Abstract
The possibility that the present acceleration of the Universe is driven by a kind of viscous fluid is exploited. At background level this model is similar to the generalized Chaplygin gas model (GCGM). But, at the perturbative level, the viscous fluid exhibits interesting properties. In particular the oscillations in the power spectrum that plagues the GCGM are not present. Possible fundamental descriptions for this viscous dark energy are discussed.
References
Sahni, V.: Dark matter and dark energy. [astro-ph/0403324]
Padmanabhan, T.: Dark Energy: The Cosmological Challenge of the Millennium. [astro-ph/0411044]
Peebles, P.J.E., Ratra, B.: Rev. Mod. Phys. 75, 559 (2003)
Sahni V., Starobinsky, A.: Int. J. Mod. Phys. D 9, 373 (2000)
Lazkoz, R., Nesseris, S., Perivolaropoulos, L.: Evidence for cosmological oscillations in the Gold SnIa dataset. [astro-ph/0503230]
Bento, M.C., Bertolami, O., Santos, N.M.C., Sen, A.A.: Supernovae constraints on models of dark energy revisited. [astro-ph/0412638]
Padmanabhan, T.: Phys. Rep. 380, 235 (2003)
Carroll, S.M.: Living Rev. Rel. 4, 1 (2001)
Caldwell, R.R., Dave, R., Steinhardt, P.: Phys. Rev. Lett. 80, 1582 (1998)
Brax, Ph., Martin, J.: Phys. Rev. D 61, 103502 (2000)
Armendariz-Picon, C., Mukhanov, V., Steinhardt, P.J.: Phys. Rev. D 63, 103510 (2001)
Kamenshchik, A.Y., Moschella, U., Pasquier, V.: Phys. Lett. B 511, 265 (2001)
Fabris, J.C., Gonçalves, S.V.B., de Souza, e P.E.: Gen. Rel. Grav. 34, 53 (2002)
Bilic, N., Tupper, G.B., Viollier, R.D.: Phys. Lett. B 535, 17 (2002)
Bento, M.C., Bertolami, O., Sen, A.A.: Phys. Rev. D 66, 043507 (2002)
Sandvik, H., Tegmark, M., Zaldarriaga, M., Waga, I.: Phys. Rev. D 69, 123524 (2004)
Weinberg, S.: Gravitation and Cosmology. Wiley, New York (1972)
Murphy, G.L.: Phys. Rev. D8, 4231 (1973)
Pimentel, L.O.: Astrophys. Spac. Sci. 116, 395 (1985)
Arbab, A.I.: Nonstandard cosmology with constant and variable gravitational and variable cosmological “constants” and bulk viscosity. PhD thesis [gr-qc/0105027]
Chimento, L.P., Jakubi, A.S., Pavón, D.: Phys. Rev. 62, 063508 (2000)
Chimento, L.P., Jakubi, A.S., Pavón, D.: Phys. Rev. 67, 087302 (2003)
Zimdahl, W.: Phys. Rev. D 53, 5483 (1996)
Zimdahl, W.: Understanding cosmological bulk viscosity. [astro-ph/9602128]
Zimdahl, W.: Helv. Phys. Acta 69, 225 (1996)
Mak, M.K., Harko, T.: Int. J. Mod. Phys. D 12, 925 (2003)
Sen, A.A., Sen, S., Sethi, S.: Phys. Rev. D 63, 107501 (2001)
Cataldo, M., Cruz, N., Lepe, S.: Viscous dark energy and phantom evolution. [hep-th/0506153]
Eckart, C.: Phys. Rev. 58, 919 (1940)
Israel, W.: Ann. Phys. 100, 310 (1976)
Israel, W., Stewart, J.M.: Ann. Phys. 118, 341 (1979)
Colistete, R., Jr. Fabris, J.C.: Bayesian Analysis of the (Generalized) Chaplygin Gas and Cosmological Constant Models using the 157 gold SNe Ia Data. [astro-ph/0501519]
Landau, L., Lifchitz, E.: Mécanique des fluides. Mir, Moscou (1971)
Spergel, D.N., Steinhardt, P.J.: Phys. Rev. Lett. 84, 3760 (1999)
Barrow, J.D.: Phys. Lett. B 180, 335 (1986)
Barrow, J.D.: Nucl. Phys. B 310, 743 (1988)
Tegmark, M. et al.: Phys. Rev. D 69, 103501 (2004)
Padmanabhan, T.: Structure Formation in the Universe. Cambridge University Press, Cambridge (1993)
Vilenkin, A., Shellard, E.P.S., Landshoff, P.V.: Cosmic String and Other Topological Defects. Cambridge University Press, Cambridge (1994)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Fabris, J., Gonçalves, S. & Ribeiro, R.d. Bulk viscosity driving the acceleration of the Universe. Gen Relativ Gravit 38, 495–506 (2006). https://doi.org/10.1007/s10714-006-0236-y
Received:
Revised:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10714-006-0236-y