%PDF-1.4 % 4 0 obj (1 Introduction: Success of inflation) endobj 5 0 obj << /D (subsection.1.1) /S /GoTo >> endobj 8 0 obj (1.1 Density perturbation) endobj 9 0 obj << /D (subsection.1.2) /S /GoTo >> endobj 12 0 obj (1.2 Further steps from observations) endobj 13 0 obj << /D (section.2) /S /GoTo >> endobj 16 0 obj (2 Basic feature of generation of non-Gaussianity of local-type.) endobj 17 0 obj << /D (subsection.2.1) /S /GoTo >> endobj 20 0 obj (2.1 Local non-Gaussianity) endobj 21 0 obj << /D (subsection.2.2) /S /GoTo >> endobj 24 0 obj (2.2 Super-horizon dynamics) endobj 25 0 obj << /D (section.3) /S /GoTo >> endobj 28 0 obj (3 Non-Gaussianity produced at the end of or after inflation) endobj 29 0 obj << /D (section.4) /S /GoTo >> endobj 32 0 obj (4 Non-Gaussianity produced during inflation) endobj 33 0 obj << /D (section.5) /S /GoTo >> endobj 36 0 obj (5 Is there any model which produces large non-Gaussianity during inflation?) endobj 37 0 obj << /D (subsection.5.1) /S /GoTo >> endobj 40 0 obj (5.1 Temporal slow-roll violation is not sufficient) endobj 41 0 obj << /D (subsection.5.2) /S /GoTo >> endobj 44 0 obj (5.2 Simple hybrid inflation does not give large non-Gaussianity) endobj 45 0 obj << /D (subsection.5.3) /S /GoTo >> endobj 48 0 obj (5.3 Modular inflation) endobj 49 0 obj << /D (section.6) /S /GoTo >> endobj 52 0 obj (6 Conclusion) endobj 53 0 obj << /D [ 54 0 R /Fit ] /S /GoTo >> endobj 56 0 obj << /Filter /FlateDecode /Length 1575 >> stream xڕWK6W(jQK=4i A=6b& Qܭ;!ey$Cp͋~uwjQrVfbiVܤ\ v.^wy*K{Y4 &jMeo̰J=.Wj"z7NRXbIMߝb;vH6\ec [C+2sgZ4)ٺa-5\iOPWCX+"+KpvUoӆ%/NEw kP\ enӺa&)[ oڎrt Хu/ FI"ኘ{<~rcuE;