## Abstract

I-balls/oscillons are long-lived spatially localized lumps of a scalar field which may be formed after inflation. In the scalar field theory with monomial potential nearly and shallower than quadratic, which is motivated by chaotic inflationary models and supersymmetric theories, the scalar field configuration of I-balls is approximately Gaussian. If the I-ball interacts with another scalar field, the I-ball eventually decays into radiation. Recently, it was pointed out that the decay rate of I-balls increases exponentially by the effects of Bose enhancement under some conditions and a non-perturbative method to compute the exponential growth rate has been derived. In this paper, we apply the method to the Gaussian-type I-ball in 3+1 dimensions assuming spherical symmetry, and calculate the partial decay rates into partial waves, labelled by the angular momentum of daughter particles. We reveal the conditions that the I-ball decays exponentially, which are found to depend on the mass and angular momentum of daughter particles and also be affected by the quantum uncertainty in the momentum of daughter particles.

Original language | English |
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Article number | 001 |

Journal | Journal of Cosmology and Astroparticle Physics |

Volume | 2014 |

Issue number | 2 |

DOIs | |

Publication status | Published - 2014 Feb |

Externally published | Yes |

## Keywords

- cosmological phase transitions
- ination
- physics of the early universe
- supersymmetry and cosmology

## ASJC Scopus subject areas

- Astronomy and Astrophysics