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CMB?. 1. Espectro de la RCF. 2. Anisotrop ías de la RCF. CMB anisotropy. +. +. Anisotropies . T( θ , φ ), Q( θ , φ ), U( θ , φ ), V( θ , φ ). spherical harmonics. X( θ , φ )= Σ lm a lm X Y s lm ( θ , φ ). X=T,E,B. s=0 for T, 2 for Q and U. E and B modes have opposite parity.
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1. Espectro de la RCF 2. Anisotropías de la RCF
CMB anisotropy + +
Anisotropies T(θ,φ), Q(θ,φ), U(θ,φ), V(θ,φ) spherical harmonics X(θ,φ)=Σlm almXYslm(θ,φ) X=T,E,B s=0 for T, 2 for Q and U E and B modes have opposite parity
Angular power spectrum T(θ,φ), Q(θ,φ), U(θ,φ), V(θ,φ) spherical harmonics aXlm, X=T,E,B information compression Cl=Σm [(almX)(almY)*]/(2l+1)
Use Ripples in CMB to Measure Composition of the Universe • The Basic Idea: Hit it and listen to the cosmic sound. • Analogy: Brass and ceramic can be discriminated by hitting them and listening to the sound created by them. • We can use sound waves to determine composition. • When CMB was emitted the Universe was a dense and hot soup of photons, electrons, protons, Helium nuclei, and dark matter particles. • Ripples in CMB propagate in the cosmic soup: the pattern of the ripples, the cosmic sound wave, can be used to determine composition of the Universe!
metric perturbations • Decomposition into scalar, vector and tensor components Linear cosmological perturbation theory
The cartoon • At early times the universe was hot, dense and ionized. Photons and matter were tightly coupled by Thomson scattering. • Short m.f.p. allows fluid approximation: baryon-photon fluid • Initial fluctuations in density and gravitational potential drive acoustic waves in the fluid: compressions and rarefactions. • A sudden “recombination” decouples the radiation and matter, giving us a snapshot of the fluid at “last scattering”. [harmonic wave]
Approximate Equation System in the Strong Coupling Regime SOUND WAVE!
Itisthenatureofthingsthattheyare tiestoeachother. —Chuang-tzu (300BC) It is the nature of things that they are ties to each other. —Chuang-tzu (300BC)