The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
Observational consequences of a landscape
Open accessAbstract
In this paper we consider the implications of the ``landscape paradigm [1], [2] for the large scale properties of the universe. The most direct implication of a rich landscape is that our local universe was born in a tunnelling event from a neighboring vacuum. This would imply that we live in an open FRW universe with negative spatial curvature. We argue that the ``overshoot problem, which in other settings would make it difficult to achieve slow roll inflation, actually favors such a cosmology. We consider anthropic bounds on the value of the curvature and on the parameters of inflation. When supplemented by statistical arguments these bounds suggest that the number of inflationary efolds is not very much larger than the observed lower bound. Although not statistically favored, the likelihood that the number of efolds is close to the bound set by observations is not negligible. The possible signatures of such a low number of efolds are briefly described.
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Cites
Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377253 · Cited by 4,860
Cosmological Inflation and Large-Scale Structure
Liddle, A. R., & Lyth, D. H. (2000) · doi:10.1017/cbo9781139175180 · Cited by 2,317
Gravitational effects on and of vacuum decay
Coleman, S., & De Luccia, F. (1980) · Physical Review D · doi:10.1103/physrevd.21.3305 · Cited by 1,537 · cited 4×
“The theory of this process, developed long ago by Coleman and De Luccia [4], is described by an instanton–a solution of the Euclidean equations of motion–with the topology of a four-sphere.”
BackgroundMethodInfluentialAnthropic Bound on the Cosmological Constant
Weinberg, S. (1987) · Physical Review Letters · doi:10.1103/physrevlett.59.2607 · Cited by 1,166
The statistics of string/M theory vacua
Douglas, M. R. (2003) · Journal of High Energy Physics · doi:10.1088/1126-6708/2003/05/046 · Cited by 791
What does inflation really predict?
Tegmark, M. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/04/001 · Cited by 216
Is the low cosmic microwave background quadrupole a signature of spatial curvature?
Efstathiou, G. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06940.x · Cited by 210
Why Is the Cosmic Microwave Background Fluctuation Level 10−5?
Tegmark, M., & Rees, M. J. (1998) · The Astrophysical Journal · doi:10.1086/305673 · Cited by 159
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Monodromy in the CMB: Gravity waves and string inflation
Silverstein, E., & Westphal, A. (2008) · Physical Review D · doi:10.1103/physrevd.78.106003 · Cited by 724
A Natural Framework for Chaotic Inflation
Kaloper, N., & Sorbo, L. (2009) · Physical Review Letters · doi:10.1103/physrevlett.102.121301 · Cited by 332
The evidence for a spatially flat Universe
Efstathiou, G., & Gratton, S. (2020) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slaa093 · Cited by 203
Emir Gümrükçüo, A., Contaldi, C. R., & Peloso, M. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/11/005 · Cited by 185
Density perturbations and the cosmological constant from inflationary landscapes
Feldstein, B., Hall, L. J., & Watari, T. (2005) · Physical Review D · doi:10.1103/physrevd.72.123506 · Cited by 74
Metadata
- Authors
- Freivogel, B., Kleban, M., Martínez, M. R., & Susskind, L.
- Venue
- Journal of High Energy Physics
- Published
- 2006-03-09
- Volume
- 2006
- Issue
- 03
- Pages
- 039-039
- ISSN
- 1029-8479 (ISSN-L)
- OpenAlex
- W2114900035
- Cited by
- 273
- References
- 8
- FWCI
- 12.53
- Type
- journal article
- Language
- en
- Open access
- bronze
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