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Open inflation models and gravitational wave anisotropies in the CMB
We study the large scale power spectrum of gravitational wave perturbations of the microwave background in the context of single-bubble open inflation models. We compute the ratio of tensor to scalar contributions to the CMB anisotropies as a function of $\Omega_0$, the spectral index $n_S$ and the...
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| Lenguaje: | eng |
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1997
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.56.3225 http://cds.cern.ch/record/321156 |