Constraining a bulk viscous matter-dominated cosmological model using SNe Ia, CMB and LSS

AIP Conference Proceedings

Volumn 1026, Issue , 2008, Pages 300-301

  Avelino, Arturo ^a   Nucamendi, U ^a   Guzman F S ^a  

^a UNIVERSIDAD MICHOACANA DE SAN NICOLÁS DE HIDALGO   (Mexico)

Author keywords

BAO; Bulk viscosity; CMB; Dark energy; Supernovae

Indexed keywords

EID: 51149106109     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.2965067     Document Type: Conference Paper

References (11)

1. C. W. Misner et al., Gravitation, W. H. Freeman and Company, 1973, pp. 557-568.
2. J. C. Fabris, S. V. B. Goncalves, and R. de Sa Ribeiro, Gen. Rel. Grav 38, 495-506 (2006).
3. A. Avelino, and U. Nucamendi, in preparation (2008).
4. R. Colistete et. al., Phys. Rev. D 76, 103516, 1-13 (2007).
5. J. Ren, and X.-H. Meng, Phys. Lett. B 633, 1-8 (2006).
6. A. G. Riess et al., arXiv:astro-ph/0611572v2 (2006).
7. M. Turner, and A. G. Riess, Astrophysical journal 569, 18 (2002).
8. A. G. Riess et al., Astrophysical journal 607, 665-687 (2004).
9. A. Melchiorri et al., Phys. Rev. D 68, 043509 (2003).
10. Y. Wang, and P. Mukherjee, Astrophysical journal 650, 1-6 (2006).
11. D. J. Eisenstein et al., Astrophysical journal 633, 560-574 (2005).