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CMB as a Probe of New Physics and Old Times

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Figure

Figure 1.1: Quadrupolar anisotropy is illustrated, where the hot and cold spots lie at the surface oflast scatter (plane of the drawing), and the observer’s line of sight is perpendicular to it
Figure 2.1: Temperature sky maps in Galactic coordinates (smoothed) from WMAP-9 (Figure fromRef
Figure 2.2: Maps of polarized intensity pWMAP-9; line segments represent the direction of polarization plane for pixels where signal-to-noise> ≡ (Q2 + U 2)0.5 in Galactic coordinates (smoothed) from 1 (Figure from Ref
Figure 3.1: Shown are the current best measurements of the TT-power-spectrum multipoles, alongwith the best-fit curve, from WMAP-9 (black), SPT (blue), and ACT (orange) experiments (Figurefrom Ref
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