Julien LESGOURGUES (.pdf)

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How do they affect CMB and LSS? 3) adiabatic versus NID : spectra for n ad =n iso =1 l(l+1)C T l /2 π NID (S rad =1) AD (R rad = 1) l
How do they affect CMB and LSS? 3) adiabatic versus NID : spectra for n ad =n iso =1 P(k) NID (S rad =1) AD (R rad = 1) k
Page 1 and 2: Isocurvature Modes after WMAP WMAP-
Page 3 and 4: What are they? they various perfect
Page 5 and 6: general case: What are they? they
Page 7 and 8: What are they? they ⇒ set of init
Page 9 and 10: How can they be generated ? Isocurv
Page 11 and 12: How can they be generated ? 1) Topo
Page 13 and 14: 1) adiabatic versus CDI : Sachs-Wol
Page 15 and 16: How do they affect CMB and LSS? 1)
Page 17: How do they affect CMB and 2) adiab
Page 25 and 26: Post-WMAP Post WMAP (1 st st yr yr)
Page 29 and 30: Post-WMAP Post WMAP (1 st st yr 2)
Page 37 and 38: Post-WMAP Post WMAP (1 st yr) bound
Page 39: Conclusions 1) NO EVIDENCE FOR ISOC

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