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A new cosmological constant model
We propose a new cosmological model with a time-dependent cosmological constant (\Lambda\propto 1/t^2), which starting at the Planck time as \Lambda_{Pl}\sim M^2_{Pl}, evolves to the present-day allowed value of \Lambda_0\sim10^{-120}M^2_{Pl}. This scenario is supported by non-critical string theory...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
1995
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1142/S0217732396000023 http://cds.cern.ch/record/275045 |