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S.T., J. Ohashi, S. Kuroyanagi, A De Felice, arXiv: 1305.3044 <br />
Potential−driven slow−roll inflation<br />
10 0 Inclusion of high L data prefers <br />
Planck+WP+BAO+high L <br />
<strong>the</strong> smaller spectral index. <br />
Planck+WP+BAO <br />
4<br />
power law inflation<br />
10 −1<br />
2<br />
1<br />
r 0.05<br />
natural<br />
2/3<br />
10 −2<br />
large−field<br />
small−field<br />
R 2 inflation<br />
10 −3<br />
very<br />
small<br />
field<br />
hybrid2<br />
hybrid1<br />
0.94 0.95 0.96 0.97 0.98 0.99 1 1.01<br />
n s
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