Spectroscopy of cosmic topology

Indian Journal of Physics

Volumn 80, Issue 11, 2006, Pages 1063-1069

  Souradeep, Tarun ^a  

^a INTER UNIVERSITY CENTRE FOR ASTRONOMY AND ASTROPHYSICS   (India)

Author keywords

Cosmic microwave background cosmology; Observations; Theory; Topology

Indexed keywords

EID: 33847012127     PISSN: 02529262     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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38. 2 [8])
39. The same line of reasoning hold for CMB polarization when expressed in terms of Gaussian scalar Ẽ(n̂) and pseudoscalar B̃(n̂) fields with corresponding two point correlation function. For brevity, we explicitly discuss only the temperature anisotropy.
40. 2, to reduce the cosmic variance.
41. For cubic torus the Dirichlet domain (DD) matches the fundamental domain (FD). However, for torus spaces with cuboid and parallelpiped FD, the corresponding DD is very different, e.g., hexahonal prism [18,25]