Julien LESGOURGUES (.pdf)

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Post-WMAP Post WMAP (1 st st yr 2) one isocurvature + adiabatic : 2 cos∆α½ (1−α) ½ α yr) ) bounds α < 0.3 (2σ)
Post-WMAP Post WMAP (1 st st yr 2) one isocurvature + adiabatic : ⇒ implications for slow-roll double inflation V = ½ m 1 2 φ1 2 + ½ m2 2 φ2 2 R = m 1 / m 2 > 1 yr) ) bounds {α , β , cos∆ , n ad , n is , n cor } functions of { R , θ k , s } n cor ≈ 0 and φ 1 θ s e-folds before the end φ 2
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 and 18: 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 31: 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

Julien LESGOURGUES (.pdf)

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