Выдержка
We propose a large class of supergravity models in terms of a single chiral matter superfield, leading to (almost) arbitrary single-field inflationary scalar potentials similar to the F-term in rigid supersymmetry. Those scalar potentials are positively semi-definite (in our approximation), and can preserve supersymmetry at the end of inflation. The only scalar superpartner of inflaton is stabilized by a higher-dimensional term in the Kähler potential. We argue that couplings of the inflaton to other sectors of the particle spectrum do not affect the inflationary dynamics, and briefly discuss reheating of the universe by the inflaton decays.
| Язык оригинала | Английский |
|---|---|
| Страницы (с-по) | 1-22 |
| Число страниц | 22 |
| Журнал | Journal of High Energy Physics |
| Том | 2014 |
| Номер выпуска | 12 |
| DOI | |
| Состояние | Опубликовано - 2014 |
Отпечаток
ASJC Scopus subject areas
- Nuclear and High Energy Physics
Цитировать
Generic scalar potentials for inflation in supergravity with a single chiral superfield. / Ketov, Sergei V.; Terada, Takahiro.
В: Journal of High Energy Physics, Том 2014, № 12, 2014, стр. 1-22.Результат исследований: Материалы для журнала › Статья
}
TY - JOUR
T1 - Generic scalar potentials for inflation in supergravity with a single chiral superfield
AU - Ketov, Sergei V.
AU - Terada, Takahiro
PY - 2014
Y1 - 2014
N2 - We propose a large class of supergravity models in terms of a single chiral matter superfield, leading to (almost) arbitrary single-field inflationary scalar potentials similar to the F-term in rigid supersymmetry. Those scalar potentials are positively semi-definite (in our approximation), and can preserve supersymmetry at the end of inflation. The only scalar superpartner of inflaton is stabilized by a higher-dimensional term in the Kähler potential. We argue that couplings of the inflaton to other sectors of the particle spectrum do not affect the inflationary dynamics, and briefly discuss reheating of the universe by the inflaton decays.
AB - We propose a large class of supergravity models in terms of a single chiral matter superfield, leading to (almost) arbitrary single-field inflationary scalar potentials similar to the F-term in rigid supersymmetry. Those scalar potentials are positively semi-definite (in our approximation), and can preserve supersymmetry at the end of inflation. The only scalar superpartner of inflaton is stabilized by a higher-dimensional term in the Kähler potential. We argue that couplings of the inflaton to other sectors of the particle spectrum do not affect the inflationary dynamics, and briefly discuss reheating of the universe by the inflaton decays.
KW - Cosmology of theories beyond the SM
KW - Supergravity models
UR - http://www.scopus.com/inward/record.url?scp=84919598576&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84919598576&partnerID=8YFLogxK
U2 - 10.1007/JHEP12(2014)062
DO - 10.1007/JHEP12(2014)062
M3 - Article
AN - SCOPUS:84919598576
VL - 2014
SP - 1
EP - 22
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
SN - 1126-6708
IS - 12
ER -