An Upper bound on the number of e-foldings
Jul, 2003Citations per year
Abstract: (arXiv)
If the present acceleration of the universe is due to an asymptotically de Sitter universe with small cosmological constant, and the principle of Cosmological Complementarity is valid, then the number of e-foldings during inflation is bounded.Note:
- 16 pages, latex. New version has extensive modifications to clarify the basic assumptions on which the bound is based and can be viewed as a response to the paper of Lowe and Marolf, correction of typos and added references
- inflation
- astrophysics: acceleration
- space-time: de Sitter
- cosmological constant
- holography
References(48)
Figures(0)
- ,
- ,
- ,
- ,
- •
- Astrophys.J. 564 (2002) 559-566
- e-Print:•
- DOI:
- ,
- ,
- J. Bock(,)
- Caltech, JPL and
- Caltech
- ,
- •
- Astrophys.J.Lett. 545 (2000) L1-L4,
- Astrophys.J.Lett. 558 (2001) L145-L146 (erratum)
- e-Print:•
- DOI:
- ,
- ,
- J. Bock(,)
- Caltech, JPL and
- Caltech
- ,
- •
- Astrophys.J.Lett. 545 (2000) L1-L4,
- Astrophys.J.Lett. 558 (2001) L145-L146 (erratum)
- e-Print:•
- DOI:
- ,
- ,
- ,
- ,
- •
- Astrophys.J.Lett. 561 (2001) L7-L10
- e-Print:•
- DOI:
- ,
- ,
- ,
- ,
- •
- Mon.Not.Roy.Astron.Soc. 334 (2002) 11
- e-Print:•
- ,
- ,
- ,
- ,
- •
- Astrophys.J. 568 (2002) 46-51
- e-Print:•
- DOI:
- Collaboration•
- •
- Astrophys.J.Suppl. 148 (2003) 175-194
- e-Print:•
- DOI:
- Collaboration•
- •
- Astrophys.J. 483 (1997) 565
- e-Print:•
- DOI:
- ,
- ,
- ,
- ,
- •
- Astron.J. 116 (1998) 1009-1038
- e-Print:•
- DOI:
- •
- Nucl.Phys.B Proc.Suppl. 124 (2003) 3-12,
- e-Print:•
- •
- JHEP 08 (2002) 045
- e-Print:•
- •
- Conf.Proc.C 930308 (1993) 284-296
- e-Print:
- •
- J.Math.Phys. 36 (1995) 6377-6396
- e-Print:•
- DOI:
- •
- JHEP 06 (2002) 017
- e-Print:•
- ,
- ,
- •
- JHEP 06 (2002) 053
- e-Print:•
- ,
- ,
- ,
- •
- JHEP 03 (2003) 031
- e-Print:•
- •
- Phys.Rev.D 70 (2004) 026001
- e-Print:•
- •
- JHEP 09 (2003) 024
- e-Print:•
- •
- Int.J.Mod.Phys.A 16 (2001) 910-921,
- e-Print:•
- •
- Phys.Rev.D 15 (1977) 2738-2751
- •
- JHEP 11 (2000) 038
- e-Print:•