Possible connection between the location of the cutoff in the cosmic microwave background spectrum and the equation of state of dark energy

Physical Review Letters

Volumn 93, Issue 22, 2004, Pages

  Enqvist, Kari ^a   Sloth, Martin S ^a,b  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC MICROWAVE BACKGROUND (CMB); COSMOLOGY; DARK ENERGY; QUANTUM GRAVITY;

ACCELERATION; ANISOTROPY; BESSEL FUNCTIONS; DEGREES OF FREEDOM (MECHANICS); ENTROPY; INFRARED RADIATION; LINEAR EQUATIONS; MATHEMATICAL MODELS; MICROWAVES; SPECTRUM ANALYSIS; ULTRAVIOLET RADIATION;

COSMIC RAYS;

EID: 42749107849     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.93.221302     Document Type: Article

References (20)

1. D. N. Spergel et al., Astrophys. J. Suppl. Ser. 148, 175 (2003).
2. C. R. Contaldi, M. Peloso, L. Kofman, and A. Linde, J. Cosmol. Astropart. Phys. 07 (2003) 002.
3. G. 't Hooft, gr-qc/9310026; L. Susskind, J. Math. Phys. (N.Y.) 36, 6377 (1995); R. Bousso, Rev. Mod. Phys. 74, 825 (2002).
4. G. 't Hooft, gr-qc/9310026; L. Susskind, J. Math. Phys. (N.Y.) 36, 6377 (1995); R. Bousso, Rev. Mod. Phys. 74, 825 (2002).
5. G. 't Hooft, gr-qc/9310026; L. Susskind, J. Math. Phys. (N.Y.) 36, 6377 (1995); R. Bousso, Rev. Mod. Phys. 74, 825 (2002).
6. J. D. Bekenstein, Phys. Rev. D 23, 287 (1981); 7, 2333 (1973).
7. J. D. Bekenstein, Phys. Rev. D 23, 287 (1981); 7, 2333 (1973).
8. A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Phys. Rev. Lett. 82, 4971 (1999).
9. S. Thomas, Phys. Rev. Lett. 89, 081301 (2002).
10. S. D. H. Hsu, Phys. Lett. B 594, 13 (2004).
11. M. Li, hep-th/0403127.
12. Q. G. Huang and M. Li, J. Cosmol. Astropart. Phys. 08 (2004) 013.
13. L. Susskind, L. Thorlacius, and J. Uglum, Phys. Rev. D 48, 3743 (1993); L. Susskind, Phys. Rev. Lett. 71, 2367 (1993); L. Susskind and L. Thorlacius, Phys. Rev. D 49, 966 (1994); L. Susskind and J. Uglum, Nucl. Phys. (Proc. Suppl.) 45BC, 115(1996).
14. L. Susskind, L. Thorlacius, and J. Uglum, Phys. Rev. D 48, 3743 (1993); L. Susskind, Phys. Rev. Lett. 71, 2367 (1993); L. Susskind and L. Thorlacius, Phys. Rev. D 49, 966 (1994); L. Susskind and J. Uglum, Nucl. Phys. (Proc. Suppl.) 45BC, 115(1996).
15. L. Susskind, L. Thorlacius, and J. Uglum, Phys. Rev. D 48, 3743 (1993); L. Susskind, Phys. Rev. Lett. 71, 2367 (1993); L. Susskind and L. Thorlacius, Phys. Rev. D 49, 966 (1994); L. Susskind and J. Uglum, Nucl. Phys. (Proc. Suppl.) 45BC, 115(1996).
16. L. Susskind, L. Thorlacius, and J. Uglum, Phys. Rev. D 48, 3743 (1993); L. Susskind, Phys. Rev. Lett. 71, 2367 (1993); L. Susskind and L. Thorlacius, Phys. Rev. D 49, 966 (1994); L. Susskind and J. Uglum, Nucl. Phys. (Proc. Suppl.) 45BC, 115(1996).
17. J. Levin, Phys. Rep. 365, 251 (2002).
18. 0 - η*)/c.
19. A. Melchiorri, L. Mersini, C. J. Odman, and M. Trodden, Phys. Rev. D 68, 043509 (2003).
20. N. Kaloper, M. Kleban, and L. Sorbo, astro-ph/406099.