2001
DOI: 10.1088/1126-6708/2001/01/027
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Brane Worlds, the Cosmological Constant and String Theory

Abstract: We argue that traditional methods of compactification of string theory make it very difficult to understand how the cosmological constant becomes zero. String inspired models can give zero cosmological constant after fine tuning but since string theory has no free parameters it is not clear that this is allowed. Brane world scenarios on the other hand while they do not answer the question as to why the cosmological constant is zero do actually allow a choice of integration constants that permit flat four space… Show more

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Cited by 22 publications
(28 citation statements)
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“…(The inclusion of a delta-function source is still necessary.) The use of the breathing mode was then explored in the context of the Randall-Sundrum I scenario (with two 3-branes [39]) in [53,54,55].…”
Section: Two-scalar Domain-wall Solutionsmentioning
confidence: 99%
“…(The inclusion of a delta-function source is still necessary.) The use of the breathing mode was then explored in the context of the Randall-Sundrum I scenario (with two 3-branes [39]) in [53,54,55].…”
Section: Two-scalar Domain-wall Solutionsmentioning
confidence: 99%
“…This connection was made in Refs. [13,14,15,16,17], which makes use of a massive five-dimensional supergravity scenario originating from an S 5 compactification of type IIB theory with a breathing mode [18]. This result ensures that the Randall-Sundrum scenario may be realized in a fully supersymmetric context.…”
Section: Introductionmentioning
confidence: 99%
“…12-15͒ with suggestions that they offer new approaches to the cosmological constant problem. [16][17][18][19][20][21][22][23][24][25] Many open questions remain, however, in the RSII scenario and its variants. One set of questions centers on the four-dimensional representation of the five-dimensional dynamics.…”
Section: Introductionmentioning
confidence: 99%