Decay of I-ball/Oscillon in Classical Field Theory
arXiv:1901.06130 · doi:10.1007/JHEP04(2019)030
Abstract
I-balls/oscillons are long-lived and spatially localized solutions of real scalar fields. They are produced in various contexts of the early universe in, such as, the inflaton evolution and the axion evolution. However, their decay process has long been unclear. In this paper, we derive an analytic formula of the decay rate of the I-balls/oscillons within the classical field theory. In our approach, we calculate the Poynting vector of the perturbation around the I-ball/oscillon profile by solving a relativistic field equation, with which the decay rate of the I-ball/oscillon is obtained. We also perform a classical lattice simulation and confirm the validity of our analytical formula of the decay rate numerically.
citations added
References in corpus (7)
- Dilute and dense axion stars
- Quantum Radiation of Oscillons
- Flat-top oscillons in an expanding universe
- Oscillons and Quasi-breathers in the ϕ^4 Klein-Gordon model
- Analytical Characterization of Oscillon Energy and Lifetime
- Correspondence of I- and Q-balls as Non-relativistic Condensates
- No quasi-stable scalaron lump forms after inflation