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CONSTRAINING THE PROPERTIES OF DARK MATTER WITH OBSERVATIONS OF THE COSMIC MICROWAVE BACKGROUND

  • Authors: Daniel B. Thomas, Michael Kopp, and Constantinos Skordis

2016 The Astrophysical Journal 830 155.

  • Provider: AAS Journals

Caption: Figure 5.

TT spectrum plotted for the ΛCDM best-fit values and for values of c2s and ﹩{c}_{\mathrm{vis}}^{2}﹩ that are close to our ﹩99.7 \% ﹩ CL. The residuals of the c2s, ﹩{c}_{\mathrm{vis}}^{2}\ne 0﹩ curves with respect to the best-fit Cls have been multiplied by a factor of 50 to make them more visible as in Figure 2. The key difference between the GDM and ΛCDM curves is the reduced smoothing of the peaks in the GDM model, caused by the reduced lensing potential.

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