Local constraints on the oscillating G model

Physical Review D

Volumn 64, Issue 4, 2001, Pages

  González, José A ^a   Quevedo, Hernando ^a   Salgado, Marcelo ^a   Sudarsky, Daniel ^a  

^a INSTITUTO DE CIENCIAS NUCLEARES   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; GRAVITY; MATHEMATICAL MODEL; OSCILLATION; PERIODICITY;

EID: 0035881893     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.64.047504     Document Type: Article

References (22)

1. A.H. Guth, Phys. Rev. D 23, 347 (1981);
2. A. Linde, Phys. Lett. 108B, 389 (1982).
3. P. de Berdarnis et al., Nature (London) 404, 955 (2000);
4. S. Hanany et al., Astrophys. J. Lett. 545, L5 (2000);
5. A.G. Riess et al., Astron. J. 116, 1009 (1998);
6. S. Perlmutter et al., Astrophys. J. 517, 565 (1999).
7. T. Broadhurst, R. Ellis, D. Koo, and A. Szalay, Nature (London) 343, 726 (1990);
8. A. Szalay, R. Ellis, D. Koo, and T. Broadhurst, in Primordial Nucleosynthesis and Evolution of the Universe, edited by K. Sato and J. Audouze (Kluwer, Dordrecht, 1991), p. 435.
9. A. Szalay, T.J. Broadhurst, N. Ellman, D.C. Koo, and R.S. Ellis, Proc. Natl. Acad. Sci. U.S.A. 90, 4853 (1993).
10. J.A. Gonzalez, H. Quevedo, M. Salgado, and D. Sudarsky, Astron. Astrophys. 362, 835 (2000).
11. M. Salgado, D. Sudarsky, and H. Quevedo, Phys. Rev. D 53, 6771 (1996).
12. M. Salgado, D. Sudarsky, and H. Quevedo, Phys. Lett. B 408, 69 (1997).
13. H. Quevedo, M. Salgado, and D. Sudarsky, Astrophys. J. 488, 14 (1997).
14. D. Sudarsky, H. Quevedo, and M. Salgado, Rev. Mex. F́s. 43, 699 (1997).
15. M. Morikawa, Astrophys. J. Lett. 362, L37 (1990).
16. BD>3000, in accordance with more recent observations
17. [C. Will (private communication)].
18. H. Quevedo, M. Salgado, and D. Sudarsky, Gen. Relativ. Gravit. 31, 767 (1999).
19. Obviously we cannot neglect the photon contribution when we evolve the equations backward in time in order to recover the nucleosynthesis predictions.
20. C. Copi, D.N. Schram, and M.S. Turner, Science 267, 192 (1995).
21. R.G. Crittenden, and P.J. Steinhardt, Astrophys. J. 395, 360 (1992).
22. L.M. Krauss, Phys. Rep. 333-334, 33 (2000).