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Автор Kaiki Taro Inoue
Дата выпуска 2001-05-21
dc.description In this paper, the cosmic microwave background (CMB) anisotropy in a multiply connected compact flat 3-torus model with the cosmological constant is investigated. Using the COBE-DMR four-year data, a full Bayesian analysis revealed that the constraint on the topology of the flat 3-torus model with low matter density is less stringent. As in compact hyperbolic models, the large-angle temperature fluctuations can be produced as the gravitational potential decays at the Λ-dominant epoch well after the last scattering. The maximum allowed number of images of the cell, N (fundamental domain), within the observable region at present is approximately 49 for Ω<sub>m</sub> = 0.1 and Ω<sub>Λ</sub> = 0.9, whereas N~8 for Ω<sub>m</sub> = 1.0 and Ω<sub>Λ</sub> = 0.
Формат application.pdf
Издатель Institute of Physics Publishing
Название COBE constraints on a compact toroidal low-density universe
Тип paper
DOI 10.1088/0264-9381/18/10/310
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 18
Первая страница 1967
Последняя страница 1978
Аффилиация Kaiki Taro Inoue; National Astronomical Observatory, Division of Theoretical Astrophysics, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Выпуск 10

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