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Potentials favored from observations <br />

(Einstein frame) <br />

Natural inflation

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Summary Overall, <strong>the</strong> single-‐field small-‐field models with are favored.

Potentials favored from observations (Einstein frame) Natural inflation

Page 1 and 2: S. Tsujikawa, J. Ohashi, S.Kuro
Page 3 and 4: Old inflation (Sato, Kazanas, G
Page 5 and 6: Standard slow-‐roll inflation
Page 7 and 8: S = ⇤ d 4 x ⇥ g ⇥ R 16 G + X
Page 9 and 10: Discrimination between inflaton
Page 11 and 12: S.T., J. Ohashi, S. Kuroyanagi,
Page 13 and 14: Horndeski’s paper in 1973
Page 15 and 16: Power spectrum of curvature per
Page 17 and 18: We can apply our general resul
Page 19 and 20: Planck constraints on Brans-Dicke g
Page 21 and 22: Higgs inflation There are severa
Page 23 and 24: Running kinetic couplings 0.3 0.25
Page 25 and 26: f NL B R f NL ・・・nonlinear e
Page 27: Observational constraints on power-