Dynamical Pair Production at Sub-Barrier Energies for Light Nuclei
arXiv:2207.06900 · doi:10.3390/particles5040041
Abstract
In the collision of two heavy ions, the strong repulsion coming from the Coulomb field is enough to produce pair(s) from vacuum fluctuations. The energy is provided by the kinetic energy of the ions and the Coulomb interaction at the production point. If, for instance, the electron is located at the center of mass (C.M.) of the two ions moving along the \emph{z}-axis, and the positron is at a distance \emph{x} from the electron, the ions can be accelerated towards each other since the Coulomb barrier is lowered by the presence of the electron. This screening results in an increase in the kinetic energy of the colliding ions and may result in an increase in the fusion probability of light ions above the adiabatic limit.
arXiv comment6 pages, 4 figures
References in corpus (9)
- Study of the 12C+12C fusion reactions near the Gamow energy
- Effects of mutual excitations in the fusion of carbon isotopes
- Characterizing the astrophysical S-factor for C+C with wave-packet dynamics
- Status on fusion at deep subbarrier energies: impact of resonances on astrophysical factors
- Absence of hindrance in microscopic C+C fusion study
- Calculation of the 12C+12C sub-barrier fusion cross section in an imaginary time-dependent mean field theory
- Chaos driven fusion enhancement factor at astrophysical energies
- Electron-positron vacuum instability in strong electric fields. Relativistic semiclassical approach
- Coulomb field correction due to virtual production in heavy ion collisions