2003
DOI: 10.1016/j.physletb.2003.06.060
|View full text |Cite
|
Sign up to set email alerts
|

Accelerating cosmologies from M/String theory compactifications

Abstract: We point out that the solution of $(4+n)$-dimensional gravity coupled to the dilaton and an $n$-form field strength can give rise to a flat 4-dimensional universe (with a scale factor) of the type proposed recently under time dependent compactifications. The compact internal spaces could be hyperbolic, flat or spherical and the solution is identical to the space-like two brane or S2-brane. As has been shown previously for SM2 solution with a fixed field strength we show that for $n=7$ (where the dilaton is van… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

1
75
0

Year Published

2003
2003
2023
2023

Publication Types

Select...
9
1

Relationship

1
9

Authors

Journals

citations
Cited by 109 publications
(76 citation statements)
references
References 31 publications
1
75
0
Order By: Relevance
“…We save these topics for future study. For large (cosmic) time t, we take the ansatz 6) for n > 0. The idea is that the two equations of motion scale differently for large t.…”
Section: Resultsmentioning
confidence: 99%
“…We save these topics for future study. For large (cosmic) time t, we take the ansatz 6) for n > 0. The idea is that the two equations of motion scale differently for large t.…”
Section: Resultsmentioning
confidence: 99%
“…For the heterotic strings, the leading correction is given by the GB terms with the coefficient [13,14]: 9) multiplied by an exponential factor of the dilaton, where α ′ is the Regge slope parameter.…”
Section: )mentioning
confidence: 99%
“…Astronomical observations indicate that our universe is flat and currently consists of approximately 2 3 dark energy and 1 3 dark matter. The nature of dark energy as well as dark matter is unknown, and many radically different models have been proposed, such as, a tiny positive cosmologi-cal constant, quintessence [16][17][18], DGP branes [19,20], the non-linear F(R) models [21][22][23], and dark energy in brane worlds, among many others [24][25][26][27][28][29][30][31][32][33][34][35][36][37][38][39][40][41][42][43]; see also the review articles [44,45], and references therein. As mentioned before, the existence of dark energy fluids comes from the observations of the accelerated expansion of the universe and the isotropic pressure cosmological models give the best fitting of the observations.…”
Section: Introductionmentioning
confidence: 99%