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The cosmological constant problem from a brane-world perspective

Stefan Förste1, Zygmunt Lalak1, Stéphane Lavignac1 and Hans Peter Nilles1

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We point out several subtleties arising in brane-world scenarios of cosmological constant cancellation. We show that solutions with curvature singularities are inconsistent, unless the contribution to the effective four-dimentional cosmological constant of the physics that resolves the singularities is fine-tuned. This holds for both flat and curved branes. Irrespective of this problem, we then study an isolated class of flat solutions in models where a bulk scalar field with a vanishing potential couples to a 3-brane. We give an example where the introduction of a bulk scalar potential results in a non-zero cosmological constant. Finally we comment on the stability of classical solutions of the brane system with respect to quantum corrections.


Keywords

p-branes

Extra Large Dimensions

Cosmology of Theories beyond the SM

Field Theories in Higher Dimensions

 

E-print Number: hep-th/0006139

Cited: by |

Refers: to

PACS

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)

11.25.Wx String and brane phenomenology

11.10.Kk Field theories in dimensions other than four

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 09 ( 1 September 2000)

Received 21 June 2000, accepted for publication 21 September 2000

Published 3 November 2000



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