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A Self-Tuning Solution of the Cosmological Constant Problem
We discuss the four-dimensional cosmological constant problem in a five-dimensional setting. A scalar field coupled to the SM forms dynamically a smooth brane with four-dimensional Poincar\'e invariance, independently of SM physics. In this respect, our solution may be regarded as a self-tuning...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
2000
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| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/474329 |