Understand
We address an issue what kind of tuning realizes a flat potential for inflaton in supergravity.
- We restrict ourselves to the case that inflationary dynamics is not affected by separate supersymmetry-breaking effects, and consider examples of a single chiral superfield as an inflaton with its vacuum of the vanishing cosmological constant.
- The examples potentially include the cases of Polonyi field or right-handed sneutrino as an inflaton.
Built on
A.S. Goncharov and A.D. Linde, Phys. Lett. B139
1984
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Similar
For reviews, D.H. Lyth and A. Riotto, arXiv:hep-ph/9807278; L. Alabidi and D.H. Lyth, arXiv:astro-ph/0510441; arXiv:astro-ph/0603539
Cited in the paper.
M. Ibe, Izawa K.-I., and T. Yanagida, arXiv:hep-ph/0409203
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Izawa K.-I., arXiv:hep-ph/0702127
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H. Murayama, H. Suzuki, T. Yanagida, and J. Yokoyama, arXiv:hep-ph/9311326
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Izawa K.-I., arXiv:hep-ph/9708315
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See S. Dimopoulos and S. Thomas, arXiv:hep-th/0307004
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Izawa K.-I., M. Kawasaki, and T. Yanagida, arXiv:hep-ph/9707201
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A. Hebecker, arXiv:hep-th/0407196
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Izawa K.-I., arXiv:hep-ph/9710479
Cited in the paper.
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