[1]
|
A. A. Penzias and A. R. W. Wilson, “Early cosmic background,” Astrophysics Tournament, Vol. 142, 1965, pp. 419-425.
|
[2]
|
G. L. Bennet, et al., “First Year Wilkinson Microwave Anisotropy Probe {WMAP} Observation,” Astrophysics Journal, Vol. 148, 2003, pp. 1-28.
|
[3]
|
R. A. Alpher and R. C. Herman, “Evolution of the Universe,” Nature, Vol. 162, 1948, pp. 774-780.
|
[4]
|
K. Huang, “Statistical mecanics,” John Wiley Sons, Inc., New York, 1963.
|
[5]
|
V. S. Murzin, “Physics of Cosmic Ray,” Moscow State Universitety, Moscow, 1970.
|
[6]
|
A. de Oliveira-Costa, et al., “Cosmik Microwave Background Anisotropies in Multiconnected Flat Spaces,” Physics Review, Vol. D69, 2004, 103518.
|
[7]
|
N. K. Eriksen, et al., “Asymmetries in the Cosmic Microwave Background Anisotropy Field,” Astrophysics Journal, Vol. 605, No. 14, 2004.
|
[8]
|
D. J. Schwarz, et al., “Large-Angle Anomalies in the CMB,” arXiv:astro-ph/0403353.
|
[9]
|
M. Turler, “New WMAP Results Give Support to Inflation,” CERN Courier, Vol. 46, No. 4, 2006, p. 12.
|
[10]
|
V. A. Magnitsky, “General Geophysics,” Moscow State Universitety, Moscow, 1995.
|