 
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520 3 |a We show that the combination of a fluid with a bulk dissipative pressure and quintessence matter can simultaneously drive an accelerated expansion phase and solve the coincidence problem of our current Universe. We then study some scenarios compatible with the observed cosmic acceleration. ©2000 The American Physical Society.  |l eng 
593 |a Departamento de fi'Sica, Universidad de Buenos Aires, 142S Buenos Aires, Argentina 
593 |a Departament de Fisica, Universidad Autónoma de Barcelona, 08193 Bellaterra, Spain 
700 1 |a Jakubi, A.S. 
700 1 |a Pavón, D. 
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