How can the observed temperature anisotropy of the CMB be used ... | Filo
How can the observed temperature anisotropy of the CMB be used ... | Filo
Apr 20, 2025
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SOLVED:Determine the locations of the peaks and troughs in the CMB anisotropy spectrum if the universe is Euclidean with a cosmological constant. Keep the sound horizon fixed in this calculation by fixing Ωm h^2 to the value in the fiducial cosmology. The peak positions then depend only on the distance to the last-scattering surface, η0-η*. Consider two Euclidean models: (i) ΩΛ=0 (so that Ωm=1 ) and (ii) ΩΛ=0.7 (so that Ωm=0.3 ). What value of h is needed in the two cases to keep Ωm h^2 fixed? D
SOLVED:Determine the locations of the peaks and troughs in the CMB anisotropy spectrum if the universe is Euclidean with a cosmological constant. Keep the sound horizon fixed in this calculation by fixing Ωm h^2 to the value in the fiducial cosmology. The peak positions then depend only on the distance to the last-scattering surface, η0-η*. Consider two Euclidean models: (i) ΩΛ=0 (so that Ωm=1 ) and (ii) ΩΛ=0.7 (so that Ωm=0.3 ). What value of h is needed in the two cases to keep Ωm h^2 fixed? D
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