1 / 28

CMB?

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.

cricket
Télécharger la présentation

CMB?

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. CMB?

  2. 1. Espectro de la RCF 2. Anisotropías de la RCF

  3. CMB anisotropy + +

  4. 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

  5. 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)

  6. 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!

  7. How do we “hear” the cosmic sound from this?

  8. metric perturbations • Decomposition into scalar, vector and tensor components Linear cosmological perturbation theory

  9. 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]

  10. Approximate Equation System in the Strong Coupling Regime SOUND WAVE!

  11. Cosmic Sound Wave!

  12. Itisthenatureofthingsthattheyare tiestoeachother.   —Chuang-tzu (300BC) It is the nature of things that they are ties to each other.   —Chuang-tzu (300BC)

More Related