S-factor

Source: Wikipedia, the free encyclopedia.

In

Coulomb repulsion between the charged reactants. It determines the rates of nuclear fusion reactions that occur in the cores of stars
.

Definition

The quantity is defined as[1]

,

where E is the energy, σ is the cross section, η is the dimensionless Sommerfeld parameter:

,

Z1 Z2 e2 is the product of the charges of the reactants, is the

permittivity of free space
, is the
reduced Planck constant and v is the relative incident velocity
.

Motivation

The Coulomb barrier causes the cross section to have a strong exponential dependence on the center-of-mass energy E. The S-factor remedies this by factoring out the Coulomb component of the cross section.

References