Tensor Anisotropies in an Open Universe
arXiv:astro-ph/9701210 · doi:10.1086/310821
Abstract
We calculate the anisotropies in the cosmic microwave background induced by long-wavelength primordial gravitational waves in a universe with negative spatial curvature, such as are produced in the ``open inflation'' scenario. The impact of these results on the COBE normalization of open models is discussed.
5pgs, 2 figs.; also avalable at http://www.sns.ias.edu/~whu, revision reflects ApJL published version, model dependence clarified
References in corpus (3)
Cited by in corpus (16)
- Efficient Computation of CMB anisotropies in closed FRW models
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Power Spectra for Cold Dark Matter and its Variants
- A Complete Treatment of CMB Anisotropies in a FRW Universe
- The Observational Mass Function of Nearby Galaxy Clusters
- Cosmological Constraints from the ROSAT Deep Cluster Survey
- Microwave background anisotropies from gravitational waves: the 1+3 covariant approach
- The Imprint of Gravitational Waves in Models Dominated by a Dynamical Cosmic Scalar Field
- Fast and accurate CMB computations in non-flat FLRW universes
- Constraints on Cosmological Parameters from the Lyman-alpha Forest Power Spectrum and COBE-DMR
- Is there a left-handed magnetic field in the solar neighborhood? Exploring helical magnetic fields in the interstellar medium through dust polarization power spectra
- Bispectrum from open inflation
- Microwave background anisotropies in quasiopen inflation
- Limits on the gravity wave contribution to microwave anisotropies
- Polarized CMB recovery with sparse component separation
- A new approach of estimating the Galactic thermal dust and synchrotron polarized emission template in the microwave bands