Large Scale Anisotropy of the CMB in an Open Universe and Constraints on the Models of Galaxy Formation
We derived the formula by which we can calculate any multipole moment of cosmic microwave background anisotropy in an open universe. we also calculate by using this formula the rms quadrupole moment expected in some cosmological models and we restrict the models by comparing the calculated quadrupole moments with the observed upper limit of the quadrupole moment of the cosmic microwave background anisotropy.
KeywordsDark Matter Cosmological Model Cosmic Microwave Background Quadrupole Moment Multipole Moment
- Gouda, N., Sugiyama, N., and Sasaki, M. 1990(a), Large Angle Anisotropy of the Cosmic Microwave Background in an Open Universe, preprint.Google Scholar
- Gouda, N., Sugiyama, N., and Sasaki, M. 1990(b), Constraints on Open Universe Models from Quadrupole Anisotropy of the Cosmic Microwave Background, preprint.Google Scholar