Orbifold construction of the modes of the Poincare dodecahedral space
arXiv:0801.4232 · doi:10.1088/1751-8113/41/29/295209
Abstract
We provide a new construction of the modes of the Poincare dodecahedral space S^3/I*. The construction uses the Hopf map, Maxwell's multipole vectors and orbifolds. In particular, the *235-orbifold serves as a parameter space for the modes of S^3/I* shedding new light on the geometrical significance of the dimension of each space of -modes, as well as on the modes themselves.
References in corpus (8)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The optimal phase of the generalised Poincare dodecahedral space hypothesis implied by the spatial cross-correlation function of the WMAP sky maps
- Correlating anomalies of the microwave sky: The Good, the Evil and the Axis
- A test of the Poincare dodecahedral space topology hypothesis with the WMAP CMB data
- CMB Alignment in Multi-Connected Universes
- A spatial correlation analysis for a toroidal universe
- Probability Density of the Multipole Vectors for a Gaussian Cosmic Microwave Background
- Constraining Cosmic Topology with CMB Polarization