Self-tuning solution of the cosmological constant problem with antisymmetric tensor field
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Publication:5944294
DOI10.1016/S0550-3213(01)00397-2zbMath0970.83040arXivhep-th/0101027OpenAlexW2049981721MaRDI QIDQ5944294
Jihn E. Kim, Hyun Min Lee, Bumseok Kyae
Publication date: 4 October 2001
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/0101027
Related Items (8)
GHOSTS AND TACHYONS IN THE FIFTH DIMENSION ⋮ Inflation with blowing-up solution of cosmological constant problem ⋮ Induced cosmology on a regularized brane in six-dimensional flux compactification ⋮ Unnamed Item ⋮ Gravitational potential correction with Gauss-Bonnet interaction ⋮ Randall-Sundrum scenario at nonzero temperature ⋮ A quintessential axion ⋮ Singular quantum mechanical viewpoint of localized gravity in brane-world scenario
Cites Work
- Why there is nothing rather than something: A theory of the cosmological constant
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Inflationary universe: A possible solution to the horizon and flatness problems
- The cosmological constant problem
- Cosmology of Randall-Sundrum models with an extra dimension stabilized by balancing bulk matter.
- Exact cosmological solution and modulus stabilization in the Randall-Sundrum model with bulk matter
- Bulk supersymmetry and brane cosmological constant
- General properties of the self-tuning domain wall approach to the cosmological constant problem
- Naked singularity and Gauss-Bonnet term in brane world scenarios
- Dynamical instability of brane solutions with a self-tuning cosmological constant
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