## Аннотация

We review the new theory of modified supergravity, dubbed the F(R) supergravity, and some of its recent applications to inflation and reheating in the early universe cosmology. The F(R) supergravity is the N = 1 locally supersymmetric extension of the f(R) gravity in four space-time dimensions. A manifestly supersymmetric formulation of the F(R) supergravity exist in terms of N = 1 superfields, by using the (old) minimal Poincaré supergravity in curved superspace. We find the conditions for stability, the absence of ghosts and tachyons. Three models of the F(R) supergravity are studied. The first example is devoted to a recovery of the standard (pure) N = 1 supergravity with a negative cosmological constant from the F(R) supergravity. As the second example, a generic R^{2} supergravity is investigated, and the existence of the AdS bound on the scalar curvature is found. As the third (and most important) example, a simple viable realization of chaotic inflation in supergravity is found. Our approach is minimalistic since it does not introduce new exotic fields or new interactions, beyond those already present in (super)gravity. The universal reheating mechanism is automatic. We establish the consistency of our approach and also apply it to preheating and reheating after inflation. The Higgs inflation and its correspondence to the Starobinsky inflation are established in the context of supergravity. We briefly review other relevant issues such as non-Gaussianity, CP-violation, origin of baryonic asymmetry, lepto-and baryo-genesis. The F(R) supergravity has promise for possible solutions to those outstanding problems too.

Язык оригинала | Английский |
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Номер статьи | 1330021 |

Журнал | International Journal of Modern Physics A |

Том | 28 |

Номер выпуска | 15 |

DOI | |

Состояние | Опубликовано - 20 июн 2013 |

Опубликовано для внешнего пользования | Да |

## ASJC Scopus subject areas

- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics
- Astronomy and Astrophysics