Peculiar Features in the Cosmic Microwave Background Radiation

نویسندگان

  • Patrick Dineen
  • Peter Coles
  • Pedro Ferreira
چکیده

4 1 Standard framework 5 1.1 Big bang models . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 1.2 The cosmic microwave background . . . . . . . . . . . . . . . . . . 10 2 Characterizing early Universe fluctuations 15 2.1 Density fluctuations . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 2.2 CMB temperature fluctuations . . . . . . . . . . . . . . . . . . . . . 18 2.3 Fluctuations on a sphere: the spherical harmonics . . . . . . . . . . . 22 2.3.1 Correlated l–modes . . . . . . . . . . . . . . . . . . . . . . . 23 2.3.2 Correlated m–modes . . . . . . . . . . . . . . . . . . . . . . 25 2.3.3 Correlations in inverted images . . . . . . . . . . . . . . . . 27 3 Non–Gaussian fluctuations in the CMB 28 3.

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تاریخ انتشار 2005