Noninteracting dark matter

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 60, Issue 10, 1999, Pages

  Vilenkin, A ^b  

^a INSTITUTE FOR ADVANCED STUDY   (United States)

^b TUFTS UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 18144381081     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.103506     Document Type: Article

References (36)

1. D. J. Eisenstein, W. Hu, and M. Tegmark, Astrophys. J. (to be published), and references therein.
2. G.E.A. Matsas, J.C. Montero, V. Pleitez, and D.A.T. Vanzella, in Conference on Topics in Theoretical Physics II - Festschrift for A.H. Zimerman, edited by H. Aratyn, J.H. Ferreira and J.F. Gomes (Instituto de Fisica Teorica, Sao Paulo, 1998), p. 219.
3. A. Vilenkin, Phys. Rev. D 27, 2848 (1983).
4. A.A. Starobinsky, in Field Theory, Quantum Gravity and Strings, edited by H.J. de Vega and N. Sanchez (Springer, Heidelberg, 1986).
5. A.A. Starobinsky and J. Yokoyama, Phys. Rev. D 50, 6357 (1994).
6. L. Kofman and A.D. Linde, Nucl. Phys. B282, 555 (1987).
7. P.J.E. Peebles and A. Vilenkin, Phys. Rev. D 59, 063505 (1999).
8. G. Felder, L. Kofman, and A. D. Linde, Phys. Rev. D 60, 103505 (1999).
9. The one-loop effective potential for the model (1) in de Sitter space was calculated in Ref. 10. Condition (4) is obtained by requiring that the one-loop correction is negligible for (Formula presented), where the expectation value (Formula presented) is taken in the de Sitter–invariant state (see Sec. III).
10. A. Vilenkin, Nucl. Phys. B226, 504 (1983).
11. E. Gaztañaga and P. Fosalba, Mon. Not. R. Astron. Soc. 301, 534 (1998)
12. M. White, astro-ph/9811227
13. J.A. Frieman and E. Gaztañaga, astro-ph/9903423.
14. A.D. Linde, Particle Physics and Inflationary Cosmology (Harwood Academic, Chur, 1990).
15. L.H. Ford, Phys. Rev. D 35, 2955 (1987).
16. P.B. Greene, L. Kofman, A. Linde, and A.A. Starobinsky, Phys. Rev. D 56, 6175 (1997).
17. J. Ellis, Nucl. Phys. B373, 399 (1992).
18. L. Randall and S. Thomas, Nucl. Phys. B449, 229 (1995).
19. D.H. Lyth and E.D. Stewart, Phys. Rev. Lett. 75, 201 (1995).
20. G. Dvali, Phys. Lett. B 355, 78 (1995).
21. M. Dine, L. Randall, and S. Thomas, Phys. Rev. Lett. 75, 398 (1995).
22. T. Damour and A. Vilenkin, Phys. Rev. D 53, 2981 (1996).
23. M. Dine, W. Fischler, and D. Nemeschansky, Phys. Lett. 136B, 169 (1984).
24. A.D. Linde, Phys. Rev. D 53, 4129 (1996).
25. G. Dvali and Z. Kakushadze, Phys. Lett. B 417, 50 (1998).
26. I. Antoniadis, S. Dimopoulos, and G. Dvali, Nucl. Phys. B516, 70 (1998).
27. L.P. Grishchuk and A.D. Popova, Zh. Éksp. Teor. Fiz. 77, 1665 (1979) [Sov. Phys. JETP 50, 835 (1979)].
28. This point was also noted by FKL in the revised version of their paper. We are grateful to Lev Kofman for pointing this out to us.
29. A. Linde and V. Mukhanov, Phys. Rev. D 56, 535 (1997).
30. P.J.E. Peebles, Astrophys. J. 510, 523 (1999)
31. Astrophys. J.P.J.E. Peebles, 510, 523 (1999).
32. K. Coble, astro-ph/9902195.
33. S.Yu. Khlebnikov and I.I. Tkachev, Phys. Rev. Lett. 77, 219 (1996).
34. N.A. Bahcall and X. Fan, Proc. Natl. Acad. Sci. USA 95, 5956 (1998)
35. P.J.E. Peebles, Philos. Trans. R. Soc. London 357, 21 (1999).
36. H. Risken, The Fokker-Planck Equation (Springer-Verlag, Berlin, 1989).