Published February 3, 2014 | Version v1
Journal article

Decay rates of Gaussian-type I-balls and Bose-enhancement effects in 3+1 dimensions

  • 1. ICRR, University of Tokyo, Kashiwa, 277-8582 (Japan)
  • 2. Kavli IPMU (WPI), TODIAS, University of Tokyo, Kashiwa, 277-8583 (Japan)

Description

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

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2014/02/001; Available from http://repo.scoap3.org/record/1189

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2014
Journal Issue
02
Journal Page Range
p. 1
ISSN
1475-7516

Optional Information

Notes
PUBLISHER-ID: JCAP02(2014)001; OAI: oai:repo.scoap3.org:1189
Funding organization
SCOAP3, CERN, Geneva (Switzerland)