CMB anisotropy: Inflation - iucaa

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oIntriguing: Lack of power at large angular scales ( θ ≥ 60 )?NASA/WMAP science teamLow Quadrupole ΔT2= 8 ± 2μK(COBE ΔT1072=+−4μK)=2
Deconvolving the primordial power spectrum(Shafieloo & Souradeep, 2004 PRD )Cited in WMAP-3 paperPrimordial power spectrumfrom Early universe candeconvolved from <strong>CMB</strong><strong>anisotropy</strong>spectrumHorizon scaleCl=∫dkkP( k)G ( k)lImproved Error sensitiveiterative Richardson-Lucydeconvolution methodRecovered spectrum shows an infra-red cut-off on Horizon scale !!!Is it cosmic topology ? Signature of pre-inflationary phase ? QG physics ? ….
Page 1 and 2: CMB anisotropy:a probe of primordia
Page 3 and 4: Thompson scattering of theCMB aniso
Page 5 and 6: Adiabatic ICTE, EE peak outof phase
Page 8 and 9: CMB Task force report 2005Null BB:
Page 10 and 11: Near future : High resolution C l(S
Page 12 and 13: European space agency(ESA)Scheduled
Page 15 and 16: Cosmic Gravity wave background from
Page 17 and 18: Is the universe infinite?Torus spac
Page 19 and 20: Correlated Circles(Cornish, Spergel
Page 21 and 22: BiPS signature of a “soccer ball
Page 23 and 24: Hunting Correlation patternsin theC
Page 25 and 26: SphericalharmonicsalmSpherical Harm
Page 27: Used Simulated 30 GHz maps from Pla
Page 31: Web references for further explorat

CMB anisotropy: Inflation - iucaa

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